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610 Sentences With "brightest star"

How to use brightest star in a sentence? Find typical usage patterns (collocations)/phrases/context for "brightest star" and check conjugation/comparative form for "brightest star". Mastering all the usages of "brightest star" from sentence examples published by news publications.

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But the brightest star in the sky is actually Sirius.
She continues to shine as the brightest star in our sky.
The planet orbits the brightest star in the system, HD 131399A.
The brightest star, Eta Carina, produces 4.7 million suns' worth of light. 
Or Mimosa, the second brightest star in the Southern Cross, or Crux.
Boat and bird are pointed towards the brightest star, whose rays are pink.
Young Tapz Young Tapz is perhaps the brightest star of the bunch right now.
It's expected to rival Sirius, the brightest star in our sky, or even Venus.
This caused it to be the second-brightest star in the sky during April 1844.
She was, one witness said, "the brightest star in the black sky of the occupation."
What was once the brightest star, and brightest light ever, just got a little dark.
As the brightest star in the night sky, Sirius was already associated with light and heat.
"He was NBC's biggest and brightest star in the '80s," says then-entertainment president Warren Littlefield.
The Aquariids take their name from the third-brightest star in the Aquarius constellation, called Delta.
Leo's brightest star, Regulus, and possibly others, will be visible to the east of the darkened sun.
If Betelgeuse does go supernova, it will be the brightest star in the sky for many months.
Once the ninth brightest star in the sky, Betelgeuse has fallen now to about the 23rd brightest.
OhnakaAntares is the brightest star in the constellation Scorpius, a red supergiant only around 555 light years away.
At 340 light-years away, it houses some of the brightest star clusters in the southern sky, too.
For example, most people believe that Polaris - or the North Star - is the brightest star in the sky.
This is the time to search for the tallest summit, and set our sights on the brightest star.
Canadian musician Peaches, possibly electroclash's brightest star, is probably the earliest antecedent to the specific late-00s electropop sound.
For almost half a century now, each has seen the other as the brightest star in the other's universe.
"GM is still the brightest star in the Mahoning Valley, but luckily we have diversified our economy," Hill said.
There's an attractively questing quality in the album's opener, "Arcturus," named after the brightest star in the Northern sky.
Regulus, the brightest star in Leo, will step out of a robe of sudden twilight over the sun's shoulder.
His films are not the most profitable, "Ghostbusters" aside, and he's not the brightest star in the Hollywood galaxy.
The arced star trails in this long-exposure shot rotate around Polaris, the brightest star in the constellation of Ursa Minor.
"; "It wasn't until I became a hen that I learned the brightest star can be born out of the greatest tragedy.
Steph Curry is the NBA's back-to-back MVP, its best point guard and the brightest star on a wildly popular team.
But when Benyamin keeps crying, she takes him to the balcony and points to the brightest star shining through Kabul's polluted sky.
For Liakopoulos's final chapter, entitled "sweet (dreams)," the brightest star is baklava swimming in a jar with ice cream and spiced syrup.
Enter Italy's brightest star and Terraforma resident Donato Dozzy, who embarks on three-hours of some of the most enthralling ambient we've ever heard.
Spitzer discovered the second-brightest star in our galaxy, the Peony nebula star (in the dusty and crowded center of this image) in 2008.
No harm in wishing upon St. John's brightest star, who, in turn, would no doubt say: Hold on, slow down, one day at a time.
Yams, born Steven Rodriguez, jump-started the career of ASAP Rocky, the Mob's brightest star, and steered him toward a sound that eschewed rap regionalism.
As it normally just looks to the naked eye like the brightest star in the sky, it's hard to pick out those phases without a telescope.
Wiiner of Stars & Nebulae: The Rainbow Star, Steve BrownSirius is the brightest star in the night sky, and it's often seen shining as a white star.
Age: 20Position: DefenderThe Dutch national team is enjoying a golden generation of talent coming through its ranks, and its brightest star is defender Matthijs de Ligt.
"One of the planets—HD 212657—orbits the brightest star known to host a planet ever found by either the Kepler or K2 missions," Mayo told Gizmodo.
Since the passing of the collective's brightest star in 2014, the remaining apostles of the late DJ Rashad have been hard at work spreading his musical gospel.
"In the 1980s when the AIDS epidemic began, Elizabeth Taylor was the brightest star in Hollywood, one of the greatest celebrities in the world," said John, 68.
Next time I look at a night sky, I'm guessing the brightest star I see glittering is my friend and funny, mystery-solving gang member, Casey. Zoinks!!!!
At just 18, he played an integral role in the bebop revolution in the late 1940s, becoming the regular sideman for the art's brightest star, Charlie Parker.
The brightest star of the 2016 postseason hasn't been MVP candidate Kris Bryant, future Rookie off the Year Corey Seager or potential Cy Young award winner Corey Kluber.
The satellites can even "flare," briefly boosting their brightness to rival that of Sirius, the brightest star in the sky, when their solar panels are oriented just right.
Although not as bright as Venus, Jupiter is a dazzling object in its own right, shining nearly eight times brighter than  Arcturus , the brightest star of the summer sky.
The brightest star in the Leo constellation is Regulus—the heart of the lion—and when it's highlighted in someone's birth chart, it can bring fame, royalty, and courage.
Dr. Meech said the astronomers were initially excited when the orbit appeared to point to the brightest star in Lyra, Vega, which is known to have a debris disk.
The two other stars in the system also orbit the brightest star, circling one another like a dumbbell and exerting their gravitational influence over the planet, named HD 131399Ab.
The planet orbits the brightest star in the system, HD 131399A / Image/caption courtesy of ESO HD 131399Ab is particularly unique because it's one of very few directly imaged exoplanets.
During this year's event, as a bonus, the moon will also interrupt the light from Regulus, the brightest star in the constellation Leo, a few hours after it passes Venus.
And, of course, Cynthia Erivo cemented her status as a soon-to-be legend as Celie from "The Color Purple," shining as the brightest star in a segment that included Oprah.
"I think you are the brightest star I have ever met in so many ways, but something is missing," the Canadian firefighter tells Loch, expressing that he's only "80 percent" into their relationship.
Using ESO&aposs Very Large Telescope, a team of researchers from the University of Oxford detected exceptionally massive stars in  30 Doradus , which is the brightest star-forming region in our galactic neighborhood.
As the June California primary nears, tourists and vandals alike now flock to the brightest star -- or dimmest light, depending on your politics -- on the international attraction known as the Hollywood Walk of Fame.
Rigel, Orion's brightest star, shimmers its blue-white light, the twinkle in the eye (the knee, actually) of a companion who has visited me, annually, every place on Earth I have lived since childhood.
It's the only moment throughout the movie in which she gets to shine as the brightest star in a city full of twinkling talent, and both Stone and Mia grab the opportunity with both hands.
Justina Machado stars as Penelope — sometimes Lupe, sometimes Lupita — a single mom, nurse and veteran raising two children with the help of her widowed, immigrant mother, Lydia (Rita Moreno, the brightest star in our solar system).
As Democrats rallied to capture several seats in Southern California during the midterms, many Republicans saw the brightest star in Ms. Kim, who routinely mentions her experiences as a Korean-American immigrant and mother of four.
The planet orbits the brightest star in the system, HD 131399A / Image/caption courtesy of ESO This graphic shows the orbit of the planet in the HD 131399 system (red line) and the orbits of the stars (blue lines).
But the brightest star of the constellation is Raul Labrador, one of the most conservative members of the US House — who recently announced his intention to run for Idaho governor and has spent considerable time courting the Central Committee's endorsement.
"The brightest star at Fox News, Megyn Kelly is a newly minted role model for women who sees her gender as irrelevant, and a conservative champion who transcends politics with her skillful skewering of windbags of both parties," the profile states.
Christian Pulisic, the team's brightest star, strongly hinted after a game in London last month that the team needed some direction after more than a year under Sarachan, a longtime Arena assistant but never a serious candidate for the permanent post.
The teams scored a combined 123 points as two of the league's brightest star quarterbacks — Jared Goff of the Rams and Patrick Mahomes of the Chiefs — swapped big play after big play, combining for more than 212,277 yards of offense.
"  He concluded with a call to "reignite the American imagination… search for the tallest summit, set our sights on the brightest star… and rekindle the bonds of love and loyalty and memory that link us together as citizens as neighbors and patriots.
Its brightest star, Sirius, and possibly others, will appear to the west of the eclipsed sun near the Orion constellation for the west and central US. This constellation will dip below the horizon by the time the total eclipse is visible on the East Coast.
The NBA draft is unpredictable by nature, but given the depth, talent, youth, and hype surrounding this year's crop, identifying the best player right now is a lot different than predicting who will be seen as the brightest star a few years down the road.
Where and when to look for shooting starsSince the constellation of Aquarius (and, more specifically, the star Delta, the third brightest star within that, which this meteor shower is named after) is low in the southern sky as seen from the northern hemisphere, it's best to look generally to the south.
While the market that online lending companies are chasing is enormous — the U.S. consumer lending market is a $3.5 trillion business — many investors see the sector as overheated, particularly after the surprise ouster in May of Renaud Laplanche, the founder and CEO of what was long the industry's brightest star, LendingClub.
Sirius, the brightest star of all to the eye, just now making its presence known in the winter sky, also goes by the names of the Dog Star, Aschere, Canicula, Al Shira, Sothis, Alhabor, Mrgavyadha, Lubdhaka and Tenrōsei, as well as Alpha Canis Majoris, after its constellation, Canis Major, the big dog.
Mr. Makavejev was, as The Nation once put it, "the brightest star in the avant-garde firmament" in the early 1970s, thanks to movies like "Man Is Not a Bird" (1965), "Innocence Unprotected" (1968) and especially "WR: Mysteries of the Organism," a brash hodgepodge that was a darling of the 19903 Cannes Film Festival.
During an interview on the Russian radio program Moscow Speaking earlier this week, Dmitry Nosov, a member of Russia's lower parliamentary house, the State Duma, made a pitch to Conor McGregor urging the UFC featherweight champion and pound-for-pound brightest star in the MMA firmament to drop his beloved Ireland and become a Russian citizen.
In the J band Sirius is the 9th brightest star.
It is the brightest star of class O in the night sky.
POX 186 appears near the star Spica, the brightest star in Virgo.
Conon, Narrations, 8Strabo, Geography, 17. 1. 17 Also named for Canopus is Canopus, the brightest star in the southern constellation of Carina (the keel of the ship Argo), and the second-brightest star in the night sky, after Sirius.
The car was named for Vega, the brightest star in the constellation Lyra.
In 2014 the group recorded a Christmas song with Vekora: "The Brightest Star".
In February 2019, the asteroid occulted the brightest star in the night sky, Sirius.
The Rigel missile was named after Rigel, the brightest star in the constellation Orion.
Wide-field view of the Summer Triangle and the Milky Way. Deneb is at the left-centre of the picture.Names similar to Deneb have been given to at least seven different stars, most notably Deneb Kaitos, the brightest star in the constellation of Cetus; Deneb Algedi, the brightest star in Capricornus; and Denebola, the second brightest star in Leo. All these stars are referring to the tail of the animals that their respective constellations represent.
Vega is the brightest star in the northern constellation of Lyra. It has the Bayer designation α Lyrae, which is Latinised to Alpha Lyrae and abbreviated Alpha Lyr or α Lyr. This star is relatively close at only 25 light-years from the Sun, and, together with Arcturus and Sirius, one of the most luminous stars in the Sun's neighborhood. It is the fifth-brightest star in the night sky, and the second-brightest star in the northern celestial hemisphere, after Arcturus.
Bellatrix , designation γ Orionis (Latinized to Gamma Orionis, abbreviated to Gamma Ori, γ Ori), is the third-brightest star in the constellation of Orion, 5° west of the red supergiant Betelgeuse (Alpha Orionis). With a slightly variable magnitude of around 1.6, it is about the 25th-brightest star in the night sky.
In October 2017, Payne released his second solo album, 'Mountain' with singles 'The Brightest Star' and 'Hold Steady The Wire'.
It can be easily found through its brightest star, Spica.The history of the star: Spica by Richard Hinckley Allen, 1889.
He added pi and rho, not using xi and omicron as Bayer used these letters to denote Cygnus and Hercules on his map. The brightest star in the constellation is Vega (Alpha Lyrae), a main-sequence star of spectral type A0Va. Only 7.7 parsecs distant, Vega is a Delta Scuti variable, varying between magnitudes −0.02 and 0.07 over 0.2 days. On average, it is the second- brightest star of a northern hemisphere (after Arcturus) and the fifth- brightest star in all, surpassed only by Arcturus, Alpha Centauri, Canopus, and Sirius.
349.) Its brightest star was Beta Carinae (β Car) or Miaplacidus, which was known as α Roburis or α Roburis Carolii.
Fomalhaut is the third-brightest star (as viewed from Earth) known to have a planetary system, after the Sun and Pollux.
Beta Leporis (β Leporis, abbreviated Beta Lep, β Lep), formally named Nihal , is the second brightest star in the constellation of Lepus.
A bright nova was observed in Aquila in 1918 (Nova Aquilae 1918) and briefly shone brighter than Altair, the brightest star in Aquila.
HD 143183 lies approximately 1' from the 10th-magnitude O-class bright giant CD-53 6363, the second-brightest star in the cluster.
Greek letters are used to denote the brighter stars within each of the eighty-eight constellations. In most constellations, the brightest star is designated Alpha and the next brightest Beta etc. For example, the brightest star in the constellation of Centaurus is known as Alpha Centauri. For historical reasons, the Greek designations of some constellations begin with a lower ranked letter.
In his Uranometria, Johann Bayer used the Greek letters Alpha through to Omega and then A to k to label what he saw as the most prominent 35 stars in the constellation, with subsequent astronomers splitting Kappa, Mu, Nu and Pi as two stars each. Nu is also the same star as Psi Herculis. John Flamsteed numbered 54 stars for the constellation. Located 36.7 light-years from Earth, Arcturus, or Alpha Boötis, is the brightest star in Boötes and the fourth-brightest star in the sky at an apparent magnitude of −0.05; It is also the brightest star north of the celestial equator, just shading out Vega and Capella.
Rigel is one of the brightest stars in the sky, usually the brightest star in the constellation Orion. It is frequently mentioned in works of fiction.
NGC 206 is a bright star cloud in the Andromeda Galaxy. It is notable for being the brightest star cloud in Andromeda as viewed from Earth.
Alpha Ophiuchi (α Ophiuchi, abbreviated Alpha Oph, α Oph), also named Rasalhague ,also or . is a binary star and the brightest star in the constellation of Ophiuchus.
Canis Major contains Sirius, the brightest star in the night sky, known as the "dog star". It is bright because of its proximity to the Solar System. In contrast, the other bright stars of the constellation are stars of great distance and high luminosity. At magnitude 1.5, Epsilon Canis Majoris (Adhara) is the second-brightest star of the constellation and the brightest source of extreme ultraviolet radiation in the night sky.
Epsilon, Omicron2, Delta, and Eta Canis Majoris were called Al Adzari "the virgins" in medieval Arabic tradition. Marking the dog's right thigh on Bayer's atlas is Epsilon Canis Majoris, also known as Adhara. At magnitude 1.5, it is the second-brightest star in Canis Major and the 23rd-brightest star in the sky. It is a blue-white supergiant of spectral type B2Iab, around 404 light-years from Earth.
Deneb () is a first-magnitude star in the constellation of Cygnus, the swan. Deneb is one of the vertices of the asterism known as the Summer Triangle and the "head" of the Northern Cross. It is the brightest star in Cygnus and the 19th brightest star in the night sky, with an average apparent magnitude of +1.25. A blue-white supergiant, Deneb rivals Rigel as the most luminous first magnitude star.
Some accounts have Crow ultimately leaving the earth altogether, having been called up into the heavens where he became Canopus, the second-brightest star in the night sky.
Alpha Phoenicis (α Phoenicis, abbreviated Alpha Phe or α Phe), formally named Ankaa (distinguish Ancha, with the same pronunciation) is the brightest star in the constellation of Phoenix.
Alpha Aurigae (Capella), the brightest star in Auriga, is a G8III class star (G-type giant) 43 light-years away and the sixth-brightest star in the night sky at magnitude 0.08. Its traditional name is a reference to its mythological position as Amalthea; it is sometimes called the "Goat Star". Capella's names all point to this mythology. In Arabic, Capella was called al-'Ayyuq, meaning "the goat", and in Sumerian, it was called mul.
Hamal , designation Alpha Arietis (α Arietis, abbreviated Alpha Ari, α Ari), is the brightest star in the northern zodiacal constellation of Aries. With an apparent visual magnitude of 2.0, it is the mean 50th brightest star in the night sky. Based upon parallax measurements made with the Hipparcos astrometry satellite, Hamal is about from Earth. It is a giant star that may host an orbiting planet with a mass greater than Jupiter.
HD 91312 (HR 4132, HIP 51658) is a star in the constellation Ursa Major. Its apparent magnitude is 4.73. It is the brightest star of Ursa Major without Flamsteed designation.
In medieval Muslim astronomy, Orion was known as al-jabbar, "the giant". Orion's sixth brightest star, Saiph, is named from the Arabic, saif al-jabbar, meaning "sword of the giant".
The Alcyone name comes from the brightest star in the Pleiades star cluster, on which the Subaru logo is based. The XT range was replaced by the Subaru SVX in 1992.
NGC 5999 is an open cluster in the constellation Norma. Its brightest star is HIP 78355. It is 5310 light-years distant and thought to be around 400 million years old.
Beta Arietis (β Arietis, abbreviated Beta Ari, β Ari), officially named Sheratan , is a star system and the second-brightest star in the constellation of Aries, marking the ram's second horn.
In Chinese astronomy, Arcturus is called Da Jiao (), because it is the brightest star in the Chinese constellation called Jiao Xiu (). Later it became a part of another constellation Kang Xiu ().
Beta Carinae (Latinised from β Carinae, abbreviated Beta Car, β Car), officially named Miaplacidus , is the second-brightest star in the constellation of Carina and one of the brightest stars in the night sky, with apparent magnitude 1.68. It is the brightest star in the southern asterism known as the Diamond Cross, marking the southwestern end of the asterism. It lies near the planetary nebula IC 2448. Parallax measurements place it at a distance of from the Sun.
Betelgeuse is usually the tenth-brightest star in the night sky and, after Rigel, the second-brightest in the constellation of Orion. It is a distinctly reddish semiregular variable star whose apparent magnitude, varying between +0.0 and +1.6, has the widest range displayed by any first-magnitude star. At near-infrared wavelengths, Betelgeuse is the brightest star in the night sky. Its Bayer designation is α Orionis, Latinised to Alpha Orionis and abbreviated Alpha Ori or α Ori.
Alpha Trianguli Australis, known as Atria, is a second-magnitude orange giant and the brightest star in the constellation, as well as the 42nd-brightest star in the night sky. Completing the triangle are the two white main sequence stars Beta and Gamma Trianguli Australis. Although the constellation lies in the Milky Way and contains many stars, deep-sky objects are not prominent. Notable features include the open cluster NGC 6025 and planetary nebula NGC 5979.
Alpha Coronae Australis (α Coronae Australis, abbreviated Alf CrA, α CrA), officially named Meridiana , is the brightest star in the constellation of Corona Australis and is located about 125 light-years from Earth.
Bradley's discovery confirmed Copernicus' theory that the Earth revolved around the Sun. In 1.5 million years, Gamma Draconis will pass within 28 light years of Earth. For a period, if its current absolute magnitude does not change, it will be the brightest star in the night sky, nearly as bright as Sirius is at present. It is by far the brightest star having a zenith above a point near London which led to its vaunting in these places as the "zenith star".
Dutch painting in the seventeenth century. 2nd edition. Westview Press; pp. 94–95. Another readily identifiable constellation is Leo, above the Holy Family, with its brightest star, Regulus, in the centre of the picture.
The brightest star of the cluster is a K5 III giant star, with 7.1 magnitude, but its membership is questionable. One more 7.9 magnitude star is visible at the north edge of the cluster.
Alpha Ceti (α Ceti, abbreviated Alpha Cet, α Cet), officially named Menkar , is the second-brightest star in the constellation of Cetus. It is a cool luminous red giant about 250 light years away.
"He was the true king of our storytellers, the brightest star that flashed upon our skies" - Upton Sinclair, Author of The JungleBack cover of the Penguin book released in conjunction with the series broadcast.
It is now obsolete. Its brightest star, HD 85951, was named Felis by the International Astronomical Union on 1 June 2018 and it is now so included in the List of IAU-approved Star Names.
Brightest Star is the debut mini-album from J-pop vocal group Bright. This was their first CD released under major label Rhythm Zone. The album ranked weekly on the Oricon chart at No. 133.
Capella , designated α Aurigae (Latinized to Alpha Aurigae, abbreviated Alpha Aur, α Aur), is the brightest star in the constellation of Auriga, the sixth- brightest star in the night sky, and the third-brightest in the northern celestial hemisphere after Arcturus and Vega. A prominent object in the northern winter sky, it is circumpolar to observers north of 44°N. Its name meaning "little goat" in Latin, Capella depicted the goat Amalthea that suckled Zeus in classical mythology. Capella is relatively close, at from the Sun.
Its traditional name means "the southern claw". Zubeneschamali (Beta Librae) is the corresponding "northern claw" to Zubenelgenubi. The brightest star in Libra, it is a green-tinged star of magnitude 2.6, 160 light-years from Earth.
The all female Platoon. Named after the blue giant Spica star, which holds the title of being the brightest star in the Virgo constellation. It is another main Platoon in the series. Their engine is Flame Swallow.
Canopus , also designated α Carinae, Latinised to Alpha Carinae, is the brightest star in the southern constellation of Carina and the second- brightest star in the night sky. With a visual apparent magnitude of −0.74, it is outshone only by Sirius. Located around from the Sun, Canopus is a bright giant of spectral type A9, so it is essentially white when seen with the naked eye. It has a luminosity over 10,000 times the luminosity of the Sun, is eight times as massive, and has expanded to 71 times the Sun's radius.
Nebulosity is visible to the north and east of the cluster, which is 7 arcminutes in diameter. The brightest star appears in the eastern part of the cluster and is of the 7th magnitude; another bright star has a yellow hue. Dolidze 11 is an open cluster 400 million years old, farthest away of the three at 3700 light-years. More than 10 stars are visible in an amateur instrument in this cluster, of similar size to Dolidze 9 at 7 arcminutes in diameter, whose brightest star is of magnitude 7.5.
Altair , designated α Aquilae (Latinised to Alpha Aquilae, abbreviated Alpha Aql, α Aql), is the brightest star in the constellation of Aquila and the twelfth brightest star in the night sky. It is currently in the G-cloud—a nearby interstellar cloud, an accumulation of gas and dust. Altair is an A-type main sequence star with an apparent visual magnitude of 0.77 and is one of the vertices of the Summer Triangle asterism (the other two vertices are marked by Deneb and Vega).Summer Triangle, entry, The Internet Encyclopedia of Science, David Darling.
VEGA is an English rock band. They were formed in 2009 and have released six albums to date, with their most recent released in June 2020. VEGA are named after the fifth-brightest star in the night sky.
The Second Brightest Star is the eleventh studio album by the English progressive rock band Big Big Train. It contains a mix of new songs along with re-worked material from the band's previous two albums, Folklore and Grimspound.
Procyon (top left), Betelgeuse (top right), and Sirius (bottom) form the Winter Triangle. Orion is to the right. Viewed from Northern Hemisphere. Procyon is usually the eighth-brightest star in the night sky, culminating at midnight on 14 January.
Despite the division, Lacaille kept Argo's Bayer designations. Therefore, Carina has the Alpha, Beta and Epsilon originally assigned to Argo Navis, while Vela's brightest stars are Gamma and Delta, Puppis has Zeta as its brightest star, and so on.
His family name was originally Boyron. His father and mother were leading players. He was born in Paris. He was orphaned at age 9, and joined the child company Petits Comédiens Dauphins at age 12, becoming its brightest star.
Lambda Scorpii (Latinised from λ Scorpii, abbreviated Lambda Sco, λ Sco), formally named Shaula , is, despite being designated "λ" (Lambda), the second- brightest star system in the constellation of Scorpius, and one of the brightest stars in the night sky.
The third-brightest star is 21 Leonis Minoris, a rapidly rotating white main-sequence star of average magnitude 4.5. The constellation also includes two stars with planetary systems, two pairs of interacting galaxies, and the unique deep-sky object Hanny's Voorwerp.
A line from Sirius, the brightest star in the sky, through Canopus, the second-brightest, continued for the same distance lands within a couple of degrees of the pole. In other words, Canopus is halfway between Sirius and the pole.
It has a diameter of roughly 400 solar diameters. The secondary, a spectroscopic binary that orbits the primary every 3600 years, is a blue-green hued star of magnitude 5.6. Beta Herculis, also called Kornephoros, is the brightest star in Hercules.
A primary star, which is brighter and typically bigger than its companion stars, is designated by a capitalized A. Its companions are labelled B, C, and so on. For example, Sirius, the brightest star in the sky, is actually a double star, consisting of the naked- eye visible Sirius A and its dim white-dwarf companion Sirius B. The first exoplanet tentatively identified around the second brightest star in the triple star system Alpha Centauri is accordingly called Alpha Centauri Bb. If an exoplanet orbits both of the stars in a binary system, its name can be, for example, Kepler-34(AB) b.
Aldebaran is the brightest star in the constellation of Taurus (center). The traditional name Aldebaran derives from the Arabic al Dabarān ("الدبران"), meaning "the follower", because it seems to follow the Pleiades. In 2016, the International Astronomical Union Working Group on Star Names (WGSN) approved the proper name Aldebaran for this star. Aldebaran is the brightest star in the constellation Taurus and so has the Bayer designation α Tauri, Latinised as Alpha Tauri. It has the Flamsteed designation 87 Tauri as the 87th star in the constellation of approximately 7th magnitude or brighter, ordered by right ascension.
Another visible ternary is Alpha Centauri, in the southern constellation of Centaurus, which contains the fourth-brightest star in the night sky, with an apparent visual magnitude of −0.01. This system also underscores the fact that no search for habitable planets is complete if binaries are discounted. Alpha Centauri A and B have an 11 AU distance at closest approach, and both should have stable habitable zones. There are also examples of systems beyond ternaries: Castor is a sextuple star system, which is the second-brightest star in the constellation Gemini and one of the brightest stars in the nighttime sky.
Each NASA flight director is allowed to choose a symbol or color to represent his or her team. Heflin chose to call his team Sirius. It is the brightest star in the heavens, and is sometimes referred to as the "dog" star.
Old Man of the South Pole on painted ceramic The Old Man of the South Pole (in or ) is the Taoist deification of Canopus, the brightest star of the constellation Carina. It is the symbol of happiness and longevity in Far Eastern culture.
Brightest Star (also titled Light Years) is a 2013 American independent romantic comedy film directed by Maggie Kiley and starring Chris Lowell and Rose McIver. The film is based on Kiley's short film Some Boys Don't Leave. It is also Kiley's directorial debut.
Zeta Ophiuchi (ζ Oph, ζ Ophiuchi) is a star located in the constellation of Ophiuchus. It has an apparent visual magnitude of 2.57, making it the third- brightest star in the constellation. Parallax measurements give an estimated distance of roughly from the Earth.
Alphard , designated Alpha Hydrae (α Hydrae, abbreviated Alpha Hya, α Hya), is the brightest star in the constellation of Hydra. It is a single giant star, cooler than the sun but larger and more luminous. It is about 177 light years away.
Two bright stars Phi Cassiopeiae (magnitude 5) and HD 7902 (magnitude 7) can be imagined as eyes. The next brightest star is the red supergiant variable star V466 Cassiopeiae. The cluster features a rich field of about 150 stars of magnitudes 9-13.
NGC 3572 plus nebulosity. V533 Car is the brightest star in the frame, on the right (south is up). V533 Carinae is a bright supergiant with a luminosity around 100,000 times that of the sun. The temperature is over 8,000 K and the radius around .
It is found in a region often called the Sea due to its profusion of constellations with watery associations such as Cetus the whale, Pisces the fish, and Eridanus the river. At apparent magnitude 2.9, Beta Aquarii is the brightest star in the constellation.
The brightest star, is a young A-type main-sequence star, and further out are two lower-mass stars. A Jupiter-mass planet or a low-mass brown dwarf was once thought to be orbiting the central star, but this has been ruled out.
Electra , designated 17 Tauri, is a blue-white giant star in the constellation of Taurus. It is the third-brightest star in the Pleiades open star cluster (M45); the most visible stars in this group are named for the Seven Sisters of Greek mythology.
Vega Platoon consists solely of men. Named after the Vega star, which is the brightest star in the Lyra constellation and the fifth-brightest star at night. One of the main platoons of Season 1, their engine is the Iron Burger, which is loosely based on the Pennsylvania Railroad S1 6-4-4-6 steam locomotive designed by Raymond Loewy, but has the same 4-8-8-4 wheel arrangement as Big One. The engine was destroyed and the members were killed at the end of Season 1, during the Alfort Armada's invasion of the Galaxy Railways, after they brought the Gustav Cannons to Big One's aid.
With an apparent visual magnitude of −0.05, Arcturus is the brightest star in the northern celestial hemisphere and the fourth-brightest star in the night sky, after Sirius (−1.46 apparent magnitude), Canopus (−0.72) and α Centauri (combined magnitude of −0.27). However, α Centauri AB is a binary star, whose components are both fainter than Arcturus. This makes Arcturus the third-brightest individual star, just ahead of α Centauri A (officially named Rigil Kentaurus), whose apparent magnitude . The French mathematician and astronomer Jean-Baptiste Morin observed Arcturus in the daytime with a telescope in 1635, a first for any star other than the Sun and supernovae.
Aldebaran , designated α Tauri (Latinized to Alpha Tauri, abbreviated Alpha Tau, α Tau), is an orange giant star measured to be about 65 light-years from the Sun in the zodiac constellation Taurus. It is the brightest star in Taurus and generally the fourteenth-brightest star in the night sky, though it varies slowly in brightness between magnitude 0.75 and 0.95. Aldebaran is believed to host a planet several times the mass of Jupiter, named . Aldebaran is a red giant, cooler than the sun with a surface temperature of , but its radius is about 44 times the sun's, so it is over 400 times as luminous.
Supergiants are rare and short-lived stars, but their high luminosity means that there are many naked- eye examples, including some of the brightest stars in the sky. Rigel, the brightest star in the constellation Orion is a typical blue-white supergiant; Deneb is the brightest star in Cygnus, a white supergiant; Delta Cephei is the famous prototype Cepheid variable, a yellow supergiant; and Betelgeuse, Antares and UY Scuti are red supergiants. μ Cephei is one of the reddest stars visible to the naked eye and one of the largest in the galaxy. Rho Cassiopeiae, a variable, yellow hypergiant, is one of the most luminous naked- eye stars.
'Agojo so'jo (Tewa: 'Big star') is a god in Native American Tewa mythology. He represents the Morning star, the brightest star in the morning. 'Agojo so'jo was the husband of the Evening Star. They were once mortals, but when the Evening Star died, 'agojo so'jo pursued her.
The constellation Scutum as it can be seen by the naked eye. The constellation Scutum in the night sky, enhanced for color and contrast. Scutum is not a bright constellation, with the brightest star, Alpha Scuti, at magnitude 3.85. But some stars are notable in the constellation.
Epsilon Microscopii is radiating about 36 times the Sun's luminosity from its photosphere at an effective temperature of 9,126 K. Epsilon Microscopii was a latter designation of 4 Piscis Austrini. This star was the brightest star in Globus Aerostaticus, the obsolete constellationIan Ridpath's Star Tales - Globus Aerostaticus.
This was first noticed by William Herschel in 1783, although in his first calculation he identified this point with Lambda Herculis. It will eventually become the brightest star in the sky in approximately 3 million years from today, at -0.4, slightly less bright than Canopus today.
Alpha Corvi (α Corvi, abbreviated Alpha Crv, α Crv), also named Alchiba , is an F-type main-sequence star and the fifth-brightest star in the constellation of Corvus. Based on parallax measurements made during the Hipparcos mission, it is approximately 49 light-years from the Sun.
Beta Corvi (β Corvi, abbreviated Beta Crv, β Crv), officially named Kraz , is the second-brightest star in the southern constellation of Corvus with an apparent visual magnitude of 2.647. Based on parallax measurements obtained during the Hipparcos mission, it is about distant from the Sun.
Alpha Gruis, Latinized from α Gruis, officially named Alnair , is a single star in the southern constellation of Grus. At magnitude 1.7 it is the brightest star in Grus and one of the brightest stars in the sky. It is a B-type main-sequence star away.
Beta Pegasi (β Pegasi, abbreviated Beta Peg, β Peg), formally named Scheat , is a red giant star and the second-brightest star (after Epsilon Pegasi) in the constellation of Pegasus. It forms the upper right corner of the Great Square of Pegasus, a prominent rectangular asterism.
Atria, the brightest star of the Southern Triangle, is always moving and has variable magnitude. The star's characteristics represent why it was chosen as a symbol of the organization, which focuses on "both the inequality and the variability of the relationship between men and women in society".
Eta Corvi (Eta Crv, η Corvi, η Crv) is an F-type main-sequence star, the sixth-brightest star in the constellation of Corvus. Two debris disks have been detected orbiting this star, one at ~150 AU, and a warmer one within a few astronomical units (AU).
The Platoon of the main characters. Named after the brightest star in the night, it is the main Platoon in the series. Their engine is Big One, which is based on the Union Pacific Railroad's 4-8-8-4 Big Boy locomotives, the largest steam locomotives ever built.
Beta Delphini (β Delphini, abbreviated Beta Del, β Del) is a binary star in the constellation of Delphinus. It is the brightest star in Delphinus. The two components of the system are designated Beta Delphini A (officially named Rotanev , which is historically the name of the system) and B.
In the image at the right, 2MASX J00403079-1353088 is the edge-on galaxy directly below the brightest star in the image. It is possibly a satellite of NGC 210, but without a redshift to determine its distance, it could just as possibly be completely unrelated to NGC 210.
The cluster and association lie in the neighboring Sagittarius Arm of the Milky Way. Zeta1 Scorpii (spectral type O8 and magnitude 4.71.Sky Catalogue 2000.0) is the brightest star in the association, and one of the most radiant stars known in the galaxy.Crossen & Tirion, Binocular Astronomy, p. 119.
The North America Nebula (NGC 7000 or Caldwell 20) is an emission nebula in the constellation Cygnus, close to Deneb (the tail of the swan and its brightest star). The shape of the nebula resembles that of the continent of North America, complete with a prominent Gulf of Mexico.
NGC 2439, with R Puppis the brightest star R Puppis (R Pup) is a variable star in the constellation Puppis. It is a rare yellow hypergiant and a candidate member of the open cluster NGC 2439. It is also an MK spectral standard for the class G2 0-Ia.
Canopus has persistently been the brightest star over the ages; other stars appear brighter only during relatively temporary periods, during which they are passing the Solar System at a much closer distance than Canopus. Working out exactly which stars were or will be the brightest at any given point in the past or future is difficult since it requires precise 3D proper motions of large numbers of stars and precise distances. This information only started to become available with the 1997 Hipparcos satellite data release. Jocelyn Tomkin used this data to compile a list of brightest star in Earth's night sky at each period within the last or next 5 million years.
Ankaa is the brightest star in the constellation. It is an orange giant of apparent visual magnitude 2.37 and spectral type K0.5IIIb, 77 light years distant from Earth and orbited by a secondary object about which little is known. Lying close by Ankaa is Kappa Phoenicis, a main sequence star of spectral type A5IVn and apparent magnitude 3.90. Located centrally in the asterism, Beta Phoenicis is the second brightest star in the constellation and another binary star. Together the stars, both yellow giants of spectral type G8, shine with an apparent magnitude of 3.31, though the components are of individual apparent magnitudes of 4.0 and 4.1 and orbit each other every 168 years.
Within the constellation's borders, there are 47 stars brighter than or equal to apparent magnitude 6.5. Traditionally representing the mouth of the fish, Fomalhaut is the brightest star in the constellation and the 19th brightest star in the night sky, with an apparent magnitude of 1.16. Located 25.13 ± 0.09 light- years away, it is a white main sequence star that is 1.92 ± 0.02 times as massive and 16.63±0.48 as luminous as the Sun. Its companion Fomalhaut b was thought to be the first extrasolar planet ever detected by a visible light image, thanks to the Hubble Space Telescope, but infrared observations have since retracted this claim: it is instead a spherical cloud of dust.
Epsilon Ursae Majoris (Latinised from ε Ursae Majoris, abbreviated Epsilon UMa, ε UMa), officially named Alioth , is, despite being designated "ε" (epsilon), the brightest star in the constellation of Ursa Major, and at magnitude 1.77 is the thirty-second brightest star in the sky. It is the star in the tail of the bear closest to its body, and thus the star in the handle of the Big Dipper (or Plough) closest to the bowl. It is also a member of the large and diffuse Ursa Major moving group. Historically, the star was frequently used in celestial navigation in the maritime trade, because it is listed as one of the 57 navigational stars.
Eta Carinae and Carina Nebula in the constellation of Carina As a 4th-magnitude star, Eta Carinae is comfortably visible to the naked eye in all but the most light-polluted skies in inner city areas according to the Bortle scale. Its brightness has varied over a wide range, from the second- brightest star in the sky at one point in the 19th century to well below naked eye visibility. Its location at around 60°S in the far Southern Celestial Hemisphere means it cannot be seen by observers in Europe and much of North America. Located between Canopus and the Southern Cross, Eta Carinae is easily pinpointed as the brightest star within the large naked eye Carina Nebula.
Epsilon Leonis (ε Leo, ε Leonis) is the fifth-brightest star in the constellation Leo, consistent with its Bayer designation Epsilon. It is known as Algenubi or Ras Elased Australis. Both names mean "the southern star of the lion's head". Australis is Latin for "southern" and Genubi is Arabic for "south".
46 Leonis Minoris (abbreviated 46 LMi), formally named Praecipua , is the brightest star in the constellation of Leo Minor. It is of spectral class K0+III-IV and of magnitude 3.83. It is a red clump giant. Based upon parallax measurements, its distance from the Sun is approximately 95 light-years.
Leo I is located only 12 arc minutes from Regulus, the brightest star in the constellation. For that reason, the galaxy is sometimes called the Regulus Dwarf. Scattered light from the star makes studying the galaxy more difficult, and it was not until the 1990s that it was detected visually.
Aries has three prominent stars forming an asterism, designated Alpha, Beta, and Gamma Arietis by Johann Bayer. Alpha (Hamal) and Beta (Sheratan) are commonly used for navigation. There is also one other star above the fourth magnitude, 41 Arietis (Bharani). α Arietis, called Hamal, is the brightest star in Aries.
Alpha Doradus is a blue-white star of magnitude 3.3, 176 light-years from Earth. It is the brightest star in Dorado. Beta Doradus is a notably bright Cepheid variable star. It is a yellow-tinged supergiant star that has a minimum magnitude of 4.1 and a maximum magnitude of 3.5.
Alpha Trianguli Australis (Latinised from α Trianguli Australis, abbreviated Alpha TrA, α TrA), officially named Atria , is the brightest star in the southern constellation of Triangulum Australe, forming an apex of a triangle with Beta Trianguli Australis and Gamma Trianguli Australis that gives the constellation its name (Latin for southern triangle).
It is radiating 304 times the Sun's luminosity from its enlarged photosphere at an effective temperature of 4,410 K. It was also known to be part of a much bigger constellation named Telescopium Herschelii. It was also the constellation's brightest star before it was unrecognized by the International Astronomical Union (IAU).
The three brightest stars—Alpha, Beta and Nu Fornacis—form a flattened triangle facing south. With an apparent magnitude of 3.91, Alpha Fornacis is the brightest star in Fornax. Six star systems have been found to have exoplanets. The Fornax Dwarf galaxy is a small faint satellite galaxy of the Milky Way.
The Brightest Star in the Sky () is a 2019 Chinese web series starring Huang Zitao and Janice Wu. It is a coming-of-age story featuring love, friendship, and music, set in the backdrop of the musical industry. It aired on Tencent, iQiyi, and Youku from March 25 to May 6, 2019.
Its age is estimated at 10 million years, as its five hottest stars are all giants of spectral class B0. The Night Sky Observer's Guide gives the apparent brightness of the brightest star as 8.59 visual magnitudes. The absolute magnitude may be an impressive -8.2 mag, or a luminosity of 160,000 Suns.
Gamma Doradus (Gamma Dor, γ Doradus, γ Dor) is the third-brightest star in the constellation of Dorado.Gamma Dor , Jim Kaler, Stars. Accessed on line November 17, 2008. It has an apparent visual magnitude of approximately 4.25 and is a variable star, the type star of the class of Gamma Doradus variables.
Delta Aquarii (δ Aquarii, abbreviated Delta Aqr, δ Aqr), officially named Skat , is the third-brightest star in the constellation of Aquarius. The apparent visual magnitude is 3.3, which can be seen with the naked eye. The distance to this star is about based upon parallax measurements, and it has a close companion.
Alpha Vulpeculae (α Vulpeculae, abbreviated Alpha Vul, α Vul), officially named Anser , is the brightest star in the constellation of Vulpecula. It is approximately 297 light-years from Earth. It forms a wide optical binary with 8 Vulpeculae. Alpha Vulpeculae is a red giant of spectral class M1 and has apparent magnitude +4.4.
Zeta Persei is the third-brightest star in the constellation at magnitude 2.86. Around 750 light-years from Earth, it is a blue-white supergiant 26–27 times the radius of the Sun and 47,000 times its luminosity. It is the brightest star (as seen from Earth) of a moving group of bright blue-white giant and supergiant stars, the Perseus OB2 Association or Zeta Persei Association. Zeta is a triple star system, with a companion blue- white main sequence star of spectral type B8 and apparent magnitude 9.16 around 3,900 AU distant from the primary, and a white main sequence star of magnitude 9.90 and spectral type A2, some 50,000 AU away, that may or may not be gravitationally bound to the other two.
Vivian E. Robson notes that many of the traditional constellations outside of the zodiac constellations occupy large degrees of arc and typically compass several of the tropical zodiac signs. Ptolemy referred to stars by reference to the anatomy or parts of the constellations in which they appeared; thus Arcturus he named the "right knee of Boötes". Most of the Western names of stars, such as Algol or Betelgeuse, are Arabic in origin. In 1603 the Augsburg lawyer-uranographer Johann Bayer introduced the current classificatory system for the brighter stars, in which stars are identified as belonging to their constellations by Greek letters, in (roughly) descending order of brightness; so that Regulus, brightest star in Leo, is called α Leonis, the brightest star of the Lion.
Beta Ursae Minoris (β Ursae Minoris, abbreviated Beta UMi, β UMi), formally named Kochab , is the brightest star in the bowl of the Little Dipper asterism (which is part of the constellation of Ursa Minor), and only slightly fainter than Polaris, the northern pole star and brightest star in Ursa Minor. Kochab is 16 degrees from Polaris and has an apparent visual magnitude of 2.08. The distance to this star from the Sun can be deduced from the parallax measurements made during the Hipparcos mission, yielding a value of . Amateur astronomers can use Kochab as a very precise guide for setting up a telescope, as the celestial north pole is located 43 arcminutes away from Polaris, very close to the line connecting Polaris with Kochab.
The is a minivan produced by the Japanese automaker Toyota since 2002. It is available as a seven- or eight-seater with petrol and hybrid engine options. Hybrid variants have been available since 2003 and it incorporates Toyota's Hybrid Synergy Drive technology. The vehicle was named after Alphard, the brightest star in the constellation Hydra.
The brightest star is WR 25 WR 25 is a binary system in the central portion of the Carina Nebula, a member of the cluster. The primary is a Wolf–Rayet star, possibly the most luminous star in the galaxy. The secondary is hard to detect but thought to be a luminous OB star.
Mu Herculis is a quadruple star system. The brightest star is a well-studied G-type subgiant, whose parameters are precisely determined from asteroseismology. It was believed to be a close binary with a low-mass stellar or a large substellar companion. This was confirmed when low- mass companion was resolved using near-infrared spectroscopy.
Most of these stars lie in Hydra. The three brightest stars—Delta, Alpha and Gamma Crateris—form a triangle located near the brighter star Nu Hydrae in Hydra. Within the constellation's borders, there are 33 stars brighter than or equal to apparent magnitude 6.5. Delta Crateris is the brightest star in Crater at magnitude 3.6.
Procyon A is 1.4 times the Sun's mass, while its smaller companion is 0.6 times as massive as the Sun. The system is from Earth, the shortest distance to a northern-hemisphere star of the first magnitude. Gomeisa, or Beta Canis Minoris, with a magnitude of 2.89, is the second-brightest star in Canis Minor.
The dust disk around Fomalhaut—the brightest star in Piscis Austrinus constellation. Asymmetry of the disk may be caused by a giant planet (or planets) orbiting the star. The formation of giant planets is an outstanding problem in the planetary sciences. In the framework of the solar nebular model two theories for their formation exist.
Iota Cassiopeiae is known to be a quintuple star system. The brightest star system, ι Cassiopeiae A, contains a white-colored A-type main-sequence star with a mean apparent magnitude of +4.61. The primary component is a tighter binary star system itself. The two stars themselves were resolved by adaptive optics, revealing two stars.
The last occultation by a planet took place on November 17, 1981, when it was occulted by Venus. This is the brightest star that can be principally occulted by an exterior planet between 5000 BC and 5000 AD. However, only Mars can do this, and only rarely; the last time was on September 3, 423.
Nebraska Historic Buildings Survey—Reconnaissance Final Report of Cheyenne County, Nebraska. Nebraska State Historical Society. Retrieved June 22, 2010. The last of these was named by citizens who declared it would become the state's "banner county", and "the brightest star in the constellation of Nebraska counties".Fitzpatrick, Lilian Linder (1925). "Banner County". Nebraska Place- Names.
Delta Herculis (δ Herculis, abbreviated Delta Her, δ Her) is a multiple star system in the constellation of Hercules. Its light produces to us apparent magnitude 3.12, as such the third-brightest star in the large, fairly dim constellation. Based on parallax measurement taken during the Hipparcos mission, it is approximately from the Sun.
HD 179070 also known as Kepler-21 is a F-type subgiant star. A transiting exoplanet was discovered orbiting this star by the Kepler spacecraft. At a magnitude of 8.25 this was the brightest star observed by Kepler to host a validated planet until the discovery of an exoplanet orbiting HD 212657 in 2018.
Delta Equulei, Latinized from δ Equulei, is the second brightest star in the constellation Equuleus. Delta Equulei is a binary star system about 60 light years away, with components of class G0 and F5. Their combined magnitude is 4.47, and their absolute magnitude is 3.142. There is controversy as to the exact masses of the stars.
Mimosa , designated β Crucis (Latinised to Beta Crucis, abbreviated Beta Cru, β Cru), is the second-brightest object in the constellation of Crux, after Acrux (Alpha Crucis), and the 20th-brightest star in the night sky. It forms part of the prominent asterism called the Southern Cross. Mimosa is a binary star or a possible triple star system.
Alpha Cygni, called Deneb, is the brightest star in Cygnus. It is a white supergiant star of spectral type A2Iae that varies between magnitudes 1.21 and 1.29, one of the largest and most luminous A-class stars known. It is located about 3200 light-years away. Its traditional name means "tail" and refers to its position in the constellation.
Aquila is a constellation on the celestial equator. Its name is Latin for 'eagle' and it represents the bird that carried Zeus/Jupiter's thunderbolts in Greek-Roman mythology. Its brightest star, Altair, is one vertex of the Summer Triangle asterism. The constellation is best seen in the northern summer, as it is located along the Milky Way.
It was made up of a small group of stars, now called 33 Arietis, 35 Arietis, 39 Arietis, and 41 Arietis, in the north of the constellation of Aries. The brightest star is now known as 41 Arietis (Bharani). At magnitude 3.63, it is a blue-white main sequence star of spectral type B8V around 166 light-years distant.
Pismis 24-1, also known as HD 319718, is the brightest star of the open cluster Pismis 24 within the nebula NGC 6357 about 6,500 light-years away. It was once thought to be the most massive star known, but is composed of at least three individual objects, each still among the most luminous and most massive stars known.
The star's magnitude as observed from Earth is 9; this signifies that the body is not visible with the naked eye, but can be seen with a telescope. HD 2039 lies roughly 280 light years from the Sun, which is about as far from the Sun as the second brightest star in the night sky, Canopus.
The star-like objects that Halt reported hovering low to the north and south are thought by some sceptics to have been misinterpretations of bright stars distorted by atmospheric and optical effects, another common source of UFO reports. The brightest of them, to the south, matched the position of Sirius, the brightest star in the night sky.
V533 Carinae is the brightest star in the region. The other bright stars in NGC 3572 are hot young stars such as HD 97166 and all the clusters in the region are only a few million years old. V533 Carinae is classified as a double star with the companion being a magnitude 11.5 star 21.7 arc-seconds away.
The constellations Phoenix, Grus, Pavo and Tucana, are known as the Southern Birds. The brightest star, Alpha Phoenicis, is named Ankaa, an Arabic word meaning 'the Phoenix'. It is an orange giant of apparent magnitude 2.4. Next is Beta Phoenicis, actually a binary system composed of two yellow giants with a combined apparent magnitude of 3.3.
55 It is located 5° WNW of delta Monocerotis and 2° SSE of 18 Monocerotis. The brightest star of the cluster is an orange G8 subgiant star of 8.0 magnitude, but it is possible that it is a foreground star. The cluster contains also blue giants. The brightest main sequence star is a B9 star with magnitude 9.1.
The central stars of Praesepe. ε Cancri is the brightest star, left of centre (north is towards bottom right). ε Cancri (Latinised to Epsilon Cancri) is the system's Bayer designation (which originally referred to the entire cluster). In 2016, the IAU organized a Working Group on Star Names (WGSN) to catalog and standardize proper names for stars.
The Dutch swimming team eventually signed contracts with Philips, Nike, and Speedo. Enough funds were raised to open a swim school in Eindhoven, Van den Hoogenband's place of residence. The team eventually grew to ten. Pieter remained the Netherlands' brightest star, and along with fellow Dutch Inge de Bruijn brought the Netherlands many victories in the sport.
With an apparent magnitude of 2.59, Gamma Corvi—also known as Gienah—is the brightest star in the constellation. It is an aging blue giant around four times as massive as the Sun. The young star Eta Corvi has been found to have two debris disks. Three star systems have exoplanets, and a fourth planetary system is unconfirmed.
Alpha Hydri (α Hyi, α Hydri) is the second brightest star in the southern circumpolar constellation of Hydrus. It is readily visible to the naked eye with an apparent visual magnitude of +2.9. It is sometimes informally known as the Head of Hydrus. This should not be confused with Alpha Hydrae (Alphard) in the constellation Hydra.
Beta Gruis (β Gruis, abbreviated Beta Gru, β Gru), formally named Tiaki , is the second brightest star in the southern constellation of Grus. It was once considered the rear star in the tail of the constellation of the (Southern) Fish, Piscis Austrinus: it, with Alpha, Delta, Theta, Iota, and Lambda Gruis, belonged to Piscis Austrinus in medieval Arabic astronomy.
Alnilam (ε Orionis) is a supergiant, approximately 2,000 light-years away from Earth and magnitude 1.70. It is the 29th-brightest star in the sky and the fourth-brightest in Orion. It is 375,000 times more luminous than the Sun. Its spectrum serves as one of the stable anchor points by which other stars are classified.
Sigma Sagittarii (σ Sagittarii, abbreviated Sigma Sgr, σ Sgr), formally named Nunki , is the second-brightest star in the constellation of Sagittarius. It has an apparent magnitude of +2.05, making it readily visible to the naked eye. The distance to this star, determined using parallax measurements from the Hipparcos astrometry satellite, yields an estimated value of from the Sun.
Beta Librae (β Librae, abbreviated Beta Lib, β Lib), formally named Zubeneschamali , is (despite its 'beta' designation) the brightest star in the zodiac constellation of Libra. From parallax measurements, its distance can be estimated as from the Sun. The apparent visual magnitude of this star is 2.6. According to Eratosthenes, Beta Librae was observed to be brighter than Antares.
Beta Leonis Minoris (Beta LMi, β Leonis Minoris, β LMi) is a binary star in the constellation of Leo Minor. It has an overall apparent visual magnitude of approximately 4.2. Although it is the only star in Leo Minor with a Bayer designation, it is only the second brightest star in the constellation (the brightest is 46 Leonis Minoris).
The name Hadar comes from the GUCCCo. Star Class boats being named after stars or constellations. "Hadar" is more commonly known as "Beta Centauri" and is the tenth-brightest star in the night sky. It is in the southern hemisphere and part of the Centaurus constellation and one of the two stars that point to the Southern Cross.
O'Toole in the 1983 made-for-TV miniseries The Blue and the Gray. He was also a regular the series Automan (1983) and Our House (1986). Also in 1986, O'Loughlin played the part of Mr. Parks in a first season episode of Highway to Heaven entitled "The Brightest Star". In 1988, he played Tom Callahan in Dirty Dancing.
Procyon is the brightest star in the constellation of Canis Minor and usually the eighth-brightest star in the night sky, with a visual apparent magnitude of 0.34. It has the Bayer designation α Canis Minoris, which is Latinised to Alpha Canis Minoris, and abbreviated α CMi or Alpha CMi, respectively. As determined by the European Space Agency Hipparcos astrometry satellite, this system lies at a distance of just , and is therefore one of Earth's nearest stellar neighbours. A binary star system, Procyon consists of a white-hued main-sequence star of spectral type F5 IV–V, designated component A, in orbit with a faint white dwarf companion of spectral type DQZ, named Procyon B. The pair orbit each other with a period of 40.8 years and an eccentricity of 0.4.
There is some evidence for the existence of close stellar companions of Betelgeuse, orbiting it within its gaseous envelope (see From a Changeling Star by Jeffrey Carver and the television series Space Battleship Yamato, below). Astronomers believe that this tremendous star is only 10 million years old, but has evolved rapidly because of its great mass. Currently in a late stage of stellar evolution, it is expected to erupt in a Type II supernova, possibly within the next million years (see From a Changeling Star by Jeffrey Carver, "Transit of Betelgeuse" by Robert R. Chase and Calculating God by Robert J. Sawyer, below). Betelgeuse is the eighth-brightest star in the night sky and second- brightest star in the constellation of Orion, outshining its neighbour Rigel (Beta Orionis) only rarely.
Regulus is the brightest star in the constellation of Leo (right tip, below is bright Jupiter in 2004). α Leonis (Latinized to Alpha Leonis) is the star system's Bayer designation. The traditional name Rēgulus is Latin for 'prince' or 'little king'. In 2016, the International Astronomical Union organized a Working Group on Star Names (WGSN) to catalog and standardize proper names for stars.
In 1953, a new dog unit was named as Sirius Patrol, after the star constellation Canis Major. It contains Sirius, also well known as the brightest star in the night sky, called “dog-star”. Prince Frederik of Denmark took part in a Sirius expedition from 11 February to 31 May 2000, which gave the Unit a new value in the story of Greenland.
The constellation's dimmer stars were noted by Johann Bayer, who named eight stars including Alpha and Beta, and John Flamsteed, who numbered fourteen. Procyon is the seventh-brightest star in the night sky, as well as one of the closest. A yellow-white main sequence star, it has a white dwarf companion. Gomeisa is a blue-white main sequence star.
Carina contains Canopus, a white-hued supergiant that is the second brightest star in the night sky at magnitude −0.72. Alpha Carinae, as Canopus is formally designated, is 313 light-years from Earth. Its traditional name comes from the mythological Canopus, who was a navigator for Menelaus, king of Sparta. There are several other stars above magnitude 3 in Carina.
Hamal is the brightest star in the constellation of Aries. Alpha Arietis is the star's Bayer designation. It also bears the Flamsteed designation of 13 Arietis. The traditional name Hamal (also written Hemal, Hamul, Ras Hammel) derives from the Arabic rās al-ħamal "head of the ram", in turn from the name for the constellation as a whole, Al Ħamal "the ram".
Libra is a constellation of the zodiac and is located in the Southern celestial hemisphere. Its name is Latin for weighing scales, and its symbol is 20px (Unicode ♎). It is fairly faint, with no first magnitude stars, and lies between Virgo to the west and Scorpius to the east. Beta Librae, also known as Zubeneschamali, is the brightest star in the constellation.
Epsilon Lupi, Latinized from ε Lup, is a multiple star system in the southern constellation of Lupus. At an apparent visual magnitude of 3.41, Epsilon Lupi can be readily viewed from the southern hemisphere with sufficiently dark skies. It is the fifth-brightest star or star system in the constellation. Parallax measurements give a distance to this system of roughly .
The Winx Club notices that some of the stars in the sky are disappearing. They determine that the return of Valtor is linked to this strange occurrence. The fairies travel to Lumenia, the Magic Dimension's brightest star and the light source for Stella's home planet of Solaria. Lumenia's queen gives them the power of Cosmix to protect the magical universe's billions of stars.
On 19 February 2019, between 5:11 and 5:32 UTC, Jürgenstock occulted the star Sirius in the constellation Canis Major, the brightest star in the night sky. The shadow crossed Southern Argentina, Southern Chile, Central America, and the Caribbean. Occultations are typically an excellent method to determine a minor planet's dimension (cross-section) by exactly measuring the duration of the event.
Pi³ Orionis (π³ Orionis, abbreviated Pi³ Ori, π³ Ori), also named Tabit , is a star in the equatorial constellation of Orion. At an apparent visual magnitude of 3.16, it is readily visible to the naked eye and is the brightest star in the lion's hide (or shield) that Orion is holding. As measured using the parallax technique, it is distant from the Sun.
Zeta Arae (ζ Ara, ζ Arae) is the third-brightest star in the southern constellation Ara. The apparent visual magnitude of this star is 3.1, which can be seen from suburban skies in the southern hemisphere. From the parallax measurements, it is located at a distance of from Earth. The spectrum of this star matches a stellar classification of K3 III.
The second method uses Canopus (the second-brightest star in the sky) and Achernar. Make a large equilateral triangle using these stars for two of the corners. The third imaginary corner will be the south celestial pole. If Canopus has not yet risen, the second- magnitude Alpha Pavonis can also be used to form the triangle with Achernar and the pole.
In Māori mythology, Atutahi is the name of Canopus, (Alpha Carinae). Atutahi is the second brightest star in the night-time sky, second only to Sirius (Takurua). Aotahi, Autahi, and Atutahi, "First-light" or "Single-light", were equivalent names that also intimated the star's solitary or self-centered nature. Atutahi is considered to be very tapu star, and always dwells alone.
Just shading Alpha, Beta Aquarii is the brightest star in Aquarius with an apparent magnitude of 2.91. It also has the proper name of Sadalsuud. Having cooled and swollen to around 50 times the Sun's diameter, it is around 2200 times as luminous as the Sun. It is around 6.4 times as massive as the Sun and around 56 million years old.
Were the Sun to be observed from this star system, it would appear to be a magnitude 2.55 star in the constellation Aquila with the exact opposite coordinates at right ascension , declination . It would be as bright as β Scorpii is in our sky. Canis Minor would obviously be missing its brightest star. Procyon's closest neighboring star is Luyten's Star, about away.
Arcturus is the brightest star in the constellation of Bootes. α Boötis (Latinised to Alpha Boötis) is the star's Bayer designation. The traditional name Arcturus derives from Ancient Greek Ἀρκτοῦρος (Arktouros) and means "Guardian of the Bear", ultimately from ἄρκτος (arktos), "bear" and οὖρος (ouros), "watcher, guardian". It has been known by this name since at least the time of Hesiod.
DL Crucis has a visual apparent magnitude of 6.3 so it is just visible with the unaided eye in dark skies. It lies in the small southern constellation of Crux, halfway between η Crucis and ζ Crucis and close to the constellation's brightest star α Crucis. This area of sky lies within the Milky Way and close to the Coalsack Nebula.
Although none of the stars are particularly bright, they lie in a dim area of the sky, rendering the asterism easy to distinguish in the night sky. Gamma and Delta serve as pointers toward Spica. Also called Gienah, Gamma is the brightest star in Corvus at magnitude 2.59. Its traditional name means "wing", the star marking the left wing in Bayer's Uranometria.
Gamma Gruis (γ Gruis, abbreviated Gam Gru, γ Gru), formally named Aldhanab , is a star in the southern constellation of Grus (it once belonged to the Ptolemaic constellation Piscis Austrinus). With an apparent visual magnitude of 3.0, it is the third-brightest star in Grus. Based upon parallax measurements, this star is located at a distance of roughly from the Sun.
Eta Ceti (η Cet, η Ceti) is a star in the equatorial constellation of Cetus. It has the traditional name Deneb Algenubi or Algenudi. The apparent visual magnitude of this star is +3.4, making it the fourth-brightest star in this otherwise relatively faint constellation. The distance to this star can be measured directly using the parallax technique, yielding a value of .
During the 1980s, Gary did several guest voice-over appearances in such Disney television series as Darkwing Duck, DuckTales, TaleSpin, The Little Mermaid series and Bonkers. She voiced a gazelle and a hippo on the Lion King read-along cassette story, The Brightest Star. She also voiced Maleficent and the Opening narrator in 'Fantasmic'. She voiced Muffy Vanderschmere in TaleSpin.
It is radiating over 12,000 times the luminosity of the Sun from its swollen photosphere at an effective temperature of 9,840 K. 9 Persei has one visual companion, designated component B, at an angular separation of and magnitude 12.0. Vizier catalog entry The Double Cluster. 9 Persei is the brightest star on right side of the image. North is to the left.
Beta Tauri (Latinised from β Tauri, abbreviated Beta Tau, β Tau), officially named Elnath (pronounced or , sometimes spelled Alnath), is the second- brightest star located in the constellation borders of Taurus and Auriga with an apparent magnitude of 1.65. It is a chemically peculiar B7 giant star, 134 light years away from Earth. It had a co-existing name Gamma Aurigae.
The symbol representing Taurus is 20px (Unicode ♉), which resembles a bull's head. A number of features exist that are of interest to astronomers. Taurus hosts two of the nearest open clusters to Earth, the Pleiades and the Hyades, both of which are visible to the naked eye. At first magnitude, the red giant Aldebaran is the brightest star in the constellation.
Alpha Camelopardalis (Alpha Cam, α Camelopardalis, α Cam) is a star in the constellation Camelopardalis, with an apparent visual magnitude of 4.3. It is the third-brightest star in this not-very-prominent circumpolar constellation, the first and second-brightest stars being β Camelopardalis and CS Camelopardalis, respectively. It is the farthest constellational star, with a distance of 6,000 light-years from Earth.
Altair is the brightest star in the constellation Aquila and the twelfth brightest star in the night sky. With an apparent visual magnitude of 0.77, it is one of the closest stars visible to the unaided eye (most of the nearest stars are red dwarfs too dim to see without a telescope). It forms a part of two well-known triplet asterisms: With β and γ Aquilae it forms the straight line of stars sometimes referred to as the Family of Aquila or the Shaft of Aquila; more prominently, it is the southernmost vertex of the Summer Triangle, the other two vertices being the bright stars Deneb and Vega (see High Sierra, below). The name Altair is from the Arabic (النسر الطائر an-nasr aṭ-ṭā’ir), which translates literally as the flying eagle, from its belonging to the constellation.
Canopus is the brightest star in the constellation of Carina (top). The absorption lines in the spectrum of Canopus shift slightly with a period of . This was first detected in 1906 and the Doppler variations were interpreted as orbital motion. An orbit was even calculated, but no such companion exists and the small radial velocity changes are due to movements in the atmosphere of the star.
Columba is rather inconspicuous, the brightest star, Alpha Columbae, being only of magnitude 2.7. This, a blue- white star, has a pre-Bayer, traditional, Arabic name Phact (meaning ring dove) and is 268 light-years from Earth. The only other named star is Beta Columbae, which has the alike-status name Wazn. It is an orange-hued giant star of magnitude 3.1, 87 light-years away.
Canes Venatici is one of the 88 official modern constellations. It is a small northern constellation that was created by Johannes Hevelius in the 17th century. Its name is Latin for 'hunting dogs', and the constellation is often depicted in illustrations as representing the dogs of Boötes the Herdsman, a neighboring constellation. Cor Caroli is the constellation's brightest star, with an apparent magnitude of 2.9.
Cancer is one of the twelve constellations of the zodiac and is located in the Northern celestial hemisphere. Its name is Latin for crab and it is commonly represented as one. Its astrological symbol is♋. Cancer is a medium-size constellation with an area of 506 square degrees and its stars are rather faint, its brightest star Beta Cancri having an apparent magnitude of 3.5.
Even so, it radiates about as much energy in 20 seconds as the Sun does in a year. A close point source has been discovered hidden in the surrounding nebulosity, but there has been no confirmation of this being a star or whether it is physically associated. The Pistol Star is the brightest star in this image of the Quintuplet cluster, just below centre.
Beta Pyxidis (Beta Pyx, β Pyxidis, β Pyx) is a double star located in the southern constellation Pyxis. It has an apparent visual magnitude of 3.954, making it the second brightest star in that faint constellation. Based upon parallax measurements, the star is an estimated 420 light-years (128 parsecs) from the Earth. The spectrum matches a bright giant or supergiant star of stellar classification G7Ib-II.
About 25 stars are visible in a telescope with a aperture. M26 spans a linear size of 22 light years across with a tidal radius of , and is at a distance of 5,160 light years from the Earth. The brightest star is of magnitude 11 and the age of this cluster has been calculated to be 85.3 million years. It includes one known spectroscopic binary system.
A faint constellation, its three brightest stars—Alpha, Beta and Gamma Pyxidis—are in a rough line. At magnitude 3.68, Alpha is the constellation's brightest star. It is a blue-white star approximately distant and around 22,000 times as luminous as the Sun. Pyxis is located close to the stars that formed the old constellation Argo Navis, the ship of Jason and the Argonauts.
The brightest star in Equuleus is Alpha Equulei, traditionally called Kitalpha, a yellow star magnitude 3.9, 186 light-years from Earth. Its traditional name means "the section of the horse". There are few variable stars in Equuleus. Only around 25 are known, most of which are faint. Gamma Equulei is an alpha CVn star, ranging between magnitudes 4.58 and 4.77 over a period of around 12½ minutes.
Sports Illustrated referred to Edwards as "a combination of Santa Claus and Genghis Khan." In 1986, Edwards became the second Wittenberg football coach to be inducted into the College Football Hall of Fame. The brightest star of the Edwards era at Wittenberg was quarterback Charlie Green. With Green leading the team, Wittenberg compiled a 25-0-1 record and won two national championships from 1962 to 1964.
11 A few years later, Gustav Fröding made his debut. While controversial in his own time, Fröding has proven to be Sweden's most popular poet.Olsson (2009), p 300 The poetry of Erik Axel Karlfeldt was awarded the Nobel Prize in Literature in 1931. The novelist Selma Lagerlöf (1858–1940) was arguably the brightest star of the 1890s, and her influence has lasted up to modern times.
Actress Emma Barton was chosen to play Honey Edwards in September 2005, after a successful screen test with Perry Fenwick. Barton commented, "I can’t wait to join EastEnders and play Honey. She’s a really sweet girl, who always wants to do the best for everyone but she’s not exactly the brightest star in the sky." Barton was axed from the show in April 2008.
Altair is the brightest star in the constellation Aquila α Aquilae (Latinised to Alpha Aquilae) is the star's Bayer designation. The traditional name Altair has been used since medieval times. It is an abbreviation of the Arabic phrase (An-nisr) Al-ta'ir "". In 2016, the International Astronomical Union organized a Working Group on Star Names (WGSN) to catalog and standardize proper names for stars.
Sitara Brooj Akbar, (literal translation The Brightest Star in the Constellation) was born on the 10th of February,2000 in the small town of Rabwah in Punjab, Pakistan is the eldest of 5 siblings and belongs to the Ahmadiyya Muslim Community. She is currently serving as the youth ambassador for Pakistan Association Dubai. and is a student. She is interested in research, community work and international relations.
Beta Columbae (β Columbae, abbreviated Beta Col, β Col), officially named Wazn , is the second brightest star in the southern constellation of Columba. It has an apparent visual magnitude of 3.1, which is bright enough to be viewed with the naked eye even from an urban location. Parallax measurements place it at a distance of about from the Sun. Beta Columbae is the star's Bayer designation.
Octans is a very faint constellation; its brightest member is Nu Octantis, a spectral class K1 III giant star with an apparent magnitude 3.73. It is 63.3 ± 0.8 light-years distant from Earth. Beta Octantis is the second brightest star in the constellation. Sigma Octantis, the southern pole star, is a magnitude 5.4 star just over 1 degree away from the true South Celestial Pole.
Cor Scorpii ("Scorpion's Heart" in Latin) is a black metal band from Sogndal, Norway, founded in 2004 by Gaute Refsnes, the former keyboardist of Windir. Cor Scorpii is an alternative name of Antares, the 15th brightest star in the sky. The name was chosen because the band members felt that it conveyed a mysterious and atmospheric feeling, corresponding to the musical and lyrical content.
Omicron Velorum is a blue-white subgiant of spectral type B3III-IV located around 495 light-years from the Solar System. A slowly pulsating B star, it ranges between magnitudes 3.57 and 3.63 over 2.8 days. It is the brightest star in, and gives its name to, the Omicron Velorum Cluster, also known as IC 2391, an open cluster located around 500 light-years away.
At an apparent magnitude of 1.94, this is the brightest star in Pavo. Based upon parallax measurements, this star is about distant from the Earth. It has an estimated six times the Sun's mass and 6 times the Sun's radius, but 2,200 times the luminosity of the Sun. The effective temperature of the photosphere is 17,700 K, which gives the star a blue-white hue.
Epsilon Pegasi (Latinised from ε Pegasi, abbreviated Epsilon Peg, ε Peg), formally named Enif , is the brightest star in the northern constellation of Pegasus. With an average apparent visual magnitude of 2.4, this is a second- magnitude star that is readily visible to the naked eye. The distance to this star can be estimated using parallax measurements from the Hipparcos astrometry satellite, yielding a value of around .
Alpha Leporis (α Leporis, abbreviated Alpha Lep, α Lep), formally named Arneb , is the brightest star in the constellation of Lepus. Alpha Leporis is the star's Bayer designation. The traditional name Arneb comes from the Arabic أرنب ’arnab 'hare' ('Lepus' is Latin for hare). In 2016, the International Astronomical Union organized a Working Group on Star Names (WGSN) to catalog and standardize proper names for stars.
Alnilam is the middle and brightest of the three stars of Orion's Belt It is the 29th-brightest star in the sky (the 4th- brightest in Orion) and is a blue supergiant. Together with Mintaka and Alnitak, the three stars make up Orion's belt, known by many names across many ancient cultures. Alnilam is the middle star. It is slightly variable, from magnitude 1.64 to 1.74.
The Carina Nebula. Eta Carinae is the brightest star, on the left side. Mass loss is one of the most intensively studied aspects of massive star research. Put simply, calculated mass loss rates in the best models of stellar evolution do not reproduce the observed properties of evolved massive stars such as Wolf–Rayets, the number and types of core collapse supernovae, or their progenitors.
Mohatu is the King of the Pride Lands during the events of the story The Brightest Star. He is the grandfather of Mufasa and Scar and the great-grandfather of Simba. He went to find water for the animals of the land during a drought and helped the animals get on with each other. When he died, he became a star which was brighter than the others.
Delta Scuti (δ Sct, δ Scuti) is a giant star in the southern constellation Scutum. With an apparent visual magnitude of 4.72, it is the fifth-brightest star in this small and otherwise undistinguished constellation. Analysis of the parallax measurements made during the Hipparcos mission place this star at a distance of about from Earth. Delta Scuti is the prototype of the Delta Scuti type variable stars.
Nu Eridani (ν Eri) is a star in the constellation Eridanus. It is visible to the naked eye with an apparent visual magnitude of 3.93. The distance to this star is roughly 520 light years, based upon an annual parallax shift of 0.00625 arcseconds. If the star were from the Sun, it would be the brightest star in the night sky with an apparent magnitude of −2.84.
Alcyone , designated η Tauri (Eta Tauri, abbreviated Eta Tau, η Tau), is a multiple star system in the constellation of Taurus. Approximately 440 light years from the Sun, it is the brightest star in the Pleiades open cluster, which is a young cluster, around 100 million years old. There are a number of fainter stars very close to Alcyone, all likely members of the same cluster.
Lambda Velorum (λ Velorum, abbreviated Lambda Vel, λ Vel), officially named Suhail , is a star in the southern constellation of Vela. With a mean apparent visual magnitude of 2.21, this is the third-brightest star in the constellation and one of the brighter stars in the sky. The distance to this star can be measured directly using the parallax technique, yielding an estimated from the Sun.
NGC 346. HD 5980 is the brightest star on the left, just above centre. HD 5980 is visually a single star, but the spectrum reveals three hot luminous components. The physical parameters of the three stars are uncertain because of the difficulties of resolving their spectra, the partial eclipses, apparent intrinsic variations with the orbital phase, and the strong variability of at least one component.
This is corroborated by the Greek name for Boötes, Arctophylax, which means "Bear Watcher". Callisto, in the form of a bear was almost killed by her son, who was out hunting. Zeus rescued her, taking her into the sky where she became Ursa Major, "the Great Bear". Arcturus, the name of the constellation's brightest star, comes from the Greek word meaning "guardian of the bear".
Gamma Lyrae (Latinized from γ Lyrae, abbreviated Gamma Lyr, γ Lyr), formally named Sulafat , is the second-brightest star in the northern constellation of Lyra. With an apparent visual magnitude of 3.3, it is readily visible to the naked eye. Parallax measurements yield an estimated distance of from the Sun. At that distance, the visual magnitude of the star is diminished by an extinction factor of due to interstellar dust.
HR 5955 is a single star in the far southern constellation of Apus. It is 28.5 minutes earlier than and about 5 deg. north of the yellow giant star Gamma Apodis, which is the second brightest star in the constellation of Apus. This object has an orange hue and is visible to the naked eye as a dim point of light with an apparent visual magnitude of 5.70.
In classical mythology Corona Borealis generally represented the crown given by the god Dionysus to the Cretan princess Ariadne and set by him in the heavens. Other cultures likened the pattern to a circle of elders, an eagle's nest, a bear's den, or even a smokehole. Ptolemy also listed a southern counterpart, Corona Australis, with a similar pattern. The brightest star is the magnitude 2.2 Alpha Coronae Borealis.
Flamsteed's listing of Nu1, Nu2, Nu3, Xi1, Xi2, Omicron1 and Omicron2 have all remained in use. Canis Major as depicted in Urania's Mirror, a set of constellation cards published in London c.1825. Next to it are Lepus and Columba (partly cut off). Sirius is the brightest star in the night sky at apparent magnitude −1.46 and one of the closest stars to Earth at a distance of 8.6 light-years.
Carbon monoxide observations provide much of the information about the molecular clouds in which most stars form. Beta Pictoris, the second brightest star in the constellation Pictor, shows an excess of infrared emission compared to normal stars of its type, which is caused by large quantities of dust and gas (including carbon monoxide) near the star. Solid carbon monoxide is a component of comets. Halley's Comet is about 15% carbon monoxide.
Alpha Fornacis (α Fornacis, abbreviated Alpha For, α For) is a binary star system in the southern constellation of Fornax. It is the brightest star in the constellation and the only one brighter than magnitude 4.0. Based on parallax measurements obtained during the Hipparcos mission, it is approximately 46 light-years (14 parsecs) distant from the Sun. Its two components are designated Alpha Fornacis A (officially named Dalim ) and B.
31 Lyncis is the fourth-brightest star in the constellation of Lynx. It has the traditional name Alsciaukat, pronounced . The orange-hued star is visible to the naked eye with a baseline apparent visual magnitude of +4.25. It is a single star located about 380 light years away from the Sun, based on parallax, and is moving further away with a heliocentric radial velocity of +25 km/s.
Map of the constellation Mons Maenalus Mons Maenalus (Latin for Mount Maenalus) was a constellation created by Johannes Hevelius in 1687. It was located between the constellations of Boötes and Virgo, and depicts a mountain in Greece that the herdsman is stepping upon. It was increasingly considered obsolete by the latter half of the 19th century. Its brightest star is 31 Boötis, a G-type giant of apparent magnitude 4.86m.
Psi2 Aurigae (also known as 50 Aurigae), with an apparent magnitude of 4.8, was the brightest star in the constellation, Bode assigning it the designation 'a'. Located 420 ± 20 light-years distant from earth, Note: see VizieR catalogue I/311. it is an orange giant of spectral type K3III. Other stars belonging to the constellation include Psi4, Psi5, Psi7, 63, 64, 65 and 66 Aurigae, and Omicron Geminorum.
The Solar System and all of the visible stars are in different orbits about the core of the Milky Way galaxy. Thus, their relative positions change over time, and for the nearer stars this movement can be measured. As a star moves toward or away from us, its apparent brightness changes. Sirius is currently the brightest star in Earth's night sky, but it has not always been so.
Alpha Arae, Latinized from α Arae, is the second brightest star in the southern constellation of Ara. With an average apparent visual magnitude 2.93, it is readily visible to the naked eye from the southern hemisphere. This star is close enough to the Earth that its distance can be estimated using parallax data collected during the Hipparcos mission. It is around away, with a 7% margin of error.
Alpha Antliae (Alpha Ant, α Antliae, α Ant) is the brightest star in the constellation of Antlia but it has not been given a proper name. It is approximately 320 light-years from the Solar System. It is a K-type giant star with an apparent visual magnitude of 4.25. This star has 2.2 times the mass of the Sun and has expanded to 41 times the solar radius.
It is about 1.4 to 1.7 times more massive than the Sun, and about two times wider than the Sun. Its effective temperature is about 6400 K. An infrared excess has been detected, indicating the presence of a circumstellar disk. 110 Herculis is the 17th-brightest star in the constellation. It is located in the sky about halfway between Rasalague in Ophiuchus and Albireo in Cygnus, offset a trifle west.
Beta Horologii, Latinized from β Horologii, is the third-brightest star in the southern constellation of Horologium. It is faintly visible to the naked eye with an apparent visual magnitude of 4.98. Based upon an annual parallax shift of 11.07 mas as seen from Earth, it is located about 295 light years from the Sun. The star is moving away with a radial velocity of +24 km/s.
Beta Lacertae (Beta Lac, β Lacertae, β Lac) is the fourth-brightest star in the constellation of Lacerta. Based upon an annual parallax shift of 19.19 mas, it is 170 light years distant from Earth. At that distance, the visual magnitude is diminished by an extinction factor of 0.17 due to interstellar dust. This is an evolved G-type giant with an apparent visual magnitude of approximately 4.43.
Baptiste learned to play guitar as a boy in Dominica where he was born. In the 1970s, he was involved in bands on the island playing French Creole music that originated in the archipelago formed from Guadeloupe to Martinique. The music known as "cadence" further developed into zouk. Baptiste, however, was deeply influenced by roots rock reggae which was at its peak with Bob Marley as the brightest star.
The stars of the modern constellation Grus once formed the "tail" of Piscis Austrinus. In 1597 (or 1598), Petrus Plancius carved out a separate constellation and named it after the crane. Its only star brighter than 4th magnitude is Fomalhaut, the 18th-brightest star in the night sky. Surrounded by a circumstellar disk, it was announced as having a planet in 2008, though this discovery has been challenged.
Gamma Microscopii (γ Microscopii, γ Mic) is the brightest star in the faint southern constellation of Microscopium. It has an apparent visual magnitude of 4.68, which is too dim to be viewed from city skies. The distance to this star has been determined using parallax measurements made with the Gaia telescope, which place it at . Based upon a stellar classification of G6 III, this is a G-type giant star.
U Mon can often be seen with the naked eye between Sirius and Procyon, but drops below naked eye visibility at deep minima. It lies about two degrees west of α Mon, at fourth magnitude the brightest star in Monoceros. At its brightest U Mon can reach magnitude 5.45. At a shallow minimum it drops to about magnitude 6.0, but at its deepest minima it is below magnitude 7.5.
Alpha Sagittae, formally named Sham , is a single star in the northern constellation of Sagitta. Alpha Sagittae is the Bayer designation, which is latinized from α Sagittae and abbreviated Alpha Sge or α Sge. It is visible to the naked eye as a yellow-hued star with an apparent visual magnitude of +4.38. Despite the name, this is not the brightest star in the constellation – that distinction belongs to Gamma Sagittae.
The brightest star in the HD 131399 system is designated HD 131399 A. Its spectral type is A1V, and it is 2.08 times as massive as the Sun. The two lower-mass stars are designated HD 131399 B and C, respectively. B is a G-type main- sequence star, while HD 131399 C is a K-type main-sequence star. Both stars are less massive than the Sun.
Gamma2 Normae, Latinized from γ2 Nor, is the brightest star in the southern constellation of Norma. Its apparent magnitude is 4.02 – making it a faint star but visible to the naked eye. Based upon an annual parallax shift of 25.33 mas as seen from Earth, this star is located roughly 129 light years from the Sun. It is moving closer to the Sun with a radial velocity of −29 km/s.
The second-brightest star, the yellow-white subgiant star Alpha Trianguli (3.41m) with a close dimmer companion, is also known as Caput Trianguli or Ras al Muthallath, and is at the apex of the triangle. It lies around 7 degrees north-northwest of Alpha Arietis. Making up the triangle is Gamma Trianguli, a white main sequence star of spectral type A1Vnn of apparent magnitude 4.00 about 112 light-years from Earth.
Beta Ceti (β Ceti, abbreviated Beta Cet, β Cet), also named Diphda , is the brightest star in the constellation of Cetus. Although designated 'beta', it is actually brighter than the 'alpha' star in the constellation (Alpha Ceti). This orange giant is easy to identify due to its location in an otherwise dark section of the celestial sphere. Based on parallax measurements, it lies at an estimated distance of from the Sun.
Despite having the Bayer designation α Ceti, at visual magnitude 2.54 this star is actually not the brightest star in the constellation Cetus. That honor goes instead to Beta Ceti at magnitude 2.04. Menkar is a red giant with a stellar classification of M1.5 IIIa. It has more than twice the mass of the Sun and, as a giant star has expanded to about 89 times the Sun's radius.
Alpha Sextantis (α Sex, α Sextantis) is the brightest star in the equatorial constellation of Sextans. It is visible to the naked eye on a dark night with an apparent visual magnitude of 4.49. The distance to this star, as determined from parallax measurements, is around 280 light years. This is considered an informal "equator star", as it lies less than a quarter of a degree south of the celestial equator.
Gamma Corvi (γ Corvi, abbreviated Gamma Crv, γ Crv) is a binary star and the brightest star in the southern constellation of Corvus, having an apparent visual magnitude of 2.59. The system's two components are designated Gamma Corvi A (officially named Gienah , traditionally the name of the system)) and Gamma Corvi B. The distance to this system has been measured directly using the parallax technique, yielding an estimated from the Sun.
Beta Eridani (β Eridani, abbreviated Beta Eri, β Eri), formally named Cursa , is the second-brightest star in the constellation of Eridanus, located in the northeast end of this constellation near the shared border with Orion. The apparent visual magnitude of this star is 2.796, so it can be viewed with the naked eye in dark skies. Parallax measurements yield an estimated distance of about from the Earth.
Beta Cancri (β Cancri, abbreviated Beta Cnc, β Cnc), also named Tarf , is the brightest star in the zodiacal constellation of Cancer. It has an apparent visual magnitude of +3.5 and an absolute magnitude of −1.2. Based on parallax measurements obtained during the Hipparcos mission, it is approximately 290 light-years distant from the Sun. An exoplanet, designated Beta Cancri b, is believed to be orbiting the star.
Within each magnitude class, Bayer made no attempt to arrange stars by relative brightness. See p. 192. As a result, the brightest star in each class did not always get listed first in Bayer's order. In addition, Bayer did not always follow the magnitude class rule; he sometimes assigned letters to stars according to their location within a constellation, or the order of their rising, or to historical or mythological details.
Occasionally the order looks quite arbitrary. Of the 88 modern constellations, there are at least 30 in which "Alpha" is not the brightest star, and four of those lack an alpha star altogether. The constellations with no alpha-designated star include Vela and Puppis – both formerly part of Argo Navis, whose Greek-letter stars were split between three constellations. α Arg is Canopus and was moved to the modern constellation Carina.
Its name means "male water snake", as opposed to Hydra, a much larger constellation that represents a female water snake. It remains below the horizon for most Northern Hemisphere observers. The brightest star is the 2.8-magnitude Beta Hydri, also the closest reasonably bright star to the south celestial pole. Pulsating between magnitude 3.26 and 3.33, Gamma Hydri is a variable red giant 60 times the diameter of our Sun.
Alpha Lyncis (α Lyn, α Lyncis) is the brightest star in the northern constellation of Lynx with an apparent magnitude of +3.13. Unusually, it is the only star in the constellation that has a Bayer designation. Based upon parallax measurements, this star is located about from the Earth. This is a giant star that has exhausted the hydrogen at its core and has evolved away from the main sequence.
Gamma² Sagittarii (γ² Sagittarii, abbreviated Gamma² Sgr, γ² Sgr), formally named Alnasl , is a 3rd-magnitude star in the zodiac constellation of Sagittarius. The location of this star forms the tip of the arrow in the bow of Sagittarius the Centaur. Based on parallax measurements obtained during the Hipparcos mission, it is approximately from the Sun. It has an apparent visual magnitude of +2.98, making it the seventh-brightest star in the constellation.
The central part of the cluster is framed by bright stars making up an "A"-shaped asterism. The upper tip of this asterism is HD 111904 (HR 4887, HIP 62894), a B9 supergiant and suspected variable star. It is the brightest member of the A asterism at magnitude 5.77. The brightest star in the region of the cluster is the variable DS Cru (HD 111613, HR 4876), which lies well beyond the A asterism.
Pictor is a constellation in the Southern Celestial Hemisphere, located between the star Canopus and the Large Magellanic Cloud. Its name is Latin for painter, and is an abbreviation of the older name Equuleus Pictoris (the "painter's easel"). Normally represented as an easel, Pictor was named by Abbé Nicolas-Louis de Lacaille in the 18th century. The constellation's brightest star is Alpha Pictoris, a white main-sequence star around 97 light-years away from Earth.
Delta Lupi (δ Lupi, δ Lup) is a star in the southern circumpolar constellation of Lupus. In traditional Chinese astronomy, it is "the 2nd (star) of the Cavalry Officer" (騎官二). With an apparent visual magnitude of 3.22, it is the fourth-brightest star in the constellation. The distance to this star has been measured using the parallax technique, yielding an estimate of roughly 900 light-years with a 15% margin of error.
Older references give the star cloud's magnitude as 4.6, but more recent estimates place it a full two magnitudes brighter, at 2.5. HD 167356 is the brightest star within the Small Sagittarius Star Cloud, a white supergiant with an apparent magnitude of 6.05. This star is an Alpha-2 Canum Venaticorum variable, showing small changes in brightness as it rotates. There are three other stars in M24 with visual magnitudes between 6.5 and 7.0.
Before capella, there was tonica, a program to analyse musical notation. Since some people used tonica mainly to print musical scores, the idea for a scorewriter was born. The first version was published in 1992 as a program named "Allegro", running under MS- DOS with its own graphical interface. Since the name was already taken, the name had to be changed - taking the name from the brightest star in the constellation Auriga, Capella.
Alcyone Cone () is an extinct volcanic cone near the center of The Pleiades, at the west side of the head of Mariner Glacier in Victoria Land, Antarctica. Named by a Victoria University of Wellington Antarctic Expedition field party to Evans Neve, 1971-72, after Alcyone, the brightest star in the Pleiades constellation. The geographical landform is situated on the Pennell Coast, a portion of Antarctica lying between Cape Williams and Cape Adare.
Alpha Octantis is a binary star system in the constellation of Octans. The name is Latinized from α Octantis. Despite being labeled the "alpha" star by Johann Bayer in his star atlas Uranometria, it is not the brightest star in the constellation – that title belongs to Nu Octantis. It is visible to the naked eye as a faint, yellow-white hued point of light with an overall apparent visual magnitude of approximately 5.13.
Eta Draconis (η Draconis, abbreviated Eta Dra, η Dra) is a binary star in the northern circumpolar constellation of Draco. Despite having an apparent visual magnitude of only +2.73, it is the second-brightest star in this generally faint constellation. Based upon parallax measurements collected during the Hipparcos mission, this star is located at a distance of about from the Sun. The two components are designated Eta Draconis A (also named Athebyne ) and B.
W Hydrae is a Mira-type variable star in the constellation Hydra. The star is nearly located within the Solar neighborhood, between 75 and 120 parsecs, likely at 375 light years from the Sun. It has a visual apparent magnitude range of 5.6 to 10. In the near-infrared J band it has a magnitude of -1.7, is the 7th brightest star in the night sky, and is even brighter than Sirius.
They recorded two extended plays, The Brightest Star (November 1992) and Chemcraze (May 1993), before Dalton flew to join United States alternative rockers, The Lemonheads from mid-1992. Both EPs were issued on the Dalton-owned Half a Cow record label. Dalton and Morgan had co-written material with The Lemonheads' founder Evan Dando. In August 1992 while The Lemonheads were touring the US, Godstar recorded their debut studio album, Sleeper, in Boston.
Beta Muscae, Latinized from β Muscae, is a binary star in the southern circumpolar constellation of Musca. With a combined apparent visual magnitude of 3.07, it is the second brightest star (or star system) in the constellation. Judging by the parallax results, it is located at a distance of roughly from the Earth. This is a binary star system with a period of about 194 years at an orbital eccentricity of 0.6.
Comparison of Stephenson 2-18 and VY Canis Majoris. The open cluster Stephenson 2 was discovered by American astronomer Charles Bruce Stephenson in 1990 in the data obtained by a deep infrared survey. The cluster is also known as RSGC2, one of several massive open clusters in Scutum, each containing multiple red supergiants. The brightest star in the region of the cluster was given the identifier 1 in the first analysis of cluster member properties.
Alpha Lupi (α Lupi, α Lup) is a blue giant star, and the brightest star in the southern constellation of Lupus. According to the Bortle Dark-Sky Scale, its apparent visual magnitude of 2.3 makes it readily visible to the naked eye even from highly light-polluted locales. Based upon parallax measurements made during the Hipparcos mission, the star is around from the solar system. It is one of the nearest supernova candidates.
It is a spectroscopic binary system, one estimate placing the distance between the pair of stars as 0.21 astronomical units (AU), or half the distance between Mercury and the Sun. The two stars rotate around each other in a mere 11 days and 18 hours. The star system is located around 180 light years away from Earth. With an apparent magnitude of 3.43, Beta Pavonis is the second-brightest star in the constellation.
Dusty ring around double star IRAS 08544-4431. The next brightest star is Delta Velorum or Alsephina, also a multiple star system and one of the brightest eclipsing binaries in the sky. Together with Kappa Velorum or Markeb, Iota Carinae or Aspidiske and Epsilon Carinae or Avior, it forms the diamond-shaped asterism known as the False Cross—so called because it is sometimes mistaken for the Southern Cross, causing errors in astronavigation.
The orange-hued Lambda Velorum, or Suhail, is the third-brightest star in the constellation. A supergiant of spectral type K4Ib-II, it varies between magnitudes 2.14 and 2.3, and lies 545 light-years distant. It has around 11,000 times the luminosity, 9 to 12 times the mass and 207 times the diameter or our sun. AH Velorum is a Cepheid variable located less than a degree to the northeast of Gamma.
Within the constellation's borders, there are 57 stars brighter than or equal to apparent magnitude 6.5. With a magnitude of 3.5, Alpha Telescopii is the brightest star in the constellation. It is a blue-white subgiant of spectral type B3IV which lies around 250 light-years away. It is radiating nearly 800 times the Sun's luminosity, and is estimated to be 5.2±0.4 times as massive and have 3.3±0.5 times the Sun's radius.
Alpha Circini (α Cir, α Circini) is a variable star in the faint, southern, circumpolar constellation of Circinus. At an apparent visual magnitude of 3.19, it is the brightest star in the constellation and can be readily seen with the naked eye from the southern hemisphere. Parallax measurements of this star yield an estimated distance of from the Earth. This star belongs to a class of variables known as rapidly oscillating Ap stars.
Alpha Sculptoris, Latinized from α Sculptoris, is the Bayer designation for a blue-white star in the southern constellation of Sculptor. It has an apparent visual magnitude of +4.30, which makes it the brightest star in this generally faint constellation. Parallax measurements collected during the Hipparcos mission provide a distance estimate for this star, placing it at roughly , with a 4% margin of error. Alpha Sculptoris is a B-type giant star.
Such stars are termed ellipsoidal variables. Within a few million years, as the primary continues to evolve into a red giant star, the system may become a semi-detached binary with the Roche lobe becoming filled to overflowing. The mean apparent magnitude of +3.42 for this pair is bright enough to be readily seen with the naked eye. It forms the second brightest star or star system in this generally faint constellation, following Beta Trianguli.
Zeta Telescopii (ζ Telescopii) is the second-brightest star in the southern constellation of Telescopium. It is a solitary, orange-hued star that is visible to the naked eye with an apparent visual magnitude of +4.13. Based upon an annual parallax shift of 25.84 mas as seen from Earth, it is located around 127 light years from the Sun. This is a red clump giant star of spectral type K1 III-IV.
"Winning" is a pop rock single originally written and recorded by Russ Ballard on his 1976 album of the same name. It was subsequently recorded by Latin rock band Santana for the 1981 album, Zebop!. The lead vocal on the Santana version was performed by Alex Ligertwood. It was the sixth track on the album and was released as the third single (backed with "Brightest Star") and as a promotional music video.
Alpha Monocerotis, Latinized from α Monocerotis, is the Bayer designation for the brightest star in the equatorial constellation of Monoceros. It can be viewed with the naked eye, having an apparent visual magnitude of 3.94. Based upon an annual parallax shift of 22.07 mas as seen from Earth, it is located 148 light years away from the Sun. The star is moving away from the Sun with a radial velocity of +10.5 km/s.
Cepheus is a constellation in the northern sky, named after Cepheus, a king of Aethiopia in Greek mythology. Cepheus was one of the 48 constellations listed by the second century astronomer Ptolemy, and it remains one of the 88 constellations in the modern times. The constellation's brightest star is Alpha Cephei, with an apparent magnitude of 2.5. Delta Cephei is the prototype of an important class of star known as a Cepheid variable.
"Radiance" was also promoted in Spears' music videos for "Hold It Against Me" (2011) and "Criminal" (2011). In 2011, it was revealed that "Radiance" was going to be spun-off into a flanker fragrance titled "Cosmic Radiance". With the tagline "Be the brightest star in the universe", the fragrance was released in August 2011, with an accompanying remix album by Spears released on October 7, 2011. "Cosmic Radiance" was created by Honorine Blanc and Harry Fremont.
Delta Crateris (δ Crt, δ Crateris; traditional name: Labrum) is a solitary star in the southern constellation of Crater. With an apparent visual magnitude of 3.56, it is the brightest star in this rather dim constellation. It has an annual parallax shift of 17.56 mas as measured from Earth, indicating Delta Crateris lies at a distance of 163 ± 4 light years from the Sun. This is an evolved orange-hued giant star belonging to the spectral class K0 III.
Beta Hydri (β Hyi, β Hydri) is a star in the southern circumpolar constellation of Hydrus. (Note that Hydrus is not the same as Hydra.) With an apparent visual magnitude of 2.8, this is the brightest star in the constellation. Based upon parallax measurements the distance to this star is about . This star has about 104% of the mass of the Sun and 181% of the Sun's radius, with more than three times the Sun's luminosity.
The core investment strategy of the company was then known as involving convergence trading: using quantitative models to exploit deviations from fair value in the relationships between liquid securities across nations and asset classes. In fixed income the company was involved in US Treasuries, Japanese Government Bonds, UK Gilts, Italian BTPs, and Latin American debt, although their activities were not confined to these markets or to government bonds.LTCM was the brightest star on Wall Street at that time.
Circinus is a faint constellation, with only one star brighter than fourth magnitude. Alpha Circini, a white main sequence star with an apparent magnitude of 3.19, is 54 light-years away and 4° south of Alpha Centauri. Not only the brightest star in the constellation, it is also the brightest example of a rapidly oscillating Ap (RoAp) star in the night sky. It has the unusual spectral type A7 Vp SrCrE, showing increased emissions of strontium, chromium and europium.
23 Vulpeculae is the second brightest star in the constellation. In 1967, the first pulsar, PSR B1919+21, was discovered in Vulpecula by Jocelyn Bell, supervised by Antony Hewish, in Cambridge. While they were searching for scintillation of radio signals of quasars, they observed pulses which repeated with a period of 1.3373 seconds. Terrestrial origin of the signal was ruled out because the time it took the object to reappear was a sidereal day instead of a solar day.
Entries for caelum and caelum. It is the eighth-smallest constellation, and subtends a solid angle of around 0.038 steradians, just less than that of Corona Australis. Due to its small size and location away from the plane of the Milky Way, Caelum is a rather barren constellation, with few objects of interest. The constellation's brightest star, Alpha Caeli, is only of magnitude 4.45, and only one other star, (Gamma) γ 1 Caeli, is brighter than magnitude 5 .
Dong was initially hesitant about being placed in a band but eventually warmed up to the other members. Choosing the stage-name Taeyang (meaning sun) because "the sun is the brightest star from the incalculable stars in the universe," Taeyang abandoned the idea of rapping to focus on singing. Following the release of several single albums, Big Bang's first album, Big Bang Vol. 1 – Since 2007, was a moderate success, and included Taeyang's first solo song "Ma Girl".
The constellation Lepus as it can be seen by the naked eye. There are a fair number of bright stars, both single and double, in Lepus. Alpha Leporis, the brightest star of Lepus, is a white supergiant of magnitude 2.6, 1300 light-years from Earth. Its traditional name, Arneb (أرنب ’arnab), means "hare" in Arabic. Beta Leporis, traditionally known as Nihal (Arabic for "quenching their thirst"), is a yellow giant of magnitude 2.8, 159 light-years from Earth.
Nu Puppis (ν Puppis) is a solitary, blue-hued star in the southern constellation of Puppis. It is the fifth-brightest star in Puppis, with an apparent visual magnitude of 3.17. Based upon an annual parallax shift of 8.78 mas as seen from Earth, it is located about 370 light years from the Sun. The system made its closest approach about 3.6 million years ago when it underwent perihelion passage at a distance of roughly 27 light years.
The following year, Niu played a supporting role in the popular historical romance drama Princess Agents, which led to increased recognition for the actor. In 2018, Niu played his first leading role in the youth campus drama Your Highness, The Class Monitor. He also played the male lead in the youth film Born to Be Wild. In 2019, Niu starred in the music romance drama The Brightest Star in the Sky as a talented singer who suffers numerous setbacks.
It is the brightest star of class O in the night sky. Alnitak Ab is a blue subgiant of spectral type B1IV with an absolute magnitude of -3.9 and an apparent magnitude of 4.3, discovered in 1998. A fourth star, 9th magnitude Alnitak C, has not been confirmed to be part of the Aa-Ab-B group, and may simply lie along the line of sight. The Alnitak system is bathed in the nebulosity of IC 434.
HD 85951 is the star's entry in the Henry Draper Catalogue and HR 3923 that in the Bright Star Catalogue. This was the brightest star in the now-obsolete constellation of Felis. In 2016, the IAU organized a Working Group on Star Names (WGSN) to catalog and standardize proper names for stars. The WGSN approved the name Felis for this star on 1 June 2018 and it is now so included in the List of IAU-approved Star Names.
Beta Indi, Latinized from β Indi, is the second brightest star in the southern constellation of Indus. It is visible to the naked eye as a faint, orange-hued point of light with an apparent visual magnitude of 3.67. The star is located approximately 600 light years from the Sun, based on parallax, but is drifting closer with a radial velocity of −5 km/s. The stellar classification of this star is K1II, matching an evolved bright giant.
TW Piscis Austrini can be seen close by and is possibly associated with Fomalhaut as it lies within a light-year of it. Of magnitude 6.5, it is a BY Draconis variable. The second brightest star in the constellation, Epsilon Piscis Austrini is a blue-white star of magnitude +4.17. Located 400 ± 20 light-years distant, it is a blue-white main sequence star 4.10 ± 0.19 times as massive as the Sun, and around 661 times as luminous.
Dalin gave a sketch of Swedish culture and history using language which had an unprecedented richness of sarcasm and irony. In the 1730s and 1740s, Dalin was unrivalled as the brightest star in the Swedish literary sky. He was the first to refine the language for practical purposes, in comparison with the laboured poetry of the 17th century, and he was the first author to be read and appreciated by the general public.Algulin, pp.39–41Gustafson, p.
Visible in the same field and as prominent as the red supergiants in infrared images is the carbon star MZ Cephei, which is much closer to us than NGC 7419. It is a slow irregular variable star with a range of 14.7 - 15.4. The visually brightest star in the core region of the cluster is a yellow giant, placed at around 500 parsecs by Gaia astrometry. The even brighter nearby star HD 216721 is also a foreground object.
Curious spiral around red giant star R Sculptoris. No stars brighter than 3rd magnitude are located in Sculptor. This is explained by the fact that Sculptor contains the south galactic pole where stellar density is very low. Overall, there are 56 stars within the constellation's borders brighter than or equal to apparent magnitude 6.5. The brightest star is Alpha Sculptoris, an SX Arietis-type variable star with a spectral type B7IIIp and an apparent magnitude of 4.3.
Geminiano Montanari. Geminiano Montanari (1 June 1633 – 13 October 1687) was an Italian astronomer, lens-maker, and proponent of the experimental approach to science. He is best known for his observation, made around 1667, that the second-brightest star (called Algol as derived from its name in Arabic) in the constellation of Perseus varied in brightness. It is likely that others had observed this effect before, but Montanari was the first named astronomer to record it.
Beta Doradus (Beta Dor, β Doradus, β Dor) is the second brightest star in the southern constellation of Dorado. It has a variable apparent visual magnitude, visible to the naked eye from the southern hemisphere. Based upon parallax measurements with the Hubble Space Telescope, it is located at a distance of from Earth. Beta Doradus is a Cepheid variable that regularly changes magnitude from a low of 4.08 to a high of 3.46 over a period of 9.842 days.
MY Camelopardalis (MY Cam) is a binary star system located in the Alicante 1 open cluster, some away in the constellation Camelopardalis. It is one of the most massive known binary star systems and a leading candidate for a massive star merger. MY Cam is the brightest star in Alicante 1. The system consists of two hot blue O-type stars with one component having a mass of 32 solar masses and the other 38 solar masses.
The RMC survey identified luminous objects in the Large Magellanic Cloud and one of the brightest was RMC 136. This is now commonly shortened to R136, which is now known to be an extremely young dense open cluster at the core of the NGC 2070 cluster in the Tarantula Nebula. R136 was eventually resolved and the brightest "star" at the centre was termed R136a. This was further resolved into multiple components, one of which is R136a3.
Lying near the constellation's northern border with Telescopium is Alpha Pavonis, the brightest star in Pavo. Its proper name — Peacock — is an English translation of the constellation's name. It was assigned by the British Her Majesty's Nautical Almanac Office in the late 1930s; the Royal Air Force insisted that all bright stars must have names, the star hitherto having lacked a proper name. Alpha has an apparent (or visual) magnitude of 1.91 and spectral type B2IV.
Since the 1975 Army reform Italian army aviation units are named for celestial objects: regiments are numbered with a single digit and named for stars in the 88 modern constellationss. Accordingly, an army aviation regiment's coat of arms highlights the name-giving star within its constellation. Squadron groups were numbered with two digits and named for constellations, or planets of the Solar System. The 7th Army Aviation Regiment was named for Vega the brightest star in the Lyra constellation.
Mu Tucanae was dropped by Francis Baily, who felt the star was too faint to warrant a designation, and Kappa's two components came to be known as Kappa1 and Kappa2. The layout of the brighter stars of Tucana has been likened to a kite. Within the constellation's boundaries are around 80 stars brighter than an apparent magnitude of 7. At an apparent magnitude of 2.86, Alpha Tucanae is the brightest star in the constellation and marks the toucan's head.
A few million years ago, ε Canis Majoris was much closer to the Sun than it is at present, causing it to be a much brighter star in the night sky. About 4.7 million years ago, Adhara was 34 light-years from the Sun, and was the brightest star in the sky with a magnitude of –3.99. No other star has attained this brightness since, nor will any other star attain this brightness for at least five million years.
Beta Volantis, Latinized from β Volantis, is the brightest star of the southern constellation of Volans. It has an apparent visual magnitude of 3.75, which is sufficiently bright to allow it to be viewed with the naked eye. Based upon an annual parallax shift of 30.33 mas as seen from Earth, its distance can be estimated as 107.5 light years from the Sun. The star is moving away from the Sun with a radial velocity of +27 km/s.
Illustration of the ε Carinae system Epsilon Carinae is located roughly from the Sun. Measurements during the Hipparcos mission give the pair an angular separation of 0.46 arcseconds with a difference in magnitude of 2.0. At their estimated distance, this angle is equivalent to a physical separation of around 4 astronomical units. The primary component has an apparent visual magnitude of 2.2, which by itself would still make it the third-brightest star in the constellation.
Other F-type stars include Procyon's primary star, the brightest star in the constellation Canis Minor. The supergiant pulsates, showing small variations in its brightness and spectral lines. The pulsations have been given periods of 67 and 123 days, with an amplitude of about 0.05 magnitudes. The profiles of many spectral lines show variations that would be expected from a pulsating spergiant, but it isn't clear if they have the same period as the brightness variations.
Alpha Aquarii (α Aquarii, abbreviated Alpha Aqr, α Aqr), officially named Sadalmelik , is a single star in the constellation of Aquarius. The apparent visual magnitude of 2.94 makes this the second-brightest star in Aquarius. Based upon parallax measurements made during the Hipparcos mission, it is located at a distance of roughly from the Sun. It forms the primary or 'A' component of a double star designated WDS J22058-0019 (the secondary or 'B' component is UCAC2 31789179).
The brightest star, Kappa Tucanae A, is a yellow-white F-type subgiant with an apparent magnitude of +5.0. Its binary companion, Kappa Tucanae B, has a magnitude of 7.74 and is located about 6″ away from the primary. It completes an orbit around the primary every 857 years. The other binary pair, the magnitude +7.8 C, and the magnitude +8.4 D, are closer to one another, at 1.12 arcseconds, or at least 23 astronomical units.
The last such eclipse occurred from 2009–2011, and it is hoped that the extensive observations that will likely be carried out may yield further insights into the nature of this system. Another eclipsing binary is Beta Lyrae, which is a semidetached binary star system in the constellation of Lyra. Other interesting binaries include 61 Cygni (a binary in the constellation Cygnus, composed of two K class (orange) main-sequence stars, 61 Cygni A and 61 Cygni B, which is known for its large proper motion), Procyon (the brightest star in the constellation Canis Minor and the eighth-brightest star in the night time sky, which is a binary consisting of the main star with a faint white dwarf companion), SS Lacertae (an eclipsing binary which stopped eclipsing), V907 Sco (an eclipsing binary which stopped, restarted, then stopped again) and BG Geminorum (an eclipsing binary which is thought to contain a black hole with a K0 star in orbit around it), 2MASS J18082002−5104378 (a binary in the "thin disk" of the Milky Way, and containing one of the oldest known stars).
Circinus is a small, faint constellation in the southern sky, first defined in 1756 by the French astronomer Nicolas-Louis de Lacaille. Its name is Latin for compass, referring to the drafting tool used for drawing circles (it should not be confused with Pyxis, a constellation that represents a mariner's compass which points north). Its brightest star is Alpha Circini, with an apparent magnitude of 3.19. Slightly variable, it is the brightest rapidly oscillating Ap star in the night sky.
Determining that the coordinates were wrong, he assigned the designation to another star. Kappa Horologii, too, was unable to be verified—although it most likely was the star HD 18292—and the name fell out of use. In 1879, American astronomer Benjamin Apthorp Gould assigned designations to what became Mu and Nu Horologii as he felt they were bright enough to warrant them. At magnitude 3.9, Alpha Horologii is the brightest star in the constellation, located 115 (±0.5) light-years from Earth.
There are 37 stars brighter than apparent magnitude 6.5 in the constellation; three are brighter than magnitude 4.5. 46 Leonis Minoris, an orange giant of magnitude 3.8, is located some 95 light-years from Earth. At magnitude 4.4, Beta Leonis Minoris is the second-brightest star and the only one in the constellation with a Bayer designation. It is a binary star, the brighter component of which is an orange giant and the fainter a yellow-white main sequence star.
The Homunculus was ejected in an enormous outburst from Eta Carinae. Light from this event reached Earth in 1841, when Eta Carinae briefly became the second-brightest star in the sky, after Sirius; the ejected gas and dust have since obscured much of its light. The near-supernova explosion produced two polar lobes, and a large but thin equatorial disk, all moving outward at up to . The Homunculus Nebula is a virtually unique structure, believed to result from the extremely young age.
These Grand Cru vineyards include Burgundy's most iconic, sought-after and expensive red wines, with Romanée-Conti of Domaine de la Romanée-Conti at the pinnacle: "There can be little doubt that in the firmament of the Cote de nuits, Vosne-Romanée is the brightest star."The Great Domaines of Burgundy by Remington Norman & Charles Taylor, Kyle Cathie, 2010, p.68 There is no Flagey-Échezeaux appellation; the village and Premier Cru vineyards of this commune are part of the Vosne-Romanée AOC.
31 Boötis is a single star in the northern constellation of Boötes, located 470 light years from the Sun. It is visible to the naked eye as a faint, yellow-hued star with an apparent visual magnitude of 4.86. The object is moving closer to the Earth with a heliocentric radial velocity of −16.5 km/s. It was known to be part of a constellation between Virgo and Boötes named Mons Maenalus, it was also the brightest star in the constellation.
28 Cygni is a single star in the northern constellation of Cygnus. It is a faint blue-white hued star but visible to the naked eye with an apparent visual magnitude of 4.93. The distance to 28 Cyg, as estimated from its annual parallax shift of , is around 620 light years. It has an absolute magnitude of −2.56, which means that if the star were just away it would be brighter than Sirius, the brightest star in the night sky.
Alpha Lacertae, Latinized from α Lacertae, is a single white-hued star in the constellation of Lacerta, located 103 light years from the Sun. It is the brightest star in Lacerta with an apparent visual magnitude of 3.76. The star is moving closer to the Earth with a heliocentric radial velocity of −4.5 km/s. This is an ordinary A-type main-sequence star with a stellar classification of A1 V, which indicates it is generating energy through hydrogen fusion at its core.
Maia , designated 20 Tauri (abbreviated 20 Tau), is a star in the constellation of Taurus. It is a blue giant of spectral type B8 III, a chemically peculiar star, and the prototype of the Maia variable class of variable star. Maia is the fourth-brightest star in the Pleiades open star cluster (Messier 45), after Alcyone, Atlas and Electra. It is surrounded by one of the brighter reflection nebulae within the Pleiades, designated NGC 1432 and sometimes called the Maia Nebula.
It is now so entered in the IAU Catalog of Star Names. 20 Tauri is the star's Flamsteed designation. Although it is about the 15th brightest star in Taurus, Maia does not have a Bayer designation, but does have the Bright Star Catalogue designation HR 1149 and the Henry Draper Catalogue designation HD 23408. It has been listed as double star WDS J03458+2422; one companion is a 14th magnitude star nearly away that is probably an unrelated background object.
Beta Circini, Latinized from β Circini, is an A-type main sequence star and is the second-brightest star in the constellation of Circinus. It has an apparent visual magnitude of approximately 4.069, which is bright enough to be viewed with the naked eye. Based upon an annual parallax shift of 35.17 mas as seen from the Earth, it is located about 93 light years from the Sun. With a stellar classification of A3 Va, this is an A-type main-sequence star.
This video sequence is based on an artist's impression of exocomets orbiting the star Beta Pictoris. Beta Pictoris (abbreviated β Pictoris or β Pic) is the second brightest star in the constellation Pictor. It is located 63.4 light years from the Solar System, and is 1.75 times as massive and 8.7 times as luminous as the Sun. The Beta Pictoris system is very young, only 20 to 26 million years old, although it is already in the main sequence stage of its evolution.
She finally gets her chance to meet Chihiro again, and during a discussion about the stars (in which Sakuya says that the star Alphard, the brightest star in the constellation Hydra, is her favorite), Chihiro suddenly exclaims that he hates Sakuya and disappears once again. Sakuya becomes even more troubled when, a few days later, Chihiro suddenly enrolls at her school and becomes a classmate. As the story goes on, Sakuya's feelings towards Chihiro grows, and Chihiro starts warming up to her.
In 2010, he competed in an international competition hosted by Tourisme Montréal to "search for the brightest star under the rainbow" and won the first annual Queer of the Year title. He partnered Steve Adams in an episode of Hot Pink Shorts: The Making Of in which they co- directed a short film within one day. In the one-hour show, they were given advice on how to proceed with the short. The result was the seven-minute short Just the Tip.
The two visibly distinguishable components of Albireo The large distance between the components, as well as their difference in color, make Albireo one of the easiest observable visual binaries. The brightest member, which is the third-brightest star in the constellation Cygnus, is actually a close binary itself. Also in the Cygnus constellation is Cygnus X-1, an X-ray source considered to be a black hole. It is a high-mass X-ray binary, with the optical counterpart being a variable star.
Lambda Muscae (λ Mus, λ Muscae), often catalogued HD 102249 or HIP 57363, is the fourth-brightest star in the Southern Hemisphere constellation of Musca (the Fly). Lambda Muscae visibly makes up the far end of the tail of the visual Musca constellation. It is a star in a dual system according to studies, and one of the stars catalogued in astronomer Johann Bayer's 1603 publications Uranometria. Lambda Muscae more recently has been recorded as having a stellar classification of A7III.
Beta Canum Venaticorum (β Canum Venaticorum, abbreviated Beta CVn, β CVn), also named Chara , is a G-type main-sequence star in the northern constellation of Canes Venatici. At an apparent visual magnitude of 4.26, it is the second-brightest star in the constellation. Based upon an annual parallax shift of 118.49 mas, this star is distant from the Sun. Along with the brighter star Cor Caroli, the pair form the "southern dog" in this constellation that represents hunting dogs.
Since the 1975 army reform Italian army aviation units are named for celestial objects: groupings, and later regiments, are numbered with a single digit and named for stars in the 88 modern constellationss. Accordingly an army aviation regiment's coat of arms highlights the name-giving star within its constellation. Squadron groups were numbered with two digits and named for constellations, or planets of the Solar System. The 1st Army Light Aviation Grouping was named for Antares the brightest star in the Scorpius () constellation.
Since the 1975 army reform Italian army aviation units are named for celestial objects: groupings, and later regiments, are numbered with a single digit and named for stars in the 88 modern constellations. Accordingly, an army aviation regiment's coat of arms highlights the name-giving star within its constellation. Squadron groups were numbered with two digits and named for constellations, or planets of the Solar System. The 5th Army Light Aviation Grouping was named for Rigel the brightest star in the Orion constellation.
Since the 1975 army reform Italian army aviation units are named for celestial objects: groupings, and later regiments, are numbered with a single digit and named for stars in the 88 modern constellationss. Accordingly an army aviation regiment's coat of arms highlights the name-giving star within its constellation. Squadron groups were numbered with two digits and named for constellations, or planets of the Solar System. The 4th Army Light Aviation Grouping was named for Altair the brightest star in the Aquila constellation.
Betelgeuse is the brightest near-infrared source in the sky with a J band magnitude of −2.99; only about 13% of the star's radiant energy is emitted as visible light. If human eyes were sensitive to radiation at all wavelengths, Betelgeuse would appear as the brightest star in the night sky. Various catalogues list up to nine faint visual companions to Betelgeuse. They are at distances of about one to four arc-minutes and all are fainter than 10th magnitude.
WR 25 is the brightest star in the image. The orange star to its left is a foreground object. The primary star of the WR 25 system is approximately 2.4 million times brighter than the Sun and illuminates the far southern end of the Trumpler 16 cluster. The model used to derive the stellar parameters is unsuitable for use in binary systems with the authors noting that the companion contributes more than 15% of the system luminosity, so the luminosity is highly uncertain.
This fleet of 61 cars had begun operation between Washington, D.C. and New York City on the Northeast Corridor in 1969 under Penn Central and quickly gained acceptance with the traveling public, despite various engineering problems. Writing in the mid-1970s, railroad historian John H. White Jr. described them as "Amtrak's brightest star." In 1973, Budd still had the tooling in place from the Metroliner order, meaning that any new order derived from that design could begin almost at once.
Since the 1975 Army reform Italian army aviation units are named for celestial objects: regiments are numbered with a single digit and named for stars in the 88 modern constellationss. Accordingly an army aviation regiment's coat of arms highlights the name-giving star within its constellation. Squadron groups were numbered with two digits and named for constellations, or planets of the Solar System. The 2nd Army Aviation Regiment was named for Sirius () the brightest star in the Canis Major constellation.
The net proper motion of Vega is , which results in angular movement of a degree every . In the Galactic coordinate system, the space velocity components of Vega are (U, V, W) = , for a net space velocity of . The radial component of this velocity—in the direction of the Sun—is , while the transverse velocity is . Although Vega is at present only the fifth-brightest star in the night sky, the star is slowly brightening as proper motion causes it to approach the Sun.
ESO 69-6, two merging galaxies with prominent long tails, photographed by the Hubble Space Telescope Triangulum Australe has few deep-sky objects—one open cluster and a few planetary nebulae and faint galaxies. NGC 6025 is an open cluster with about 30 stars ranging from 7th to 9th magnitude. Located 3 degrees north and 1 east of Beta Trianguli Australis, it lies about away and is about in diameter. Its brightest star is MQ Trianguli Australis at apparent magnitude 7.1.
Thus when Mao was renowned for his poetry, the North Koreans matched this by claiming that Kim Il-sung had written plays during the anti-Japanese struggle of the 1930s. Two plays that were allegedly written by Kim Il-sung are The Sea of Blood and The Flower Girl. Nonetheless, Kim Il-sung also wrote poems, such as one called "Brightest Star", written in 1992 to congratulate Kim Jong-il on behalf of the latter's birthday. Kim Il-sung also wrote song lyrics.
Elnath's absolute magnitude is -1.34, similar to another star in Taurus, Maia in the Pleiades star cluster. Like Maia, β Tauri is a B-class giant with a luminosity 700 times solar. It has evolved away from the main sequence to become a giant star, larger and cooler than when it was on the main sequence. However, being approximately 130 light-years distant compared to Maia's estimated 360 light-years, β Tauri ranks as the second-brightest star in the constellation.
Gnosia is Greek (from γνωσία in hellenistic common and γνῶσις in ancient Greek, which means knowledge), short for Gnōsia stella corōnæ "star of the crown of Knossos". Asteroth is Hebrew, עשתרות ‘ašterôt "Astarte (idols)" and mainly referred to the constellation. As the brightest star in Corona Borealis, it lent its name to Alphekka Meridiana, the brightest in the constellation of Corona Australis. The International Astronomical Union Working Group on Star Names (WGSN) has chosen Alphecca as the preferred formal name for this star.
Diagram of H. A. Rey's alternative way to connect the stars of the constellation Gemini. Twins are shown holding hands. Gemini is dominated by Castor and Pollux, two bright stars that appear relatively very closely together forming an o shape, encouraging the mythological link between the constellation and twinship. The twin above and to the right (as seen from the Northern Hemisphere) is Castor, whose brightest star is α Gem; it is a second-magnitude star and represents Castor's head.
Alpha Pictoris (α Pic, α Pictoris) is the brightest star in the southern constellation of Pictor. It has an apparent visual magnitude of 3.27, which is bright enough to be viewed from urban areas in the southern hemisphere. This star is close enough for its distance to be measured using parallax shifts, which yields a value of roughly from the Sun, with a 5% margin of error. Alpha Pictoris has the distinction of being the south pole star of the planet Mercury.
Pleione (pronounced or ) is a binary star and the seventh-brightest star in the Pleiades star cluster (Messier 45). It has the variable star designation BU Tauri (BU Tau) and the Flamsteed designation 28 Tauri (28 Tau). The star is located approximately from the Sun, appearing in the constellation of Taurus. Pleione is located close on the sky to the brighter star Atlas, so is difficult for stargazers to distinguish with the naked eye despite being a fifth magnitude star.
Boötes is a constellation in the northern sky, located between 0° and +60° declination, and 13 and 16 hours of right ascension on the celestial sphere. The name comes from the Greek Βοώτης, Boōtēs, meaning “herdsman” or “plowman” (literally, “ox-driver”; from βοῦς bous “cow”). One of the 48 constellations described by the 2nd-century astronomer Ptolemy, Boötes is now one of the 88 modern constellations. It contains the fourth-brightest star in the night sky, the orange giant Arcturus.
47 arcseconds, it is located roughly from the Sun. If the star were at a distance of , it would have a magnitude of +0.4 and be the third- brightest star in the night sky. This star has a stellar classification of G9 III, which indicates it is an evolved G-type giant star. It has an estimated 172% of the Sun's mass and has expanded to 12 times the radius of the Sun, from which it is shining with 64.6 times the solar luminosity.
" Along with the announcement, a marketing poster featuring the singer that shows the perfume bottle as being decorated with black and white jewels was also released. The tagline of the fragrance is "Be the brightest star in the universe". According to Fragantica, the composition of "Cosmic Radiance" "opens with strong and optimistic citruses, and a refreshing glittery red bouquet opening its fragrant petals in the very heart of the composition. Base notes twinkle and warm with notes of amber, soft vanilla and creamy sandalwood.
The rocket, named after Vega, the brightest star in the constellation Lyra, is a single-body launcher (no strap-on boosters) with three solid rocket stages: the P80 first stage, the Zefiro 23 second stage, and the Zefiro 9 third stage. The upper module is a liquid rocket called AVUM. The improved version of the P80 stage, the P120C, will be used as the side boosters of the Ariane 6. Italy is the leading contributor to the Vega program (65%), followed by France (13%).
The majority of the population consists of A and B type main sequence stars, the B type stars being the oldest members, and a number of G type giant stars. One yellow-hued G type star is the brightest star in M38 at a magnitude of 7.9. The brightest stars in M38 are magnitude 9 and 10. M38 is accompanied by NGC 1907, a smaller and dimmer cluster that lies half a degree south-southwest of M38; it is at a distance of 4,200 light-years.
French explorer and astronomer Nicolas-Louis de Lacaille gave Bayer designations to its stars in 1756, some of which had been previously considered part of the neighbouring constellation Piscis Austrinus. The constellations Grus, Pavo, Phoenix and Tucana are collectively known as the "Southern Birds". The constellation's brightest star, Alpha Gruis, is also known as Alnair and appears as a 1.7-magnitude blue-white star. Beta Gruis is a red giant variable star with a minimum magnitude of 2.3 and a maximum magnitude of 2.0.
From the equator to about the 40th parallel south it is visible low in the northern sky during the same (thus winter) months. Vega, Lyra's brightest star, is one of the brightest stars in the night sky, and forms a corner of the famed Summer Triangle asterism. Beta Lyrae is the prototype of a class of binary star known as Beta Lyrae variables. These binary stars are so close to each other that they become egg-shaped and material flows from one to the other.
South of Delta is Gamma Lyrae, a blue giant and the second-brightest star in the constellation. Around 190 parsecs distant, it has been referred to as a "superficially normal" star. The final star forming the lyre's figure is Beta Lyrae, also a binary composed of a blue bright giant and an early B-type star. In this case, the stars are so close together that the larger giant is overflowing its Roche lobe and transferring material to the secondary, forming a semidetached system.
16 Puppis is a suspected astrometric binary star system in the southern constellation of Puppis, and is located in the northernmost part of its constellation, almost due north of the bright star Rho Puppis, and east of Canis Major. It is visible to the naked eye as a faint, blue-white hued star with an apparent visual magnitude of 4.40. The star is located is approximately 465 light years away from the Sun based on parallax. It was the brightest star in Officina Typographica, an obsolete constellation.
The second brightest star is Scheat, a red giant of spectral type M2.5II-IIIe located around 196 light-years away from Earth. It has expanded until it is some 95 times as large, and has a total luminosity 1,500 times that of the Sun. Beta Pegasi is a semi-regular variable that varies from magnitude 2.31 to 2.74 over a period of 43.3 days. Markab and Algenib are blue-white stars of spectral types B9III and B2IV located 133 and 391 light-years distant respectively.
Every Gaelic family has its star and it is no reflection on his brothers to say that the brightest star in the Flannelly household was Mick. He is the most be-medalled Waterfod GAA player of all time having won 25 county medals in all grades: 15 county senior hurling, three minor hurling, 4 senior football and 3 junior football. He also captained Waterford to its second All-Ireland minor hurling title in 1948. In all, he played in 18 senior hurling county finals losing only three.
The series garnered over 5 billion views online during its run. In November, he was announced as one of the two leads in action drama Forward Forever alongside Jackson Yi. In 2018, Huang starred in Negotiator, a spin-off of the 2016 hit drama The Interpreter. The same year, he was cast in the youth period drama The Files of Teenagers in the Concession. In 2019, he acted as a Chinese pop star in the music romance youth drama The Brightest Star in the Sky.
In 40,000 years Voyager 2 will be within 1.7 ly of Ross 248 (another star which is approaching the Sun) and in 296,000 years it will pass within 4.6 ly of Sirius which is the brightest star in the night sky. The spacecraft are not expected to collide with a star for 1 sextillion (1020) years. In October 2020, astronomers reported a significant unexpected increase in density in the space beyond the Solar System as detected by the Voyager 1 and Voyager 2 space probes.
Overall, there are 41 stars within the constellation's borders with apparent magnitudes brighter than or equal to 6.5. With an apparent magnitude of 3.68, Alpha Pyxidis is the brightest star in the constellation. Located 880 ± 30 light-years distant from Earth, it is a blue-white giant star of spectral type B1.5III that is around 22,000 times as luminous as the Sun and has 9.4 ± 0.7 times its diameter. It began life with a mass 12.1 ± 0.6 times that of the Sun, almost 15 million years ago.
Alpha Librae (α Librae, abbreviated Alpha Lib, α Lib) is a double star and, despite its 'alpha' designation, it is the second-brightest star system (or star) in the constellation of Libra. The two components are designated α¹ Librae and α² Librae. The system bore the traditional name of Zubenelgenubi , though the International Astronomical Union now regards that name as only applying to α² Librae. Alpha² Librae is 0.33 degrees north of the ecliptic so it can be occulted by the Moon and (very rarely) by planets.
The Albireo system is a double star designated Beta Cygni (β Cygni, abbreviated Beta Cyg, β Cyg). The International Astronomical Union uses the name "Albireo" specifically for the brightest star in the system. Although designated 'beta', it is fainter than Gamma Cygni, Delta Cygni, and Epsilon Cygni and is the fifth-brightest point of light in the constellation of Cygnus. Appearing to the naked eye to be a single star of magnitude 3, viewing through even a low-magnification telescope resolves it into its two components.
Beta Andromedae (β Andromedae, abbreviated Beta And, β And), officially named Mirach , is a prominent star in the northern constellation of Andromeda. It is northeast of the Great Square of Pegasus and is theoretically visible to all observers north of 54° S. It is commonly used by stargazers to find the Andromeda Galaxy. The galaxy NGC 404, also known as Mirach's Ghost, is seven arc minutes away from Mirach. This star has an average apparent visual magnitude of 2.05, making it the brightest star in the constellation.
Its companion, almost 3 arcminutes away, is a 13th-magnitude star which may or may not be in orbit around Beta. The remaining member of the triangle is Gamma Trianguli Australis with an apparent magnitude of 2.87. It is an A-type main sequence star of spectral class A1 V, which lies away. Located outside the triangle near Beta, Delta Trianguli Australis is the fourth-brightest star at apparent magnitude +3.8. It is a yellow giant of spectral type G2Ib-II and lies away.
Telescopium is a minor constellation in the southern celestial hemisphere, one of twelve named in the 18th century by French astronomer Nicolas-Louis de Lacaille and one of several depicting scientific instruments. Its name is a Latinized form of the Greek word for telescope. Telescopium was later much reduced in size by Francis Baily and Benjamin Gould. The brightest star in the constellation is Alpha Telescopii, a blue-white subgiant with an apparent magnitude of 3.5, followed by the orange giant star Zeta Telescopii at magnitude 4.1.
Eta Ursae Majoris (Latinised from η Ursae Majoris, abbreviated Eta UMa, η UMa), formally named Alkaid , is a star in the constellation of Ursa Major. It is the most eastern (leftmost) star in the Big Dipper (or Plough) asterism. However, unlike most stars of the Big Dipper, it is not a member of the Ursa Major moving group. With an apparent visual magnitude of +1.84, it is the third-brightest star in the constellation and one of the brightest stars in the night sky.
Microscopium ("the Microscope") is a minor constellation in the southern celestial hemisphere, one of twelve created in the 18th century by French astronomer Nicolas-Louis de Lacaille and one of several depicting scientific instruments. The name is a Latinised form of the Greek word for microscope. Its stars are faint and hardly visible from most of the non-tropical Northern Hemisphere. The constellation's brightest star is Gamma Microscopii of apparent magnitude 4.68, a yellow giant 2.5 times the Sun's mass located 223 ± 8 light-years distant.
Thuban , designation Alpha Draconis (α Draconis, abbreviated Alpha Dra, α Dra), is a star (or star system) in the constellation of Draco. A relatively inconspicuous star in the night sky of the Northern Hemisphere, it is historically significant as having been the north pole star from the 4th to 2nd millennium BCE. Even though Johann Bayer gave Thuban the designation Alpha, its apparent magnitude of 3.65 means it is 3.7 times fainter than the brightest star in the constellation, Gamma Draconis (Eltanin), whose apparent magnitude is 2.24.
It is following an orbit through the Milky Way galaxy that has an eccentricity of 0.11, carrying it as close as to, and as far as from the galactic center. If Delta Scuti maintains its current movement and brightness, it will pass within 10 light-years of the solar system, becoming the brightest star in the sky between and . It will reach an apparent magnitude of -1.84, brighter than the current -1.46 of Sirius.Sky and Telescope, April 1998 (p60), based on computations from Hipparcos mission data.
Beta Virginis (β Virginis, abbreviated Beta Vir, β Vir), formally named Zavijava , is (despite its designation 'beta') the fifth-brightest star in the constellation of Virgo. Larger and more massive than the Sun, it is comparatively metal-rich (that is, it has a higher preponderance of elements heavier than helium). It is 0.69 degrees north of the ecliptic, so it can be occulted by the Moon and (rarely) by planets. The next planetary occultation of Zavijava will take place on 11 August 2069, by Venus.
Alpha Telescopii, Latinized from α Telescopii, is the brightest star in the southern constellation of Telescopium, with an apparent visual magnitude of 3.5. The ancient Roman astronomer Ptolemy included it in the constellation Corona Australis, but it was moved to Telescopium when that constellation was created by French astronomer Nicolas Louis de Lacaille in the 18th century. Parallax measurements put it at a distance of from Earth. At that range, the visual magnitude of the star is diminished by an extinction of 0.22 due to interstellar dust.
Marco Polo, during his visit to the Kakatiya Empire, allegedly called the temple "the brightest star in the galaxy of temples". Ramappa Temple stands majestically on a 6 ft high star-shaped platform. The hall in front of the sanctum has numerous carved pillars that have been positioned to create an effect that combines light and space wonderfully. The temple is named after the sculptor Ramappa, who built it, and is perhaps the only temple in India to be named after a craftsman who built it.
The Second Brightest Star was released on 23 June 2017 as a companion album to Folklore and Grimspound, including 40 minutes of new tracks that "explore landscapes, rivers and meeting places and take the listener on voyages of discovery across the world and to the stars" in addition to 30 minutes of extended material from Folklore and Grimspound. Big Big Train's most recent live performance was headlining The Night of the Prog festival in Lorelei, Germany, on 13 July 2018. A UK warm-up gig was played on 11 July 2018 at The Basingstoke Anvil.
Phi Sagittarii (Phi Sgr, φ Sagittarii, φ Sgr) is a star in the southern constellation of Sagittarius. With an apparent visual magnitude of 3.17, it is the ninth-brightest star in the constellation and is readily visible to the naked eye. Parallax measurements place it at a distance of roughly from the Earth. The stellar classification of this star has been rated at B8.5 III and B7 IV, with a luminosity class of III indicating it is a giant star, while a class of IV suggests it is still a subgiant star.
Neil J. Ormerod and Shane Clifton, Globalization and the Mission of the Church, Continuum International Publishing Group, 2010, , p. ix. AC Central - Alphacrucis College Parramatta Campus, 2014 On 27 April 2009 at the Australian Christian Churches National Conference, Southern Cross College officially changed its name to Alphacrucis. The new name derives from the star that sits at the foot of the Southern Cross constellation named Alpha Crucis. The principal, Stephen Fogarty, says, “Alphacrucis is the brightest star in the Southern Cross, and it’s at the foot of the cross.
Gamma Piscium (Gamma Psc, γ Piscium, γ Psc) is a star approximately 138 light years away from Earth, in the zodiac constellation of Pisces. It is a yellow star with a spectral type of G8 III, meaning it has a surface temperature of 4,833 K and is a giant star. It is slightly cooler than the Sun, yet it is 11 solar radii in size and shines with the light of 63 Suns. At an apparent magnitude of 3.7, it is the second brightest star in the constellation Pisces, between Eta and Alpha.
Her next film was Vishnu Avtar, released in 1921. De Liguoro also directed Dhruva Chartitra (1921), a mythological based on the legend of Dhruva whose quest for eternal knowledge and salvation was rewarded when he became the brightest star in the heavens, the pole star also known as Dhruvatara. The film was made as a bid for an international breakthrough for Madan Theatres and featured many Europeans in the cast along with Cooper who played the female lead, Suniti. One of Cooper's biggest successes was Pati Bhakti (1922).
Magiano follows Adelina's constellation and in the book it states: If you are very quiet and do not look away, you may see the brightest star in the constellation glow steadily brighter. It brightens until it overwhelms every other star in the sky, brightens until it seems to touch the ground, and then the glow is gone, and in its place is a girl. Her hair and lashes are painted a shifting silver, and a scar crosses one side of her face. She is dressed in Sealand silk and a necklace of sapphire .
Eta Carinae, surrounded by the Homunculus Nebula Within the large bright nebula is a much smaller feature, immediately surrounding Eta Carinae itself, known as the Homunculus Nebula (from Latin meaning Little Man). It is believed to have been ejected in an enormous outburst in 1841 which briefly made Eta Carinae the second-brightest star in the sky. The Homunculus Nebula is a small H II region, with gas shocked into ionised and excited states. It also absorbs much of the light from the extremely luminous central stellar system and re- radiates it as infrared (IR).
Because of its northern declination, Auriga is only visible in its entirety as far as 34° south; for observers farther south it lies partially or fully below the horizon. A large constellation, with an area of 657 square degrees, it is half the size of the largest, Hydra. Its brightest star, Capella, is an unusual multiple star system among the brightest stars in the night sky. Beta Aurigae is an interesting variable star in the constellation; Epsilon Aurigae, a nearby eclipsing binary with an unusually long period, has been studied intensively.
It has a mass of 1.28 solar masses and a radius of 1.32 solar radii. The star KELT-2A (HD 42176A) is the brightest star in Auriga known to host a transiting exoplanet, KELT-2Ab, and is the fifth- brightest transit hosting star overall. The brightness of the star KELT-2A allows the mass and radius of the planet KELT-2Ab to be known quite precisely. KELT-2Ab is 1.524 Jupiter masses and 1.290 Jupiter radii and on a 4.11-day- long orbit, making it another hot Jupiter, similar to HAT-P-9b.
It has an overall magnitude of 5.4 and a fairly large diameter of 14.0 arcseconds, classified as a Trumpler Class I 3 m cluster. The brightest star in the cluster is magnitude 8; there are approximately 12 stars of magnitude 9–10 and 20 stars of magnitude 11–13. A picture of NGC 1893 obtained by the Spitzer Space Telescope. An association of recently formed stars is surrounded by the nebula IC 410. NGC 1931 is a nebula in Auriga, slightly more than one degree to the west of M36.
Kepler's illustration of the 1604 supernova in the foot of Ophiuchus (the serpent-bearer) In October 1604, a new star was seen. By night, it was the brightest star in the sky, and it was visible during the day as well for more than three weeks, before eventually dimming. Both Lodovico delle Colombe and Kepler published their accounts of the new star in 1606. Van Heeck was ready to publish before them, sending his manuscript of De Nova Stella Disputatio ('Discussion of the New Star') to Federico Cesi in Rome in January 1605.
Stars of this type have oddly localised magnetic fields and are slightly variable. Alpha Circini forms a binary star system with an orange dwarf companion of spectral type K5 and magnitude 8.5, which with a separation of 5.7 arcseconds is only discernible with a telescope. The distance between the two stars is 260 AU and they take 2600 years to rotate around a common centre of gravity. The second brightest star is Beta Circini, a white main sequence star of spectral type A3Va and a magnitude of 4.07, about 100 light- years away.
The brighter stars, however, are not true members of the cluster, as they are closer to the Earth than the dimmer ones. NGC 5823 appears distinct to the observer, sometimes seen as a reversed "S", as described by John Herschel, although it has also been described as "tulip-shaped" and "boxy". That cluster can be easily mistaken with a similar cluster, NGC 5822, nearby in Lupus. Comparatively, open cluster NGC 5715 is fainter (integrated magnitude of 9.8)—its brightest star is only 11th magnitude—and smaller (7.0 arcminutes), comprising only 30 stars.
The constellation's brightest star—and the only one brighter than an apparent magnitude of 4—is Alpha Horologii (at 3.85), an ageing orange giant star that has swollen to around 11 times the diameter of the Sun. The long-period variable-brightness star, R Horologii (4.7 to 14.3), has one of the largest variations in brightness among all stars in the night sky visible to the unaided eye. Four star systems in the constellation are known to have exoplanets; at least one—Gliese 1061—contains an exoplanet in its habitable zone.
Canis Major is a prominent constellation because of its many bright stars. These include Sirius (Alpha Canis Majoris), the brightest star in the night sky, as well as three other stars above magnitude 2.0. Furthermore, two other stars are thought to have previously outshone all others in the night sky—Adhara (Epsilon Canis Majoris) shone at −3.99 around 4.7 million years ago, and Mirzam (Beta Canis Majoris) peaked at −3.65 around 4.42 million years ago. Another, NR Canis Majoris, will be brightest at magnitude −0.88 in about 2.87 million years' time.
Their name is a reference to Spica, the brightest star in the constellation of Virgo. On January 10, 2012, the group released their first digital single, "Doggedly" (독하게; also translated "Potently"). The music video sparked high interest, as their fellow label-mate Lee Hyori made an appearance.열애중 이효리, 그 치명적 매력 어디갈까. OSEN (January 3, 2012). Retrieved on March 23, 2012. On January 31, B2M Entertainment announced that the group would have their formal debut with a mini-album, titled Russian Roulette. The full-length music video was released on February 7.
Overall, there are 127 stars within the constellation's borders brighter than or equal to apparent magnitude 6.5. In his book Star Names and Their Meanings, R. H. Allen gave the names Yang Mun for Alpha Lupi, the brightest star in Lupus, and KeKwan for the blue giant Beta Lupi, both from Chinese. However, the first name is in error; both stars were part of a large Chinese constellation known in modern transliteration as Qíguān, the Imperial Guards. Most of the brightest stars in Lupus are massive members of the nearest OB association, Scorpius–Centaurus.
He numbered 89 stars (now with Flamsteed designations), though 6 and 11 turned out to be stars in Aquarius. Within the constellation's borders there are 177 stars of apparent magnitude 6.5 or greater. Epsilon Pegasi, also known as Enif, marks the horse's muzzle. The brightest star in Pegasus, is an orange supergiant of spectral type K21b that is around 12 times as massive as the Sun and is around 690 light-years distant from Earth. It is an irregular variable, its apparent magnitude varying between 2.37 and 2.45.
NGC 6940 has hundreds of members. The cluster is quite scattered and in between its members are also visible field stars. For example, two bright stars, an 8.6 mag B8III giant star at the NE edge and a 9.1 mag A0III giant at the SW corner of the cluster are too young to be true members of NGC 6940 and are probably background stars. The brightest star (lucida) of NGC 6940 is the red giant VG Vulpeculae, a semiregular variable star whose magnitude ranges from 9.0 to 9.5 every 80 days approximately.
According to a 1928 address by Charles M. Harger, heated debate in the first days of the capitol included the phrases, "justice for all," "Southern rights," "The flag and the Constitution," and heard for the first time were pleas for "Kansas, the brightest star of all". On July 4, the legislators passed their bill to move to Shawnee Mission, and quickly overrode the governor's veto of the measure. After adjourning on the sixth, they loaded up their property, and on horses and wagons headed for the new site, with the governor compelled to follow.
Alpha Apodis (Alpha Aps, α Apodis, α Aps) is the brightest star in the southern circumpolar constellation of Apus, with an apparent magnitude of approximately 3.825. It had the Greek alpha designation as part of the constellation which Johann Bayer called Apis Indica in his 1603 Uranometria star atlas. With a declination of –79°, this is a circumpolar star for much of the southern hemisphere. It can be identified on the night sky by drawing an imaginary line through Alpha Centauri and Alpha Circini then extending it toward the south celestial pole.
On December 13, 2007, NASA's Lunar Surface Access Module was retitled "Altair", after the 12th brightest star in the northern hemisphere's night sky, Altair in the constellation Aquila. In Latin, means "eagle", providing a connection to the first crewed lunar landing, Apollo 11's Eagle; the name Altair itself is a latinization of the Arabic , meaning "the eagle," "the bird," or "the flyer." Prior to the announcement of the "Altair" name, reports had suggested other names had been considered by NASA, but Altair won in a vote by the design team over Pegasus.
Delta Cygni (δ Cygni, abbreviated Delta Cyg, δ Cyg) is a binary star of a combined third-magnitude in the constellation of Cygnus. It is also part of the Northern Cross asterism whose brightest star is Deneb. Based upon parallax measurements obtained during the Hipparcos mission, Delta Cygni is located roughly distant from the Sun. Delta Cygni's two components are designated Delta Cygni A (officially named Fawaris ) and B. More widely separated is a faint third component, a 12th magnitude star that is moving along with the others.
Photograph of Telescopium Herschelii with constellations Gemini, Auriga, Perseus and the Pleiades Telescopium Herschelii on a celestial globe at the Herschel Museum of Astronomy, Bath Illustrated in Urania's Mirror (1825), next to Lynx Telescopium Herschelii (Latin for Herschel's telescope), also formerly known as Tubus Hershelli Major, is a former constellation in the northern celestial hemisphere. Maximilian Hell established it in 1789 to honour Sir William Herschel's discovery of the planet Uranus. It fell out of use by the end of the 19th century. Psi2 Aurigae at apparent magnitude 4.8 was the constellation's brightest star.
Li Shengjiao was born in 1935 in Nanjing, the then capital of China, in a distinguished family. His father Dr. Li Linsi was an educator and diplomat who enjoyed equal fame with Shanghai diplomat Wellington Koo, while his mother Tang Liling was a brilliant pianist who was considered by Italian pianist Mario Paci as "the brightest star of tomorrow". His family moved to Shanghai when he was two years old in 1937. He grew up in Shanghai and made a name for himself in the city for his talent.
According to Wang Ying, Li's classmate at Nanjing University and an academician of the Chinese Academy of Sciences, Li was widely regarded as "a leader of tomorrow" and "the brightest star of Nanjing University". Not only was Li considered a rare talent by Nanjing University professors, he also caught the attention of China's Ministry of Foreign Affairs. The ministry reserved a position for him even before his graduation. After he graduated with flying colors, the foreign ministry appointed a representative to invite him three times. He was then 21, the youngest in the ministry.
Huang Zitao (; born May 2, 1993), also known as Tao, is a Chinese singer- songwriter, rapper, actor, model and businessman. Huang is a former member of the South Korean-Chinese boy band Exo and its Chinese sub-unit, Exo-M. After leaving Exo, he made his solo debut in China in 2015 with the mini-album TAO, under the new stage name Z.Tao. Huang made his acting debut in the romantic movie You Are My Sunshine and later received recognition for his leading roles in Negotiator and The Brightest Star in the Sky.
The visible magnitude of R Doradus varies between 4.8 and 6.6, which means it is usually visible to the naked eye, but in the infrared it is one of the brightest stars in the sky. With a near-infrared J band magnitude of −2.6, only Betelgeuse at −2.9 is brighter. In the infrared K band, it is sometimes the brightest star in the sky, although usually Betelgeuse is brighter. It is classified as a semiregular variable star of type SRb, indicating giants with slow poorly- defined variations, often alternating between periodic and irregular brightness changes.
Capella was the brightest star in the night sky from 210,000 years ago to 160,000 years ago, at about −1.8 in apparent magnitude. At −1.1, Aldebaran was brightest before this period; it and Capella were situated rather close to each other in the sky and approximated boreal pole stars at the time. Capella is thought to be mentioned in an Akkadian inscription dating to the 20th century BC. Its goat-associated symbolism dates back to Mesopotamia as a constellation called "GAM", "Gamlum" or "MUL.GAM" in the 7th- century BC document MUL.APIN.
Huang Zitao (Z.TAO) at IS BLUE Concert in Shanghai, June 15, 2019In June 2017, Huang collaborated with Jonathan Anderson, LOEWE's creative director, on the "FIRE OF YOUTH" campaign, becoming the first Asian artist invited to collaborate with LOEWE. In July 2017, Hanhoo appointed Huang as their Brand Ambassador. The brand later partially sponsored The Brightest Star in the Sky, a hit drama of Huang with product placement in the drama. In September 2017, Huang was named Yves Saint Laurent's beauty ambassador and participated in the second season of YSL's web series Before the Light.
The Carina Nebula is at the very right edge of the frame (north is up) and V533 Car is the brightest star shown, near the open cluster NGC 3572. V533 Carinae is found near the Carina Nebula on the edge of the constellation Carina towards Crux. It is a member of Collinder 240, a sparse open cluster sometimes considered to be a portion of the richer nearby cluster NGC 3572. Together with the small clusters Hogg 10 and 11, they are all part of the Carina OB2 stellar association.
Alpha Doradus (Alpha Dor, α Doradus, α Dor) is the brightest star in the southern constellation of Dorado. The distance to this system, as measured using the parallax method, is about . This is a binary star system with an overall apparent visual magnitude that varies between 3.26 and 3.30, making this one of the brightest binary stars. The system consists of a subgiant star of spectral type B revolving around a giant star with spectral type A in an eccentric orbit with a period of about 12 years.
KELT-2A (also called KELT-2, HD 42176, or HD 42176A) is a yellow white dwarf star located about 440 light-years away in the constellation Auriga. The apparent magnitude of this star is 8.77, which means it is not visible to the naked eye but can be seen with a binoculars. KELT-2A is the brightest star in the common-proper-motion binary star system KELT-2 (HD 42176). KELT-2B is an early K dwarf approximately 295 AU away, which was discovered simultaneously with the planet KELT-2Ab.
Pollux , designated β Geminorum (Latinised to Beta Geminorum, abbreviated Beta Gem, β Gem), is an orange-hued evolved giant star about 34 light-years from the Sun in the constellation of Gemini. It is the brightest star in Gemini and the closest giant star to the Sun. Since 1943, the spectrum of this star has served as one of the stable anchor points by which other stars are classified. In 2006 an extrasolar planet (designated Pollux b or β Geminorum b, later named Thestias) was confirmed to be orbiting it.
Its light is dimmed by 30% due to interstellar dust, so would have a brighter magnitude of 3.31 if not for this. The second brightest star at magnitude 3.97 is Beta Pyxidis, a yellow bright giant or supergiant of spectral type G7Ib-II that is around 435 times as luminous as the Sun, lying 420 ± 10 light-years distant away from Earth. It has a companion star of magnitude 12.5 separated by 9 arcseconds. Gamma Pyxidis is a star of magnitude 4.02 that lies 207 ± 2 light- years distant.
Antlia is a faint constellation; its brightest star is Alpha Antliae, an orange giant that is a suspected variable star, ranging between apparent magnitudes 4.22 and 4.29. S Antliae is an eclipsing binary star system, changing in brightness as one star passes in front of the other. Sharing a common envelope, the stars are so close they will one day merge to form a single star. Two star systems with known exoplanets, HD 93083 and WASP-66, lie within Antlia, as do NGC 2997, a spiral galaxy, and the Antlia Dwarf Galaxy.
Ara (Latin: "the Altar"), the southern constellation between Scorpius, Telescopium, Triangulum Australe and Norma, was (as Βωμός (Bōmǒs)) one of the Greek bulk (namely 48) described by the 2nd-century astronomer Ptolemy, and it remains one of the 88 modern constellations defined by the International Astronomical Union. The orange supergiant Beta Arae, to us its brightest star measured with near-constant apparent magnitude of 2.85, is marginally brighter than blue-white Alpha Arae. Seven star systems are known to host planets. Sunlike Mu Arae hosts four known planets.
The separate components can be resolved with the naked eye. The fifth-brightest star is Zeta Apodis at magnitude 4.8, a star that has swollen and cooled to become an orange giant of spectral type K1III, with a surface temperature of 4649 K and a luminosity 133 times that of the Sun. It is 300 ± 4 light-years distant. Near Zeta is Iota Apodis, a binary star system 1,040 ± 60 light-years distant, that is composed of two blue-white main sequence stars that orbit each other every 59.32 years.
Mu Crucis, Latinized from μ Crucis, is the seventh-brightest star in the constellation Crux commonly known as the Southern Cross. μ Crucis is a wide double star of spectral class B stars, magnitude 4.0 and 5.2 respectively. They lie about 370 light-years away, and both stars are likely physically attached. The brighter component is known as μ1 Crucis or μ Crucis A, while the fainter is μ2 Crucis or μ Crucis B. μ1 Crucis is the brighter of the two stars with an apparent magnitude of 4.0.
At its faintest Betelgeuse can fall behind Deneb and Beta Crucis, themselves both slightly variable, to be the twentieth-brightest star. Betelgeuse has a B–V color index of 1.85—a figure which points to its pronounced "redness". The photosphere has an extended atmosphere, which displays strong lines of emission rather than absorption, a phenomenon that occurs when a star is surrounded by a thick gaseous envelope (rather than ionized). This extended gaseous atmosphere has been observed moving toward and away from Betelgeuse, depending on fluctuations in the photosphere.
Spica is the brightest star in the constellation of Virgo (lower left). As one of the nearest massive binary star systems to the Sun, Spica has been the subject of many observational studies. Spica is believed to be the star that gave Hipparchus the data that led him to discover the precession of the equinoxes. A temple to Menat (an early Hathor) at Thebes was oriented with reference to Spica when it was built in 3200 BC, and, over time, precession slowly but noticeably changed Spica's location relative to the temple.
This illusion can cause a misperception that such a light is on a collision course with the aircraft. Planets or stars in the night sky can often cause the illusion to occur. Often these bright stars or planets have been mistaken for landing lights of oncoming aircraft, satellites, or even UFOs. An example of a star that commonly causes this illusion is Sirius, which is the brightest star in the northern hemisphere and in winter appears over the entire continental United States at one to three fist-widths above the horizon.
Vela is a constellation in the southern sky. Its name is Latin for the sails of a ship, and it was originally part of a larger constellation, the ship Argo Navis, which was later divided into three parts, the others being Carina and Puppis. With an apparent magnitude of 1.8, its brightest star is the hot blue multiple star Gamma Velorum, one component of which is the brightest Wolf- Rayet star in the sky. Delta and Kappa Velorum, together with Epsilon and Iota Carinae, form the asterism known as the False Cross.
Vega is the brightest star in the constellation of Lyra α Lyrae (Latinised to Alpha Lyrae) is the star's Bayer designation. The traditional name Vega (earlier Wega) comes from a loose transliteration of the Arabic word ' meaning "falling" or "landing", via the phrase ', "the falling eagle". In 2016, the International Astronomical Union organized a Working Group on Star Names (WGSN) to catalog and standardize proper names for stars. The WGSN's first bulletin of July 2016 included a table of the first two batches of names approved by the WGSN; which included Vega for this star.
Its eccentric orbit around the Galaxy indicates that it may have originated in the Milky Way's thick disk. At least four of the fifteen stars visible to the unaided eye are orange giants of spectral class K. The second brightest star in the constellation—at apparent magnitude 4.1—is Zeta Telescopii, an orange subgiant of spectral type K1III-IV. Around 1.53 times as massive as the Sun, it shines with 512 times its luminosity. Located 127 light years away from Earth, it has been described as yellow or reddish in appearance.
Sydney Skelley (voiced by Dalila Bela (season 1), Vienna Leacock (in Back to Bortron 7-season 2-present)) is a girl with black hair and green eyes. She idolizes a character named Commander Cressida, named after the moon of Uranus, who has a dog named Sirius, named after the brightest star in Earth's night sky. Sydney is imaginative and very friendly, often acting as the voice of reason for the kids. In "How Come the Moon Changes Shape?" she danced with Jet, in "Kid Kart Derby" she hugged him.
The western portion of Hydra, with Alphard the brightest star near the centre Alphard has three times the mass of the Sun. Its estimated age is 420 million years and it has evolved away from the main sequence to become a giant star with a spectral classification of K3 and luminosity class between II and III. The angular diameter has been measured using long-baseline interferometry, yielding a value of milliarcseconds, only beaten in it by Betelgeuse and R Doradus. It has expanded to 50 times the radius of the Sun.
Gacrux , Gamma Crucis (Latinised from γ Crucis, abbreviated Gamma Cru, γ Cru), is the nearest class M giant star to the Sun. With an apparent visual magnitude of +1.63, it is the third-brightest star (hence its name) in the southern constellation of Crux (the Southern Cross) and is listed 26th of the brightest stars in the night sky. A line from the two "Pointers", Alpha Centauri through Beta Centauri, leads to within 1° north of this star. Distance has been determined using parallax measurements made during the Hipparcos mission, yielding from the Sun.
Jones was soon replaced by Dee Heron, who appeared on the single "Catch the Fire" (UK #54). Heron was replaced by Kymberley Peer for "Pressure" (UK #33), "Brightest Star" (UK #45), and a re-release of "Real Love" in 1995 (UK No. 24, their biggest hit since the original version of the track). Driza Bone also had a charting album in 1994, titled Conspiracy, which debuted and peaked at No. 72 on the UK Albums Chart in November of that year. All of their chart successes were released on the Fourth & Broadway record label.
Within the constellation's borders, there are 43 stars brighter than or equal to apparent magnitude 6.5. Depicting the eyepiece of the microscope is Gamma Microscopii, which—at magnitude of 4.68—is the brightest star in the constellation. Having spent much of its 620-million-year lifespan as a blue-white main sequence star, it has swollen and cooled to become a yellow giant of spectral type G6III, with a diameter ten times that of the Sun. Measurement of its parallax yields a distance of 223 ± 8 light years from Earth.
Tianshu (Chinese 天枢) is the ancient name of Dubhe, the brightest star of Plough. In Chinese classic literature, Dubhe is the metaphor for the virtue of an emperor. Imperial Immortal Nanming (Chinese 南明帝君): The god of the fortune of mortal empires Nanming (Chinese 南明) is the alias of a Chinese constellation and/or mythological animal Vermilion Bird (Chinese 朱雀). Stellar Immortal Taibai (Chinese 太白星君): Taibai is the Chinese name for Venus, the morning star and the star of the West in Chinese Culture.
9 Sgr is the brightest star in the image, just left of the intense Hourglass Nebula core of the Lagoon Nebula. NGC 6530 is the scattering of stars on the left. 9 Sgr is a naked eye star lying in the direction of the Lagoon Nebula (Messier 8), very close to the central condensation of the Hourglass Nebula around Herschel 36. It was not catalogued by Bayer with a Greek letter, but was listed by Flamsteed as number 9 in the constellation Sagittarius. It lies close to the open cluster NGC 6530.
Polaris, the brightest star in the constellation, is a yellow-white supergiant and the brightest Cepheid variable star in the night sky, ranging from an apparent magnitude of 1.97 to 2.00. Beta Ursae Minoris, also known as Kochab, is an aging star that has swollen and cooled to become an orange giant with an apparent magnitude of 2.08, only slightly fainter than Polaris. Kochab and magnitude 3 Gamma Ursae Minoris have been called the "guardians of the pole star". Planets have been detected orbiting four of the stars, including Kochab.
This is the brightest star in the vicinity of the open cluster NGC 2287, although it is probably not a member based on its proper motion. This star has a stellar classification of B7 II/III, matching a B-type giant/bright giant hybrid. (Cidale et al. (2007) show a class of B5 V, which would indicate it is instead a B-type main-sequence star.) It is a magnetic Bp star of the helium–weak variety (CP4), with the spectrum displaying evidence for vertical stratification of helium in the atmosphere.
The observatory is home the Dearborn 18 1/2 inch refractor, which was the largest telescope in the United States in the late 1860s. Due to the complicated history, it was operated from a different site at that time, and the original tube and mounting is at the Adler Planetarium since 1929. The 18 1/2 was used to discover Sirius B, a companion to the brightest star in the night sky. The 18 1/2 was the largest telescope in the Americas for many years until the U.S. Naval Observatory's 26-inch refractor.
Alpha Muscae (α Muscae, α Mus) is a star in the southern circumpolar constellation of Musca. With an apparent visual magnitude of +2.7, it is the brightest star in the constellation. The distance to this star has been determined using parallax measurements, giving an estimate of about from Earth. With a stellar classification of B2 IV-V, this star appears to be in the process of evolving away from the main sequence of stars like the Sun and turning a subgiant star, as the supply of hydrogen at its core becomes exhausted.
Beta Camelopardalis, Latinized from β Camelopardalis, is the brightest star in the northern constellation of Camelopardalis. It is bright enough to be faintly visible to the naked eye, having an apparent visual magnitude of 4.02. Based upon an annual parallax shift of 3.74 mas as seen from Earth, it is located roughly 870 light years from the Sun. It is moving closer with a radial velocity of −190 km/s and is most likely a single star. This is a yellow-hued G-type supergiant/bright giant with a stellar classification of G1 Ib–IIa.
The system was one of the first main-sequence eclipsing binaries containing G-type star to have its properties known as well as the better-studied early-type eclipsing binaries. At the very northernmost edge of the constellation is the even fainter V361 Lyrae, an eclipsing binary that does not easily fall into one of the traditional classes, with features of Beta Lyrae, W Ursae Majoris, and cataclysmic variables. It may be a representative of a very brief phase in which the system is transitioning into a contact binary. It can be found less than a degree away from the naked-eye star 16 Lyrae, a 5th-magnitude A-type subgiant located around 37 parsecs distant. The brightest star not included in the asterism and the westernmost cataloged by Bayer or Flamsteed is Kappa Lyrae, a typical red giant around 73 parsecs distant. Similar bright orange or red giants include the 4th-magnitude Theta Lyrae, Lambda Lyrae, and HD 173780. Lambda is located just south of Gamma, Theta is positioned in the east, and HD 173780, the brightest star in the constellation with no Bayer or Flamsteed designation, is more southernly. Just north of Theta and of almost exactly the same magnitude is Eta Lyrae, a blue subgiant with a near-solar metal abundance.
Since the 1975 army reform Italian army aviation units are named for celestial objects: regiments, are numbered with a single digit and named for stars in the 88 modern constellationss. Accordingly, an army aviation regiment's coat of arms highlights the name-giving star within its constellation. Squadron groups were numbered with two digits and named for constellations, or planets of the Solar System. The 3rd Special Operations Helicopter Regiment "Aldebaran" received its name and war flag from the disbanded 3rd Army Aviation Regiment "Aldebaran", which was named for Aldebaran the brightest star in the Taurus constellation.
It is bright enough to be seen with the naked eye and can be found around 9° to the east-southeast of the Large Magellanic Cloud. The brighter component, designated γ2 Volantis, is an orange K-type giant star with a stellar classification of K0 III and an apparent magnitude of +3.62, making this the brightest star in the constellation. Its companion, γ1 Volantis, is an F-type main-sequence star of classification F2 V and an apparent magnitude of +5.70. As of 2002, the pair were at an angular separation of 14.1″ along a position angle of 296°.
In the (sub)tropics it can be seen at its clearest from September to early November, and at low southern, tropical, latitudes of less than 25°S it can be seen, seasonally, low in the North. At magnitude 2.2, Alpha Cassiopeiae, or Schedar, is generally the brightest star in Cassiopeia, though it is occasionally outshone by the variable Gamma Cassiopeiae, which has reached magnitude 1.6. The constellation hosts some of the most luminous stars known, including the yellow hypergiants Rho Cassiopeiae and V509 Cassiopeiae and white hypergiant 6 Cassiopeiae. In 1572, Tycho Brahe's supernova flared brightly in Cassiopeia.
It is located about two degrees north of Beta Librae, the brightest star in the Libra constellation. Its mass is estimated to be approximately a third that of the Sun, and it is the 89th closest known star system to the Sun. An M-class dwarf star such as Gliese 581 has a much lower mass than the Sun, causing the core region of the star to fuse hydrogen at a significantly lower rate. From the apparent magnitude and distance, astronomers have estimated an effective temperature of 3200 K and a visual luminosity of 0.2% of that of the Sun.
AG Persei is another Algol variable in Perseus, whose primary component is a B-type main sequence star with an apparent magnitude of 6.69. Phi Persei is a double star, although the two components do not eclipse each other. The primary star is a Be star of spectral type B0.5, possibly a giant star, and the secondary companion is likely a stellar remnant. The secondary has a similar spectral type to O-type subdwarfs. With the historical name Mirfak (Arabic for elbow) or Algenib, Alpha Persei is the brightest star of this constellation with an apparent magnitude of 1.79.
HR 6135 is single star in the southern constellation of Apus, less than a degree from the northern constellation border with Triangulum Australe. Its declination of minus 70° 59.4' puts it just within 20 degrees of the southern celestial pole. The star has an orange hue and is faintly visible to the naked eye with an apparent visual magnitude of 5.50, making it the 12th-brightest star in the constellation. It is located at a distance of approximately 940 light years from the Sun based on parallax, but is drifting closer with a radial velocity of −9 km/s.
Also known as Altarf or Tarf, Beta Cancri is the brightest star in Cancer at apparent magnitude 3.5. Located 290 ± 30 light-years from Earth, it is a binary star system, its main component an orange giant of spectral type K4III that is varies slightly from a baseline magnitude of 3.53—dipping by 0.005 magnitude over a period of 6 days. An aging star, it has expanded to around 50 times the Sun's diameter and shines with 660 times its luminosity. It has a faint magnitude 14 red dwarf companion located 29 arcseconds away that takes 76,000 years to complete an orbit.
Released in July 2009, The Carte Noire Readers is a series of online Jackanory style films promoting the French coffee brand Carte Noire. It stars British actors Dominic West, Greg Wise and Dan Stevens reading love scenes from a variety of classic and modern Penguin novels. In March 2010 a new series was released featuring Joseph Fiennes to celebrate the launch of Carte Noire's new cappuccino product. The 10 films were released over a series of weeks, beginning with readings of Sense and Sensibility by Jane Austen, The Brightest Star in the Sky by Marian Keyes and Presumed Innocent by Scott Turow.
Pegasus is a constellation in the northern sky, named after the winged horse Pegasus in Greek mythology. It was one of the 48 constellations listed by the 2nd-century astronomer Ptolemy, and is one of the 88 constellations recognised today. With an apparent magnitude varying between 2.37 and 2.45, the brightest star in Pegasus is the orange supergiant Epsilon Pegasi, also known as Enif, which marks the horse's muzzle. Alpha (Markab), Beta (Scheat), and Gamma (Algenib), together with Alpha Andromedae (Alpheratz, once also designated Delta Pegasi) form the large asterism known as the Square of Pegasus.
Bode incorporated 76 stars into his new constellation, made up of 26 from Andromeda, 9 from Lacerta, 6 from Cepheus, 5 from Pegasus, and 3 from Cassiopeia. The three brightest stars—all of magnitude 4—that lay within its borders are Omicron, Lambda, and Kappa Andromedae. With an apparent magnitude of 3.62, Omicron Andromedae is a multiple star system, the brightest star of which is a blue-white subgiant of spectral type B6 IIIpe and its visible companion a white star of spectral type A2. Each appears to have a close companion, making it a quadruple system.
The brightest star of the bunch is the painter Ryabovsky, a handsome man who "had sold his last picture for five hundred roubles." Olga goes with him on a steamboat trip down the Volga river, and they become lovers. Dymov gradually becomes aware of what's happening and reacts with characteristic mildness... "That man crushes me with his magnanimity," Olga Ivanovna never tires to tell the people around her. He is almost sorry for his unfaithful wife, who soon indeed starts to suffer – from humiliation and jealousy, as Ryabovsky gets first bored, then exasperated with her overbearing company.
Alvan Graham Clark (July 10, 1832 – June 9, 1897) was an American astronomer and telescope-maker. Born in Fall River, Massachusetts, he was the son of Alvan Clark, founder of Alvan Clark & Sons. On January 31, 1862, while testing a new aperture great refractor telescope in Cambridgeport, Massachusetts, Clark made the first ever observation of a white dwarf star. This discovery of Sirius B, or affectionately "the Pup", proved an earlier hypotheses (Friedrich Bessel in 1844) that Sirius, the brightest star in the night sky with an apparent magnitude of −1.46, had an unseen companion disturbing its motion.
Visually it is over 10,000 times brighter than the Sun, but its high temperature means that most of its radiation is in the ultraviolet and its bolometric luminosity is over 500,000 times that of the Sun. It is also the 72nd brightest star in terms of apparent magnitude from Earth. Naos is typical of O-type stars in having an extremely strong stellar wind, measured at 2,500 km/s, which sees the star shed more than a millionth of its mass each year, or about 10 million times that shed by the Sun over a comparable time period.
Beta Arae (β Ara, β Arae), the brightest star in the constellation of Ara, is a very luminous, relatively young, giant star with an apparent visual magnitude of 2.8 (rounded). Parallax measurements place it at roughly from Earth. The spectrum of this star matches a stellar classification of K3 Ib- IIa, with the luminosity class notation 'Ib-IIa' indicating that the star lies part way between a higher luminosity bright giant (IIa) and a lower luminosity supergiant (Ib). This represents two of the evolutionary stages that a massive star passes through after it has exhausted the hydrogen at its core.
Alpha Reticuli (Alpha Ret, α Reticuli, α Ret) is the Bayer designation of the brightest star in the southern circumpolar constellation of Reticulum, with an apparent visual magnitude of 3.3. This appears to be a solitary star located at a distance of 162 light-years from Earth. Although it is bright enough to be seen with the naked eye, the declination of this star means that it is best viewed from the southern hemisphere and is only readily visible below the tropic of cancer. This star has more than three times the mass of the Sun and is about 330 million years old.
The designation of NGC 2264 in the New General Catalogue refers to both objects and not the nebula alone. The diffuse Cone Nebula, so named because of its apparent shape, lies in the southern part of NGC 2264, the northern part being the magnitude-3.9 Christmas Tree Cluster. It is in the northern part of Monoceros, just north of the midpoint of a line from Procyon to Betelgeuse. The cone's shape comes from a dark absorption nebula consisting of cold molecular hydrogen and dust in front of a faint emission nebula containing hydrogen ionized by S Monocerotis, the brightest star of NGC 2264.
Denebola , designated Beta Leonis (β Leonis, abbreviated Beta Leo, β Leo) is the second-brightest star in the zodiac constellation of Leo, although the two components of the γ Leonis double star, which are unresolved to the naked eye, have a combined magnitude brighter than it. Denebola is an A-type main sequence star with 75% more mass than the Sun and 15 times the Sun's luminosity. Based on parallax measurements from the Hipparcos astrometry satellite, the star is at a distance of about from the Sun. Its apparent visual magnitude is 2.14, making it readily visible to the naked eye.
Beta Chamaeleontis, Latinized from β Chamaeleontis, is the third-brightest star in the southern constellation of Chamaeleon. A solitary, suspected variable star, it is visible to the naked eye as a faint blue-white point of light with an apparent visual magnitude that has been measured ranging between 4.24 and 4.30. Parallax measurements yield a distance estimate of 298 light years from the Sun, and it is drifting further away with a radial velocity of +23 km/s. This is a B-type main-sequence star with a stellar classification of B4 V that is generating energy through core hydrogen fusion.
It first appeared on a 35-cm diameter celestial globe published in 1597 (or 1598) in Amsterdam by Plancius with Jodocus Hondius. The first depiction of this constellation in a celestial atlas was in Johann Bayer's Uranometria of 1603. De Houtman included it in his southern star catalog the same year under the Dutch name Den voghel Fenicx, "The Bird Phoenix", symbolising the phoenix of classical mythology. One name of the brightest star Alpha Phoenicis—Ankaa—is derived from the Arabic العنقاء al-‘anqā’ "the phoenix", and was coined sometime after 1800 in relation to the constellation.
Torchy, the Battery Boy, was created by Mr. Bumbledrop, a lonely old toymaker who spends the majority of his days tending to his garden, where the neighborhood children play. Torchy has a lamp on his head, and when he pushes a button on his jacket and utters a mysterious phrase, the light illuminates and gives Torchy magical insights. Mr. Bumbledrop also builds a cardboard rocket ship, which allows the boy to soar through the heavens. The brightest star in the night sky is Topsy Turvy Land, home of all of the abused and neglected toys that once belonged to naughty children.
Size comparison of Pollux (left) and The Sun (right) At an apparent visual magnitude of 1.14, Pollux is the brightest star in its constellation, even brighter than its neighbor Castor (α Geminorum). Pollux is 6.7 degrees north of the ecliptic, too far north to be occulted by the moon and planets, but in the distant future it will be close enough. Parallax measurements by the Hipparcos astrometry satellite place Pollux at a distance of about from the Sun. The star is larger than the Sun, with about two times its mass and almost nine times its radius.
Saiph , designation Kappa Orionis (κ Orionis, abbreviated Kappa Ori, κ Ori) and 53 Orionis (53 Ori), is the sixth-brightest star in the constellation of Orion. Of the four bright stars that compose Orion's main quadrangle, it is the star at the south-eastern corner. A northern-hemisphere observer facing south would see it at the lower left of Orion, and a southern-hemisphere observer facing north would see it at the upper right. Parallax measurements yield an estimated distance of 650 light-years (198 parsecs) from the Sun, which is about the same as Betelgeuse.
Fomalhaut , designation Alpha Piscis Austrini (α Piscis Austrini, abbreviated Alpha PsA, α PsA) is the brightest star in the constellation of Piscis Austrinus, the "Southern Fish", and one of the brightest stars in the sky. It is a class A star on the main sequence approximately from the Sun as measured by the Hipparcos astrometry satellite. Since 1943, the spectrum of this star has served as one of the stable anchor points by which other stars are classified. It is classified as a Vega-like star that emits excess infrared radiation, indicating it is surrounded by a circumstellar disk.
It is one of the largest constellations, with an area of 722 square degrees. This is over 1,400 times the size of the full moon, 55% of the size of the largest constellation, Hydra, and over 10 times the size of the smallest constellation, Crux. Its brightest star, Alpha Andromedae, is a binary star that has also been counted as a part of Pegasus, while Gamma Andromedae is a colorful binary and a popular target for amateur astronomers. Only marginally dimmer than Alpha, Beta Andromedae is a red giant, its color visible to the naked eye.
Acrux , designated α Crucis (Latinised to Alpha Crucis, abbreviated Alpha Cru, α Cru) is a multiple star system 321 light-years from the Sun in the constellation of Crux and part of the asterism known as the Southern Cross. With a combined visual magnitude of +0.76, it is the brightest object in Crux and the 13th brightest star in the night sky. It is the southernmost first- magnitude star, 2.3 degrees more southerly than Alpha Centauri. To the naked eye Acrux appears as a single star, but it is actually a multiple star system containing six components.
Since the 1975 army reform Italian army aviation units are named for celestial objects: support regiments are numbered with a single digit and named for one of the 88 modern constellationss. As in 1996 the 4th Army Aviation Repairs Unit was supporting the 1st Army Aviation Regiment "Antares", which was named for Antares, the brightest star in the Scorpius () constellation, the army decided to name the new 4th Army Aviation Support Regiment "Scorpione" to affirm the two regiment's relationship. As the regiment was founded in the city of Viterbo the regiment's coats of arms first quarter depicts Viterbo's coat of arms.
Since the 1975 army reform Italian army aviation units are named for celestial objects: support regiments are numbered with a single digit and named for one of the 88 modern constellationss. As in 1996 the 3rd Army Aviation Repairs Unit was supporting the 4th Army Aviation Regiment "Altair", which was named for Altair, the brightest star in the Aquila constellation, the army decided to name the new 2nd Army Aviation Support Regiment "Aquila" to affirm the two regiment's relationship. As the regiment was founded in the city of Bergamo the regiment's coats of arms fourth quarter depicts Bergamo's coat of arms.
Since the 1975 army reform Italian army aviation units are named for celestial objects: support regiments are numbered with a single digit and named for one of the 88 modern constellationss. As in 1996 the 2nd Army Aviation Repairs Unit was supporting the 5th Army Aviation Regiment "Rigel", which was named for Rigel, the brightest star in the Orion () constellation, the army decided to name the new 2nd Army Aviation Support Regiment "Orione" to affirm the two regiment's relationship. As the regiment was founded in the city of Bologna the regiment's coats of arms fourth quarter depicts Bologna's coat of arms.
Beta Herculis (β Herculis, abbreviated Beta Her, β Her), formally named Kornephoros , is a binary star and the brightest star in the northern constellation of Hercules at a base apparent visual magnitude of 2.81. This is a suspected variable star with an apparent magnitude that may rise as high as 2.76. Based upon parallax measurements, it is located at a distance of from the Sun. Although Beta Herculis appears to the naked eye to be a single star, in July 1899 the American astronomer W. W. Campbell discovered from spectroscopic measurements that its radial velocity varies, and concluded that it has a companion.
Gamma Draconis (γ Draconis, abbreviated Gamma Dra, γ Dra), formally named Eltanin , is a star in the northern constellation of Draco. Contrary to its gamma-designation (historically third-ranked), it is the brightest star in Draco at magnitude 2.4, outshining Beta Draconis by nearly half a magnitude and Alpha Draconis by over a magnitude. Gamma Draconis is at a distance of from the Sun, as determined by parallax measurements from the Hipparcos astrometry satellite. In 1728, while unsuccessfully attempting to measure the parallax of this star, the English astronomer James Bradley discovered the aberration of light resulting from the movement of the Earth.
Beta Mensae, Latinized from β Mensae, is the third-brightest star in the constellation of Mensa. Despite this, it is only faintly visible to the naked eye, appearing as a dim, yellow-hued point of light with an apparent visual magnitude of 5.31. The star is positioned near the southwest edge of the Large Magellanic Cloud, but it does not form part of this much more distant satellite galaxy. Based upon an annual parallax shift of just 4.11 mas as seen from the Earth, the star is located at a distance of roughly 790 light years from the Sun.
Alpha Andromedae is the brightest star in the constellation of Andromeda (right). α Andromedae (Latinised to Alpha Andromedae) is the star's Bayer designation. Ptolemy considered Alpha Andromedae to be shared by Pegasus, and Johann Bayer assigned it a designation in both constellations: Alpha Andromedae (α And) and Delta Pegasi (δ Peg). When the modern constellation boundaries were fixed in 1930, the latter designation dropped from use.Bayer’s Uranometria and Bayer letters The star bore the traditional names Alpheratz ( Merriam-Webster Dictionary 2017 -Alpheratz ) or Alpherat and Sirrah deriving from the Arabic name, سرة الفرس "the navel of the mare".
Gamma Scuti, Latinized from γ Scuti, is a single, white-hued star in the southern constellation of Scutum. The apparent visual magnitude of 4.67 indicates this is a dim star but visible to the naked eye. Based upon an annual parallax shift of 10.21 mas as seen from Earth, this star is located about 319 light years from the Sun. Currently it is moving towards the Solar System at 41 km/s, which means in 2.35 million years it will pass at just distance, probably becoming the brightest star in the night sky, at magnitude −2.1, for a period.
Beta Trianguli (Beta Tri, β Trianguli, β Tri) is the Bayer designation for a binary star system in the constellation Triangulum, located about 127 light years from Earth. Although the apparent magnitude is only 3.0, it is the brightest star in the constellation Triangulum. This is a double-lined spectroscopic binary star system with an orbital period of 31.39 days and an eccentricity of 0.53. The members are separated by a distance of less than 5 AU. The primary component has a stellar classification of A5IV, indicating that it has evolved away from the main sequence and is now a subgiant star.
Rigel (3,828 tons) was originally a motorship owned by the Bergen Steamship Company. The vessel was named after the brightest star in the Orion constellation. The ships had been requisitioned by the German occupation authorities in Norway in 1940 to transport Allied PoWs. According to Norwegian sources Rigel, under the command of Captain Heinrich Rhode with a German crew, sailed under the German flag from Bjerkvik on 21 November 1944 carrying 951 PoWs and 114 guards. At Narvik a further 349 PoWs were loaded plus 95 German deserters and 8 Norwegian prisoners arrested by the German police.
RR Lyrae is a variable star in the Lyra constellation, figuring in its west near to Cygnus. As the brightest star in its class, it became the eponym for the RR Lyrae variable class of stars and it has been extensively studied by astronomers. RR Lyrae variables serve as important standard candles that are used to measure astronomical distances. The period of pulsation of an RR Lyrae variable depends on its mass, luminosity and temperature, while the difference between the measured luminosity and the actual luminosity allows its distance to be determined via the inverse-square law.
The stars of Boötes were incorporated into many different Chinese constellations. Arcturus was part of the most prominent of these, variously designated as the celestial king's throne (Tian Wang) or the Blue Dragon's horn (Daijiao); the name Daijiao, meaning "great horn", is more common. Arcturus was given such importance in Chinese celestial mythology because of its status marking the beginning of the lunar calendar, as well as its status as the brightest star in the northern night sky. Two constellations flanked Daijiao: Yousheti to the right and Zuosheti to the left; they represented companions that orchestrated the seasons.
The constellation Cepheus as it may be seen by the naked eye Alpha Cephei, also known as Alderamin, is the brightest star in the constellation, with an apparent magnitude of 2.51. Delta Cephei is the prototype Cepheid variable, a yellow-hued supergiant star 980 light-years from Earth. It was discovered to be variable by John Goodricke in 1784. It varies between 3.5m and 4.4m over a period of 5 days and 9 hours. The Cepheids are a class of pulsating variable stars; Delta Cephei has a minimum size of 40 solar diameters and a maximum size of 46 solar diameters.
John Herschel immediately on arrival in South Africa in 1834 and 1835 re-observed all of the James Dunlop's double stars, but had troubles identifying them or finding significant differences in the measured positions of the stars. He first began with Alpha Crucis / Acrux, the brightest star in the constellation of Crux, also commonly known as the Southern Cross, then systematically searched for all the others. Herschel also was first to designate all the Dunlop double stars to begin with the Greek letter "Δ", which persists in many amateur observational references. Hence, bright southern doubles like p Eridani is known as Δ5, Gamma Crucis / Gacrux is Δ124, etc.
No star closer than Canopus is more luminous than it, and it has been the brightest star in Earth's night sky during three epochs over the past four million years. Other stars appear brighter only during relatively temporary periods, during which they are passing the Solar System much closer than Canopus. About 90,000 years ago, Sirius moved close enough that it became brighter than Canopus, and that will remain so for another 210,000 years. But in 480,000 years, as Sirius moves further away and appears fainter, Canopus will once again be the brightest, and will remain so for a period of about 510,000 years.
7 Sagittarii is the brightest star in the region of the Lagoon Nebula, towards the right edge. 7 Sagittarii is a massive star in the southern zodiac constellation of Sagittarius which is located in the Lagoon Nebula (NGC 6530), although multiple sources have considered it a foreground star. It is a dim star but visible to the naked eye with an apparent visual magnitude of 5.37. The distance to this star can be determined from the annual parallax shift of , yielding a value of roughly 1,100 light years. It is moving closer to the Sun with a heliocentric radial velocity of −11 km/s.
Some star atlases during the early 19th century also depicted Perseus holding the disembodied head of Medusa, whose asterism was named together as Perseus et Caput Medusae; however, this never came into popular usage. The galactic plane of the Milky Way passes through Perseus, whose brightest star is the yellow-white supergiant Alpha Persei (also called Mirfak), which shines at magnitude 1.79. It and many of the surrounding stars are members of an open cluster known as the Alpha Persei Cluster. The best-known star, however, is Algol (Beta Persei), linked with ominous legends because of its variability, which is noticeable to the naked eye.
Pictor also hosts RR Pictoris, a cataclysmic variable star system that flared up as a nova, reaching apparent (visual) magnitude 1.2 in 1925 before fading into obscurity. Pictor has attracted attention because of its second-brightest star Beta Pictoris, 63.4 light-years distant from Earth, which is surrounded by an unusual dust disk rich in carbon, as well as an exoplanet (extrasolar planet). Another five stars in the constellation have been observed to have planets. Among them is HD 40307, an orange dwarf that has six planets orbiting it, one of which—HD 40307 g—is a potential super- Earth in the circumstellar habitable zone.
Located about 97 light-years away from Earth, Alpha Pictoris is the brightest star in the constellation; it is a white main-sequence star with an apparent magnitude of 3.3, and spectral type A8VnkA6. A rapidly spinning star with a projected rotational velocity estimated at 206 km/s, it has a shell of circumstellar gas. Beta Pictoris is another white main sequence star of spectral type A6V and apparent magnitude 3.86. Located around 63.4 light-years distant from Earth, it is a member of the Beta Pictoris moving group—a group of 17 star systems around 12 million years old moving through space together.
The Ancient Greeks replaced the bow and arrow depiction with that of a dog. Sirius A, the brightest star in the night sky, lies in Canis Major. In Greek Mythology, Canis Major represented the dog Laelaps, a gift from Zeus to Europa; or sometimes the hound of Procris, Diana's nymph; or the one given by Aurora to Cephalus, so famed for its speed that Zeus elevated it to the sky. It was also considered to represent one of Orion's hunting dogs, pursuing Lepus the Hare or helping Orion fight Taurus the Bull; and is referred to in this way by Aratos, Homer and Hesiod.
In 2016, she appeared on the list of Forbes 30 Under 30 (Music), being the only Asian musician on the list. In the same year, she was asked to voice a lead role in the animated film Charming, alongside Demi Lovato, Ashley Tisdale, and Avril Lavigne. She also performed at Heroes of Remix (Chinese: 盖世英雄) that same year, singing EDM versions of songs such as Like You 《喜欢你》 and The Brightest Star In The Night Sky 《夜空中最亮的星》, among others. In September 2016, she released her photobook 25 Looks and an EP, which includes four remix songs.
Fomalhaut traditionally represents the mouth of the "fish", referring to its position in its constellation, Piscis Austrinus, "the southern fish" Fomalhaut (α Piscis Austrini) is a class A star on the main sequence approximately from the Sun. It is the brightest star in the constellation of Piscis Austrinus and at magnitude 1.2 is one of the brightest stars in the sky. Fomalhaut has a flare star companion called TW Piscis Austrini and a fainter red dwarf companion designated LP 876-10 or simply Fomalhaut C. There are several debris disks around the primary star as well as a proposed planet Fomalhaut b (also named Dagon).
Capricornus is a faint constellation, with only one star above magnitude 3; its alpha star has a magnitude of only 3.6. The brightest star in Capricornus is δ Capricorni, also called Deneb Algedi, with a magnitude of 2.9, located 39 light-years from Earth. Like several other stars such as Denebola and Deneb, it is named for the Arabic word for "tail" (deneb); its traditional name means "the tail of the goat". Deneb Algedi is a Beta Lyrae variable star (a type of eclipsing binary). It ranges by about 0.2 magnitudes with a period of 24.5 hours. The other bright stars in Capricornus range in magnitude from 3.1 to 5.1.
Sperry's aircraft had left Washington Airport at 9:10 pm EST on a flight to Nashville and was climbing to 20,000 ft. Weather conditions were clear, with the ground obscured by haze, and a full moon around 25° above the horizon. At approximately 9:30pm, seven miles west of Mount Vernon, copilot W. Gates alerted Sperry to a bright blue or bluish light ahead of them and increasing in size.Project Blue Book documents on Sperry case, NICAP (accessed 08-08-08) In a letter to Flying magazine several months later, Sperry described the light as "a brilliant, diffused, bluish light of fluorescent type [...] 25 times the magnitude of the brightest star".
Gamma Arae (γ Ara, γ Arae) is a star in the southern constellation of Ara. With an apparent visual magnitude of 3.3, it is the fourth-brightest star in the constellation and is readily visible to the naked eye. From parallax measurements made during the Hipparcos mission, the distance to this star can be estimated as from Earth. This is an enormous star with 23 times the radius of the Sun. It is radiating 120,000 as much energy as the Sun from its outer envelope at an effective temperature of 21,500 K. This heat gives the star the blue-white glow of a B-type star.
51 Andromedae, abbreviated 51 And and formally named Nembus , is the 5th brightest star in the northern constellation of Andromeda, very slightly dimmer than the Andromeda Galaxy also being of 4th magnitude. It is an orange K-type giant star with an apparent magnitude of +3.59 and is about 169 light- years from the Earth/solar system. It is traditionally depicted as one of the two northern, far upper ends of the mythological, chained-to-the-rocks princess, the other being binary star system Gamma Andromedae. At an estimated age of 1.7 billion years, this is an evolved red giant star with a stellar classification of .
The most famous member of this association is HR 8799 with four directly imaged planets. The association is named after the constellation Columba. The group was at first not recognized as an individual group, but stars within the group were first assigned to the Great Austral Young Association (GAYA), because it showed similar movement and distance compared with two nearby groups. Only later it became clear that GAYA is subdivided into three groups: the Tucana-Horologium association, the Carina association and the Columba association. The brightest star in the association is the massive star HD 32309, with a spectral type of B9Vann and an apparent magnitude of 4.90.
At the beginning of the "Keys to the Kingdom" segment, Phillip is set to leave the kingdom along with his father and Aurora's parents for two days for a Royal Conference, leaving Aurora to reign over it in their absence. Before departing, Phillip encourages Aurora to do a good job while in charge of the kingdom and tells her to look at the brightest star at night, as he will be doing the same. Phillip returns at the end of the segment and is part of the celebration for Aurora's duty. Phillip also appears in Disney/Square's Kingdom Hearts Birth by Sleep in his homeworld, "Enchanted Dominion".
Celestial historian Richard Allen noted that unlike the other constellations introduced by Plancius and La Caille, Phoenix has actual precedent in ancient astronomy, as the Arabs saw this formation as representing young ostriches, Al Ri'āl, or as a griffin or eagle. In addition, the same group of stars was sometimes imagined by the Arabs as a boat, Al Zaurak, on the nearby river Eridanus. He observed, "the introduction of a Phoenix into modern astronomy was, in a measure, by adoption rather than by invention." The Chinese incorporated Phoenix's brightest star, Ankaa (Alpha Phoenicis), and stars from the adjacent constellation Sculptor to depict Bakui, a net for catching birds.
It is a poor cluster and with no central concentration, with Trumpler class III1p. The core radius of the cluster is 1 parsec (3.3 light years), while the tidal radius is 5.1 parsecs (17 light years) and represents the average outer limit of NGC 2527, beyond which a star is unlikely to remain gravitationally bound to the cluster core. 37 stars, probable members of the cluster, are located within the central part of the cluster and 96 probable members are located within the angular radius of the cluster. The brightest star members are A-type stars, with the brightest being an A3 star with magnitude 9.38.
Antares , designated α Scorpii (Latinised to Alpha Scorpii, abbreviated Alpha Sco, α Sco), is on average the fifteenth-brightest star in the night sky, and the brightest object in the constellation of Scorpius. Distinctly reddish when viewed with the naked eye, Antares is a slow irregular variable star that ranges in brightness from apparent magnitude +0.6 to +1.6. Often referred to as "the heart of the scorpion", Antares is flanked by σ Scorpii and τ Scorpii near the center of the constellation. Classified as spectral type M1.5Iab-Ib, Antares is a red supergiant, a large evolved massive star and one of the largest stars visible to the naked eye.
Bayer gave eight stars Bayer designations, labelling them Alpha through to Theta, though he had never seen the constellation directly as it never rises above the horizon in Germany. After charting the southern constellations, French astronomer Nicolas-Louis de Lacaille recharted the stars of Ara from Alpha though to Sigma, including three pairs of stars next to each other as Epsilon, Kappa and Nu. Ara contains part of the Milky Way to the south of Scorpius and thus has rich star fields. Within the constellation's borders, there are 71 stars brighter than or equal to apparent magnitude 6.5. Just shading Alpha Arae, Beta Arae is the brightest star in the constellation.
See sources at Cygnus X-1 Sirius is another binary and the brightest star in the night time sky, with a visual apparent magnitude of −1.46. It is located in the constellation Canis Major. In 1844 Friedrich Bessel deduced that Sirius was a binary. In 1862 Alvan Graham Clark discovered the companion (Sirius B; the visible star is Sirius A). In 1915 astronomers at the Mount Wilson Observatory determined that Sirius B was a white dwarf, the first to be discovered. In 2005, using the Hubble Space Telescope, astronomers determined Sirius B to be in diameter, with a mass that is 98% of the Sun.
But the brightest star in the CD's constellation of talents was Seiji Ozawa. Conducting with precision, pointedness and more fantasy than Masur had supplied, he struck "an ideal balance between conveying the underlying strength of Mendelssohn's writing and bringing out the music's wide-eyed freshness, its delicacy and its gentle, slightly teasing sense of humour". His reading of the Overture, for example, was powerful and cogent, but he was alert to every detail of the score and it seemed as though he was conducting with a smile. The only charge that could be laid against him was that his pace in the Scherzo was slightly slower than some listeners might prefer.
AE And was the brightest star in M31 when it was first noticed during an outburst, at an apparent magnitude around 15, equivalent to an absolute magnitude of −10.2, or around a million times brighter than the Sun. This implies that the outburst may have increased the luminosity of the star, which would be unusual for an LBV. The temperature at that time is not known because of a lack of spectra or multiband photometry, but a typical LBV is around 8,000K during an outburst. Since the discovery outburst, AE And has mostly been in the quiescent, or hot, LBV phase, with small irregular brightness fluctuations.
Several of the album's track titles are titled or based on various historical figures and stories. In writing about the song in 2002, Roma pointed out that "Aldebaran" is named after the brightest star in the constellation of Taurus. In the Arabic language, the title translates to "the follower" as it follows the Pleiades cluster of stars, and the song is based on future Celtic people "passing Aldebaran on their journey to new territories, continuing their migratory pattern which was so predominant in their early history." The track was recorded in its entirety at Aigle Studio as Nicky expressed the difficulty in having to recreate the recording process elsewhere.
The "Star of Yoonir" is part of the Serer cosmos. It is very important and sacred and just one of many religious symbols in Serer religion and cosmology. It is the brightest star in the night sky, Sirius. With an ancient heritage of farming, "Yoonir" is very important and sacred in Serer religion,Berg, Elizabeth L., & Wan, Ruth, "Cultures of the World: Senegal", Benchmark Books (NY) (2009), p 144, Kalis, Simone, "Médecine Traditionnelle, Religion et Divination Chez les Seereer Siin du Sénégal" - La Coonaissance de la Nuit, L'Harmattan (1997), pp 25-60, because it announces the beginning of flooding and enables Serer farmers to start planting seeds.
In defining the constellation, Lacaille gave twelve stars Bayer designations of Alpha through to Lambda, with two close stars called Eta (one now known by its Henry Draper catalogue number), while Lambda was later dropped due to its dimness. The three brightest stars, Alpha, Beta and Gamma, make up the triangle. Readily identified by its orange hue, Alpha Trianguli Australis is a bright giant star of spectral type K2 IIb-IIIa with an apparent magnitude of +1.91 that is the 42nd-brightest star in the night sky. It lies away and has an absolute magnitude of −3.68 and is 5,500 times more luminous than our Sun.
NGC 2264 including the Cone Nebula and the Christmas Tree Cluster (upside down in this image) with S Monocerotis at the very top of the image (and the base of the Christmas tree) S Monocerotis, also known as 15 Monocerotis, is a massive multiple and variable star system located in the constellation Monoceros. It is the brightest star in the Christmas Tree open cluster in the area catalogued as NGC 2264. S Monocerotis is found within an open cluster and the Washington Double Star Catalog lists many companion stars. The closest and brightest is S Mon B, magnitude 7.8 and 3 arc seconds away.
Epsilon Canis Majoris (Latinised from ε Canis Majoris, abbreviated Epsilon CMa, ε CMa) is a binary star and, despite being designated ε (epsilon), the second-brightest object in the constellation of Canis Major and one of the brightest stars in the night sky with an apparent magnitude of 1.50. About 4.7 million years ago, it was the brightest star in the sky, with an apparent magnitude of −3.99. Based upon parallax measurements obtained during the Hipparcos mission, it is about 430 light-years distant from the Sun. The two components are themselves designated ε Canis Majoris A (also officially named Adhara , the traditional name of the system) and B.
The twin below and to the left is Pollux, whose brightest star is β Gem (more commonly called Pollux); it is of the first magnitude and represents Pollux's head. Furthermore, the other stars can be visualized as two parallel lines descending from the two main stars, making it look like two figures. H. A. Rey has suggested an alternative to the traditional visualization that connected the stars of Gemini to show twins holding hands. Pollux's torso is represented by the star υ Gem, Pollux's right hand by ι Gem, Pollux's left hand by κ Gem; all three of these stars are of the fourth magnitude.
Delta Capricorni (δ Capricorni, abbreviated Del Cap or δ Cap) is a multiple star system about 39 light-years away in the constellation of Capricornus (the Sea Goat). The primary star in the system is a white giant and the combined light of its members makes it the brightest star in the constellation. The system consists of an eclipsing binary, Delta Capricorni A, and two companion stars, B and C. A's two components are themselves designated Delta Capricorni Aa (formally named Deneb Algedi , the traditional name of the system) and Ab. Delta Capricorni is 2.6 degrees south of the ecliptic and can be occulted by the Moon, and (rarely) by planets.
An artist's impression of the tentative planet Epsilon Eridani b orbiting its parent sun The planetary systems of stars other than the Sun and the Solar System are a staple element in much science fiction. Epsilon Eridani is the fifth-brightest star (by apparent magnitude) in the riverine southern constellation of Eridanus. An orange star slightly smaller and less massive than the Sun, and relatively close to the Solar System, it is frequently featured in works of science fiction. It is classified as a type K2 star, with the corresponding suggestion that it has a stable habitable zone and is well suited for life.
In most constellations, Bayer assigned Greek and Latin letters to stars within a constellation in rough order of apparent brightness, from brightest to dimmest. Since the brightest star in a majority of constellations is designated Alpha (α), many people assume that Bayer meant to order the stars exclusively by brightness. In Bayer's day, however, stellar brightness could not be measured precisely. Stars were traditionally assigned to one of six magnitude classes (the brightest to first magnitude, the dimmest to sixth), and Bayer typically ordered stars within a constellation by class: all the first-magnitude stars, followed by all the second-magnitude stars, and so on.
The R136a system at the core of R136 is a dense luminous knot of stars containing at least 12 stars, the most prominent being R136a1, R136a2, and R136a3, all of which are extremely luminous and massive WN5h stars. R136a1 is separated from R136a2, the second brightest star in the cluster, by 5,000 AU. R136 is located approximately 157,000 light-years away from Earth in the Large Magellanic Cloud, positioned on the south-east corner of the galaxy at the centre of the Tarantula Nebula, also known as 30 Doradus. R136 itself is just the central condensation of the much larger NGC 2070 open cluster. For such a distant star, R136a1 is relatively unobscured by interstellar dust.
Although of a similar distance—around 302 light- years—to the stars of the Lower Centaurus Crux subgroup, it is moving much faster at around 100 km/s and does not share a common origin. To the northwest lies Mu Muscae, an orange giant of spectral type K4III that varies between apparent magnitude 4.71 and 4.76, and has been classified as a slow, irregular variable. Near Mu is Lambda Muscae, the third-brightest star in the constellation and a white main-sequence star of spectral type A7V around 128 light-years distant from Earth. Located near Alpha is R Muscae, a classical Cepheid variable ranging from apparent magnitude 5.93 to 6.73 over 7.5 days.
There are only three stars in the constellation brighter than magnitude 4.5, and 37 stars with a magnitude brighter than 6.5. Leo Minor does not have a star designated Alpha because Baily erred and allocated a Greek letter to only one star, Beta. It is unclear whether he intended to give 46 Leonis Minoris a Bayer designation, as he recognized Beta and 46 Leonis Minoris as of the appropriate brightness in his catalogue. He died before revising his proofs, which might explain this star's omission. At magnitude 3.8, the brightest star in Leo Minor is an orange giant of spectral class K0III named 46 Leonis Minoris or Praecipua; its colour is evident when seen through binoculars.
Also a flare star, Proxima has minutes-long outbursts where it brightens by over a magnitude. The Alpha couple revolve in 80-year periodicity and will next appear closest as seen from Earth's telescopes in 2037 and 2038, together as they appear to the naked eye they present the third-brightest "star" in the night sky. One other first magnitude star Beta Centauri is in the constellation in a position beyond Proxima and toward the narrow axis of Crux, thus with Alpha forming a far-south limb of the constellation. Also called Hadar and Agena, it is a double star; the primary is a blue-hued giant star of magnitude 0.6, 525 light-years from Earth.
The FK Com stars are giants of spectral type K with an unusually rapid rotation and signs of extreme activity. Their X-ray coronae are among the most luminous (LX ≥ 1032 erg·s−1 or 1025 W) and the hottest known with dominant temperatures up to 40 MK. However, the current popular hypothesis involves a merger of a close binary system in which the orbital angular momentum of the companion is transferred to the primary. Pollux is the brightest star in the constellation Gemini, despite its Beta designation, and the 17th brightest in the sky. Pollux is a giant orange K star that makes an interesting color contrast with its white "twin", Castor.
Stars are forming throughout the entire Cloud Complex, but most of the young stars are concentrated in dense clusters like the one illuminating the Orion Nebula. VISTA reveals many young stars and other objects. The current astronomical model for the nebula consists of an ionized (H II) region, roughly centered on Theta1 Orionis C, which lies on the side of an elongated molecular cloud in a cavity formed by the massive young stars. (Theta1 Orionis C emits 3-4 times as much photoionizing light as the next brightest star, Theta2 Orionis A.) The H II region has a temperature ranging up to 10,000 K, but this temperature falls dramatically near the edge of the nebula.
Diagram of Rho Geminorum and the four companions listed in the WDS The positions of the three stars in the Rho Geminorum system on the Hertzsprung-Russell diagram. As Rho Geminorum B does not have a known B-V or temperature, a line through its absolute magnitude is drawn instead. Rho Geminorum A is a bright star with a spectral type F0V, meaning that it is a main sequence that is over a thousand kelvins hotter, one-third more massive, two-thirds larger and five-and-a-half times more luminous than the Sun. With an apparent magnitude of 4.25, it is approximately the seventeenth- brightest star in the constellation of Gemini.
Precession of Earth's axis around the north ecliptical pole A consequence of the precession is a changing pole star. Currently Polaris is extremely well suited to mark the position of the north celestial pole, as Polaris is a moderately bright star with a visual magnitude of 2.1 (variable), and it is located about one degree from the pole, with no stars of similar brightness too close. Precession of Earth's axis around the south ecliptical pole The previous pole star was Kochab (Beta Ursae Minoris, β UMi, β Ursae Minoris), the brightest star in the bowl of the "Little Dipper", located 16 degrees from Polaris. It held that role from 1500 BC to AD 500.
Polaris (), designated α Ursae Minoris (Latinized to Alpha Ursae Minoris, abbreviated Alpha UMi, α UMi), commonly the North Star or Pole Star, is the brightest star in the constellation of Ursa Minor. It is very close to the north celestial pole, making it the current northern pole star. The revised Hipparcos parallax gives a distance to Polaris of about 433 light-years (133 parsecs), while calculations by other methods derive distances around 30% closer. Polaris is a triple star system, composed of the primary star, Polaris Aa (a yellow supergiant), in orbit with a smaller companion (Polaris Ab); the pair in orbit with Polaris B (discovered in August 1779 by William Herschel).
In May (moderate northern latitudes) or June (southern latitudes), the red supergiant can be seen briefly on the western horizon after sunset, reappearing again a few months later on the eastern horizon before sunrise. In the intermediate period (June–July), it is invisible to the naked eye (visible only with a telescope in daylight), except around midday in Antarctic regions between 70° and 80° south latitude (during polar night, when the Sun is below the horizon). Betelgeuse is a variable star whose visual magnitude ranges between 0.0 and +1.6. There are periods when it will surpass Rigel to become the sixth brightest star, and occasionally it will be even brighter than Capella.
Alpha Andromedae (α Andromedae, abbreviated Alpha And or α And), officially named Alpheratz , is located 97 light-years from the Sun and is the brightest star in the constellation of Andromeda. Located immediately northeast of the constellation of Pegasus, it is the upper left star of the Great Square of Pegasus. Although it appears to the naked eye as a single star, with overall apparent visual magnitude +2.06, it is actually a binary system composed of two stars in close orbit. The chemical composition of the brighter of the two stars is unusual as it is a mercury-manganese star whose atmosphere contains abnormally high levels of mercury, manganese, and other elements, including gallium and xenon.
Westerlund 1 in infrared from 2MASS Westerlund 1 was discovered by Bengt Westerlund in 1961 during an infrared survey in the Zone of Avoidance of the sky, and described as "a heavily reddened cluster in Ara". The spectral types of the component stars could not be determined at the time except for the brightest star which was tentatively considered type M. In 1969, Borgman, Kornneef, and Slingerland conducted a photometric survey of the cluster and assigned letters to the stars they measured. This star, identified as a strong radio source, was given the letter "A". This leads to the designation Westerlund-1 BKS A used at Simbad, although the cluster was not known as Westerlund 1 at that time.
Like its northern counterpart, the Southern Pleiades spans a sizeable area of sky, approximately 50 arcminutes, so it is best viewed with large binoculars or telescope with a wide-angle eyepiece. θ Carinae is the brightest star within the open cluster, with the apparent visual magnitude of +2.74. p Carinae (PP Carinae) is another third-magnitude star known to be a member of IC 2602, although it lies well outside the main visible grouping of stars. All the other members the cluster are of the fifth magnitude and fainter, but several are naked-eye objects, including HR 4196 (V518 Car), HR 4204, HR 4205, HR 4219, HR 4220, HR 4222, HD 92536, HD 93738, and V364 Carinae.
The constellation Canis Minor as it can be seen by the naked eye. Canis Minor contains only two stars brighter than fourth magnitude. At magnitude 0.34, Procyon, or Alpha Canis Minoris, is the seventh-brightest star in the night sky, as well as one of the closest. Its name means "before the dog" or "preceding the dog" in Greek, as it rises an hour before the "Dog Star", Sirius, of Canis Major. It is a binary star system, consisting of a yellow-white main sequence star of spectral type F5 IV-V, named Procyon A, and a faint white dwarf companion of spectral type DA, named Procyon B. Procyon B, which orbits the more massive star every 41 years, is of magnitude 10.7.
It is moving closer, having a heliocentric radial velocity of −18 km/s, and will approach to within in 1.879 million years. It is an A-type main-sequence star with a stellar classification of A2 V. It is a suspected variable star with a very small amplitude. 50 Cas has an estimated 2.56 times the mass of the Sun, and about 2.5 times the Sun's radius. It is radiating 64 times the Sun's luminosity from its photosphere at an effective temperature of around 9,376 K. The star was the brightest star in the occasionally used 1775 to 19th century constellation Custos Messium, typically drawn as a depiction of Charles Messier standing on top of the giraffe (Camelopardus), between Cepheus and Cassiopeia.
He died of a heart attack in his home in Austin at the age of 77. His earliest work had concerned the planet Mars and while at Harvard he used telescope observations from 1909 to 1958 to study the areographic coordinates of features on the surface of Mars. His later work focused on the study of galaxies and he co-authored the Third Reference Catalogue of Bright Galaxies with his wife Antoinette (1921-1987), a fellow UT Austin astronomer and lifelong collaborator.Memoriam to Antoinette de Vaucouleurs from University of Texas Austin His specialty included reanalyzing Hubble and Sandage's galaxy atlas and recomputing the distance measurements utilizing a method of averaging many different kinds of metrics such as luminosity, the diameters of ring galaxies, brightest star clusters, etc.
It produces the region's most celebrated wines, all made entirely from the Pinot noir grape: "There can be little doubt that in the firmament of the Cote de nuits, Vosne-Romanée is the brightest star"The Great Domaines of Burgundy by Remington Norman & Charles Taylor, Kyle Cathie, 2010, p.68 Despite the monopoly control of four of the six grand crus, the village has at least forty growers sharing its vineyards. The wines produced from the vineyards are diverse, but they are generally considered to be rich, silky and well balanced, with a complexity which surpasses that of the other wines of Burgundy. In addition to many excellent wines at both the village and premier cru level, the village has six grand crus.
Eta Carinae (η Carinae, abbreviated to η Car), formerly known as Eta Argus, is a stellar system containing at least two stars with a combined luminosity greater than five million times that of the Sun, located around 7,500 light- years (2,300 parsecs) distant in the constellation Carina. Previously a 4th- magnitude star, it brightened in 1837 to become brighter than Rigel, marking the start of its so-called "Great Eruption". It became the second-brightest star in the sky between 11 and 14 March 1843 before fading well below naked eye visibility after 1856. In a smaller eruption, it reached 6th magnitude in 1892 before fading again. It has brightened consistently since about 1940, becoming brighter than magnitude 4.5 by 2014.
In September 2010, Gülşen became one of the signatories of a project initiated by the Istanbul Metropolitan Municipality under the slogan 'Let the Light within Me Be the Light for You', to help the old residents of hospices across the country and raise awareness about their issues. Gülşen, who has a passion for working on social projects, wrote and voiced a song for UNICEF's Stars of Istanbul education project in 2011, titled "En Parlak Yıldız (The Brightest Star)". In 2012, she went on tour for 8 days with The New York Gypsy All-Stars in five different cities in the United States, performing music in America. The artist met with Turkish Americans in Boston, New York City, Washington, D.C., Chicago and New Jersey.
Alpha Pegasi (α Pegasi, abbreviated Alpha Peg, α Peg), formally named Markab , is the third-brightest star in the constellation of Pegasus and one of the four stars in the asterism known as the Great Square of Pegasus. α Pegasi (Latinised to Alpha Pegasi) is the star's Bayer designation. It bore the traditional name Markab (or Marchab), which derived from an Arabic word مركب markab "the saddle of the horse", or is mistranscription of Mankib, which itself comes from an Arabic phrase منكب الفرس Mankib al-Faras "(the Star of) the Shoulder (of the Constellation) of the Horse" for Beta Pegasi. Markab has a stellar classification of A0 IV, indicating that it is an A-type subgiant star that has exhausted the hydrogen at its core and has evolved beyond the main sequence.
Achernar is the primary (or 'A') component of the binary system designated Alpha Eridani (α Eridani, abbreviated Alpha Eri, α Eri), which is the brightest star in the constellation of Eridanus, and the ninth-brightest in the night sky. The two components are designated Alpha Eridani A (the primary) and B (the secondary, also known informally as Achernar B). As determined by the Hipparcos astrometry satellite, it is approximately from the Sun. Of the ten apparent brightest stars in the night-time sky, Alpha Eridani is the hottest and bluest in color, due to Achernar being of spectral type B. Achernar has an unusually rapid rotational velocity, causing it to become oblate in shape. The secondary is smaller, of spectral type A, and orbits Achernar at a distance of roughly 12 astronomical units (AU).
Two years after the success of Stargazing Dog, Takashi Murakami wrote three more stories: Twin Star, The Brightest Star and a final epilogue to the series. The three were collected and published by Futabasha in a second volume titled Zoku Hoshi Mamoru Inu (Stargazing Dog's Family), which narrates the individual stories of two characters who originally appeared in Stargazing Dog: Happie's fragile brother Chibi, and Tetsuo, the boy who stole Daddy's wallet respectively. In Twin Star, we discover that Happie was chosen by Miku as her pet for being an hyperactive healthy dog, while his brother Chibi was discarded due to his delicate and sickly look. The dog was born with a heart condition, so is left to die in a cardboard box, but later adopted by Mrs.
Nagano, an old grumpy and unfriendly woman who also has delicate health. The woman thinks the puppy could be a good companion until both die due to their respective sickness, but instead both gradually improved their health condition, become a happy couple and finds a better and long life together despite their shortcomings, which makes this the exact opposite of Daddy and Happie story. In Brightest Star it is revealed that Tetsuo is the child of a single mother, abused and despised by her, so he decides to cross the country alone looking for his grandfather who lives in Hokkaido, since he is the only living person among his relatives who ever showed some affection for him. After spending a couple of days enjoying the company of Happie, the kid decides to "adopt" a dog.
The Summer Triangle The 19th brightest star in the night sky, Deneb culminates each year on October 23 at 6 PM and September 7 at 9 PM, corresponding to summer evenings in the northern hemisphere. It never dips below the horizon at or above 45° north latitude, just grazing the northern horizon at its lowest point at such locations as Minneapolis, Montréal and Turin. In the southern hemisphere, Deneb is not visible south of 45° parallel south, so it just barely rises above the horizon in South Africa, southern Australia, and northern New Zealand during the southern winter. Deneb is located at the tip of the Northern Cross asterism made up of the brightest stars in Cygnus, the others being Albireo (Beta Cygni), Gamma Cygni, Delta Cygni, and Epsilon Cygni.
Lucky McKee and Chris Sivertson co-wrote and directed the film, hailed as a monster midnight sensation in the Toronto International Film Festival. Programmed by Ryan Darbonne and Bears Fonte, the 20th anniversary lineup featured more world and U.S. premieres than ever before in the festival's history. Overall, the 2013 festival included 28 world premiere features: Cavemen, Finding Neighbors, Jack, Jules, Esther and Me, The Odd Way Home, Siren, Dog Days, Living Dolls, Political Bodies, Take Away One, 120 Days, La Navaja de Don Juan, Brightest Star, Coffee, Kill Boss, Mop King, Blood Punch, Dark Mountain, Innocence, Dug Up, Dear Sidewalk, The Road to Livingston, Sombras de Azul, Always Learning, The Bloc, The Fable of Shannon Cable, Handy, Not Safe For Work, Speak Now, and 3 References, as well as another 8 US premieres.
Technical Memorandum 33-507 – A Reduced Star Catalog Containing 537 Named Stars, NASA-CR-124573 (1971). Many of the proper names that remain in use in modern astronomy are based on Arabic star names from medieval Islamic astronomy, which in turn was substantially based on Claudius Ptolemy’s Almagest, which contained the original Greek and Latin names for stars. For example, the Arabs translated Opisthen (Οπισθεν "after" or "following") or Opiso (Οπισω "to follow after"), one of the original Greek names for the brightest star in Taurus, as Aldebaran (الدبران), which means "the Follower" in Arabic, because the star always follows behind the Pleiades as both move across the sky. Most proper names for stars, especially the Arabic names, are descriptive of the locations of the stars within their parent constellations.
The German cartographer Johann Bayer used the Greek letters alpha to theta to label the most prominent stars in the constellation, while his countryman Johann Elert Bode subsequently added iota to phi. Only lambda and pi remain in use, likely because of their proximity to the north celestial pole. Within the constellation's borders, there are 39 stars brighter than or equal to apparent magnitude 6.5. Marking the Little Bear's tail, Polaris, or Alpha Ursae Minoris, is the brightest star in the constellation, varying between apparent magnitude 1.97 and 2.00 over a period of 3.97 days. Located around 432 light-years away from Earth, it is a yellow- white supergiant that varies between spectral types F7Ib and F8Ib, and has around 6 times the Sun's mass, 2,500 times its luminosity and 45 times its radius.
NGC 206 is the richest and most conspicuous star cloud in the Andromeda Galaxy as well as one of the largest and brightest star formation regions of the Local Group. It contains more than 300 stars brighter than Mb=−3.6. It was originally identified by Edwin Hubble as a star cluster but today, due to its size, it is classified as an OB association. NGC 206 is located in a spiral arm of the Andromeda Galaxy, in a zone free of neutral hydrogen and has a double structure, with one region that has an age of around 10 million years and includes several H II regions in one of its borders and other with an age of between 40 million years and 50 million years that includes a number of cepheids.
Keyzer and de Houtman assigned fifteen stars to the constellation in their Malay and Madagascan vocabulary, with a star that would be later designated as Alpha Hydri marking the head, Gamma the chest and a number of stars that were later allocated to Tucana, Reticulum, Mensa and Horologium marking the body and tail. Lacaille charted and designated 20 stars with the Bayer designations Alpha through to Tau in 1756. Of these, he used the designations Eta, Pi and Tau twice each, for three sets of two stars close together, and omitted Omicron and Xi. He assigned Rho to a star that subsequent astronomers were unable to find. Beta Hydri, the brightest star in Hydrus, is a yellow star of apparent magnitude 2.8, lying 24 light-years from Earth.
Generally, each step is accompanied by an incantation which > is pronounced by the adept standing in the star and which evokes the image > of the deity of the star in question. (Andersen 1898:38) The deity Taiyi 太一, translated as the Great One, Great Oneness, Great Monad, and Great Unity, has been viewed as the supreme god of heaven since the late Warring States period. According to Chinese mythology and astronomical tradition, Taiyi, the Emperor of Heaven, resides in the brightest star in the bowl of the "Little Dipper", the large, reddish Kochab or Beta Ursae Minoris (β UMi) near the northern Pole star (Andersen 1989:24). Traditional Chinese astronomy calls β UMi the beijier 北極二 "North Pole second [star]", and locates Ursa Minor within the Ziweiyuan 紫微垣 Purple Forbidden enclosure.
German astronomer Johann Elert Bode depicted it as the pendulum of the clock, while Lacaille made it one of the weights. It is an orange giant star of spectral type K2III that has swollen to around 11 times the diameter of the Sun, having spent much of its life as a white main-sequence star. At an estimated 1.55 times the mass of the Sun, it is radiating 38 times the Sun's luminosity from its photosphere at an effective (surface) temperature of 5,028K. At magnitude 4.93, Delta Horologii is the second-brightest star in the constellation, and forms a wide optical double with Alpha. Delta itself is a true binary system composed of a white main sequence star of spectral type A5V that is 1.41 times as massive as the Sun with a magnitude of 5.15 and its fainter companion of magnitude 7.29.
Caelum is a faint constellation: It has no star brighter than magnitude 4 and only two stars brighter than magnitude 5\. Lacaille gave six stars Bayer designations, labeling them Alpha (α ) to Zeta (ζ ) in 1756, but omitted Epsilon (ε ) and designated two adjacent stars as Gamma (γ ). Bode extended the designations to Rho (ρ ) for other stars, but most of these have fallen out of use. Caelum is too far south for any of its stars to bear Flamsteed designations. The constellation Caelum as it can be seen by the alt=Image of the constellation Caelum, showing the pattern of its stars as seen in the night sky The brightest star, (Alpha) α Caeli, is a double star, containing an F-type main-sequence star of magnitude 4.45 and a red dwarf of magnitude 12.5 , from Earth.
He verified its observations about certain peculiarities in Ptolemy's theory of the Moon's motion, by conducting on 9 March 1497 at Bologna a memorable observation of the occultation of Aldebaran, the brightest star in the Taurus constellation, by the moon. Copernicus the humanist sought confirmation for his growing doubts through close reading of Greek and Latin authors (Pythagoras, Aristarchos of Samos, Cleomedes, Cicero, Pliny the Elder, Plutarch, Philolaus, Heraclides, Ecphantos, Plato), gathering, especially while at Padua, fragmentary historic information about ancient astronomical, cosmological and calendar systems. Copernicus spent the jubilee year 1500 in Rome, where he arrived with his brother Andrew that spring, doubtless to perform an apprenticeship at the Papal Curia. Here, too, however, he continued his astronomical work begun at Bologna, observing, for example, a lunar eclipse on the night of 5–6 November 1500.
Zeta Doradus A is a bright, high proper motion star with a spectral type of F7V, meaning that it is a main sequence star that is hotter and brighter than the Sun. With an apparent magnitude of 4.82, it is approximately the eighth brightest star in the constellation of Dorado. Though it has been known that Zeta Doradus B is a nearby star since at least the Gliese Catalogue of Nearby Stars, the connection that it is a common proper motion companion to Zeta Doradus A was only made much more recently thanks to Hipparcos satellite data. The two stars form a wide binary, with a physical separation between the components of about 0.018 parsecs (0.06 light-years) which is approximately 3700 AU. This is comparable to the 15000 AU separation between Alpha Centauri AB and Proxima Centauri.
The constellation contains 85 stars of naked eye visibility.Elijah H. Burritt - The geography of the heavens and class book of astronomy: Accompanied by a celestial atlas Huntington, 1840 Retrieved 2012-06-25E ColbertAstronomy without a telescope: being a guide-book to the visible heavens, with all necessary maps and illustrations George & C.W. Sherwood, 1869 Retrieved 2012-06-27 The brightest star in Gemini is Pollux, and the second-brightest is Castor. Castor's Bayer designation as "Alpha" arose because Johann Bayer did not carefully distinguish which of the two was the brighter when he assigned his eponymous designations in 1603. α Gem (Castor) is a sextuple star system 52 light-years from Earth, which appears as a magnitude-1.6 blue-white star to the unaided eye. Two spectroscopic binaries are visible at magnitudes 1.9 and 3.0 with a period of 470 years.
VY Canis Majoris (brightest star in the image) and its surrounding molecular cloud complex (Rutherfurd Observatory/Columbia University) VY Canis Majoris has been known to be an extreme object since the middle of the 20th century, although its true nature was uncertain. In the late 20th century, it was accepted that it was a post-main sequence red supergiant. Its angular diameter had been measured and found to be significantly different depending on the observed wavelength. The first meaningful estimates of its properties showed a very large star, well in excess of . In contrast to prevailing opinion, a 2006 study, ignoring the effects of the circumstellar envelope in the observed flux of the star, derived a luminosity of , suggesting an initial mass of and radius of based on an assumed effective temperature of 3,650 K and distance of .
Appearing to have moved off the main sequence as their core hydrogen supply is being or has been exhausted, they are enlarging and cooling to eventually become red giant stars. Markab has an apparent magnitude of 2.48, while Algenib is a Beta Cephei variable that varies between magnitudes 2.82 and 2.86 every 3 hours 38 minutes, and also exhibits some slow pulsations every 1.47 days. Eta and Omicron Pegasi mark the left knee and Pi Pegasi the left hoof, while Iota and Kappa Pegasi mark the right knee and hoof. Also known as Matar, Eta Pegasi is the fifth-brightest star in the constellation. Shining with an apparent magnitude of 2.94, it is a multiple star system composed of a yellow giant of spectral type G2 and a yellow-white main sequence star of spectral type A5V that are 3.2 and 2.0 times as massive as our Sun.
For more than 20 years, the name Frank J. Miller was synonymous with entertainment in Augusta, GA. Through his company Augusta Amusements, he and his partners operated five downtown theaters and the brightest star in that constellation was the Miller. In 1938, Jacksonville-based architect Roy Benjamin was commissioned to design a theater large enough to accommodate the city's growing audiences. The result was a beautiful Art Moderne-style building that featured Italian marble terrazzo, black walnut millwork and a performance stage framed by fluted columns and hand-painted panels. Named after its founder, the Miller Theater seated over 1600 patrons and was the second- largest theater in Georgia, behind only Atlanta's Fox Theatre (Atlanta). The Miller opened in February 1940 with a sold-out performance of “A Night at the Moulin Rouge”, beginning what would be a 40-year run as one of Augusta's premier entertainment destinations.
The story of Saint Boniface cutting down Donar's Oak illustrates the pagan practices in 8th century among the Germans. A later folk version of the story adds the detail that an evergreen tree grew in place of the felled oak, telling them about how its triangular shape reminds humanity of the Trinity and how it points to heaven.The story, not recounted in the vitae written in his time, appears in a BBC Devon website, "Devon Myths and Legends", and in a number of educational storybooks, including St. Boniface and the Little Fir Tree: A Story to Color by Jenny Melmoth and Val Hayward (Warrington: Alfresco Books 1999 ), The Brightest Star of All: Christmas Stories for the Family by Carrie Papa (Abingdon Press 1999 ) and "How Saint Boniface Kept Christmas Eve" by Mary Louise Harvey in The American Normal Readers: Fifth Book, 207–22. Silver, Burdett and Co. 1912.
The pattern of the brightest stars resembles that of Ursa Minor, in that the stars form a pattern reminiscent of a bowl with a handle. Lying south-southeast of Acrux in neighbouring Crux is Alpha Muscae. It is the brightest star in the constellation with an apparent magnitude of 2.7. Lying around 310 light-years away, it is a blue-white star of spectral type B2IV-V that is around 4520 times as luminous and 8 times as massive as the Sun. The star is a Beta Cephei variable with about 4.7 times the Sun's diameter, and pulsates every 2.2 hours, varying by 1% in brightness. A nearby star of magnitude 13 may or may not be a companion star. Marking the fly's tail is Gamma Muscae, a blue-white star of spectral type B5V that varies between magnitudes 3.84 and 3.86 over a period of 2.7 days. It is a variable of a different type, classed as a slowly pulsating B star, a type of variable.
Size comparison of Vega (on the left), swollen at the equator due to its rapid rate of rotation, to the sun The planetary systems of stars other than the Sun and its solar system are a staple element in much science fiction. Vega (Alpha Lyrae) is a blue-white star in the constellation Lyra (the lyre, see High Sierra) that is frequently featured in works of science fiction. Like its bright cousins Sirius, Deneb, and Altair, it is classified as a star of spectral type A. Roughly two and a half times the size of the sun, it is 40 times as luminous and, together with Arcturus and Sirius, one of the most radiant stars in the galactic neighborhood. Its luminosity joins with its relative proximity to the Earth—it is only 25 light-years away—to make it the fifth-brightest star in the night sky (see French and English Tragedy by George Croly).
The third brightest star in Ara at magnitude 3.13 is Zeta Arae, an orange giant of spectral type K3III that is located 490 ± 10 light-years from Earth. Around 7–8 times as massive as the Sun, it has swollen to a diameter around 114 times that of the Sun and is 3800 times as luminous. Were it not dimmer by intervening interstellar dust, it would be significantly brighter at magnitude 2.11. Delta Arae is a blue-white main sequence star of spectral type B8Vn and magnitude 3.6, 198 ± 4 light-years from Earth. It is around 3.56 times as massive as the Sun. Epsilon1 Arae is an orange giant of apparent magnitude 4.1, 360 ± 10 light-years distant from Earth. It is around 74% more massive than the Sun. At an age of about 1.7 billion years, the outer envelope of the star has expanded to almost 34 times the Sun's radius.
Alpha Centauri (Latinized from α Centauri, abbreviated Alpha Cen or α Cen) is the closest star system and closest planetary system to Earth's Solar System at 4.37 light-years (1.34 parsecs) from the Sun. It is a triple star system, consisting of three stars: α Centauri A (officially Rigil Kentaurus), α Centauri B (officially Toliman), and α Centauri C (officially Proxima Centauri). Alpha Centauri A and B are Sun-like stars (Class G and K), and together they form the binary star Alpha Centauri AB. To the naked eye, the two main components appear to be a single star with an apparent magnitude of −0.27, the brightest star in the southern constellation of Centaurus and the third-brightest in the night sky, outshone only by Sirius and Canopus. Alpha Centauri A has 1.1 times the mass and 1.519 times the luminosity of the Sun, while Alpha Centauri B is smaller and cooler, at 0.907 times the Sun's mass and 0.445 times its luminosity.
The brightest star in the constellation, Gamma Velorum, is a complex multiple star system. The brighter component, known as Gamma2 Velorum, shines as a blue-white star of apparent magnitude 1.83. It is a spectroscopic binary made up of two very hot blue stars orbiting each other every 78.5 days and separated by somewhere between 0.8 and 1.6 Astronomical Units (AU). The brighter component is a hot blue main-sequence star of spectral type O7.5 and is around 280,000 times as luminous, is around 30 times as massive and is 17 times the diameter of our Sun with a surface temperature of 35,000 K. The second component is an extremely rare example of hot star known as a Wolf–Rayet star, and is the brightest example in the sky. It has a surface temperature of 57,000 and is around 170,000 times as luminous as our sun, though it radiates most of its energy in the ultraviolet spectrum.
On November 1, 2010, a super-Earth was announced orbiting the star along with Gliese 785 b as part of the NASA-UC Eta-Earth program. The planet orbits in just under 9.5 days and was originally thought to have a minimum mass of 8.2 ± 1.2 M⊕. Spurred by the possibility of transits, additional data was acquired for less than a year which found a lower mass for the star and hence reduced the minimum mass of the planet to 6.4 ± 0.7 M⊕, and improved certainty on the time of possible transit. Transits of the planet were apparently detected and announced on September 12, 2011; this would make HD 97658 the second-to- brightest star with a transiting planet after 55 Cancri and indicating a low- density planet like Gliese 1214 b. However, the occurrence of transits was quietly retracted on April 11, 2012, and three days later it was announced that observations by the MOST space telescope could not confirm transits.
In 2014, Crystal paid tribute to his close friend Robin Williams at the 66th Primetime Emmy Awards. In his tribute he talked about their friendship, saying, "As genius as he was on stage, he was the greatest friend you could ever imagine. Supportive. Protective. Loving. It’s very hard to talk about him in the past because he was so present in all of our lives. For almost 40 years, he was the brightest star in the comedy galaxy…[His] beautiful light will continue to shine on us forever. And the glow will be so bright, it’ll warm your heart. It’ll make your eyes glisten. And you’ll think to yourselves: Robin Williams. What a concept.” Crystal stated that paying tribute to Williams so publicly and so soon after Williams had died was one of "the hardest things I've had to do" and that "I was really worried that I wasn't going to get through it.
The system had an apparent visual magnitude around 11.7 and the primary is calculated to be slightly the brightest of the three known components. By November 1993, the spectral type was WN6 and the brightness had increased to around 10.9. The absorption lines in the spectrum were no longer detectable. The brightness increased for several weeks at the end of 1993, to above 10th magnitude, and the spectral type reached WN8, before the brightness dropped rapidly close to 11th magnitude. In June 1994, the star started to cool and become brighter again. It peaked at magnitude 8.6 in September and was comfortably the brightest star in the SMC, but there are no spectra at this exact time. Very shortly after the peak it was classified as WN11. In November the spectrum was considered to be B1.5Ia+, a blue hypergiant with strong hydrogen and ionised metal lines in emission or with P Cygni profiles.
An even more luminous yet closer star, WR 25, appears to be most likely to the title. Another nearer star, Eta Carinae, which was the second-brightest star in the sky for a few years in the 19th century, appears to be slightly more luminous than WR 102ka, but is known to be a binary star system. There is also the more recently discovered Pistol Star that, like the Peony star, derives its name from the shape of the nebula in which it is embedded, and which it has probably created through heavy mass loss via fierce stellar winds and perhaps also major "mini-supernova-like" eruptions as happened to Eta Carinae around the 1830s-1840s creating the lobes observed by the Hubble Space Telescope. The luminosities of the Pistol Star, Eta Carinae, and WR 102ka are all rendered somewhat uncertain due to heavy obscuration by galactic dust in the foreground, the effects of which must be corrected for before their apparent brightness can be reduced to estimate their total radiated power or bolometric luminosity.
Doublets In 1861, the brightest star in the night sky, Sirius, was found to have smaller stellar companion using the 18 and half-inch Dearborn refracting telescope. By the 18th century refractors began to have major competition from reflectors, which could be made quite large and did not normally suffer from the same inherent problem with chromatic aberration. Nevertheless, the astronomical community continued to use doublet refractors of modest aperture in comparison to modern instruments. Noted discoveries include the Moons of Mars and a fifth moon of Jupiter, Amalthea. Asaph Hall discovered Deimos on 12 August 1877 at about 07:48 UTC and Phobos on 18 August 1877, at the US Naval Observatory in Washington, D.C., at about 09:14 GMT (contemporary sources, using the pre-1925 astronomical convention that began the day at noon, give the time of discovery as 11 August 14:40 and 17 August 16:06 Washington mean time respectively).Morley, T. A.; A Catalogue of Ground-Based Astrometric Observations of the Martian Satellites, 1877-1982, Astronomy and Astrophysics Supplement Series, Vol.
Donizetti (remarking that she was "not the brightest star") told in a letter how in rehearsal she made an almighty row (which terrified Duprez) because, after Lucia's finale (the Mad Scene) there remained the finale of Edgardo ('Fra poco a me ricovero') before the curtain fell, displacing the final applause from herself to the tenor.Susan Rutherford, The Prima Donna and Opera, 1815-1930 (Cambridge University Press 2006), p. 171-72. She also sang Lucia in the first Paris performance, in December 1837, opposite Rubini (for whom Edgardo became one of his most celebrated roles), a performance received with acclaim bordering on hysteria.Ashbrook and Lo Presti 1986, 124. She was furthermore in the London premiere in April 1838. As Rosina in The Barber of Seville, 1840 She made her Paris début at the Théâtre-Italien in 1837 as Amina in La Sonnambula. She sang in the first Paris performance of L'elisir d'amore there in January 1839, with Nicolai Ivanoff, Tamburini and Lablache, for which (as was his custom) Donizetti added an aria for Tacchinardi-Persiani and a duet for her with Tamburini.Ashbrook and Lo Presti 1986, 128.
Clematis paniculata or known in Te Reo as Puawananga is very important to the Maori community as it has great cultural significance. It is so crucial for many different reasons one of the main reasons is because it is a part of one of their legends as many tribes believe that Puawananga along with the Whauwhapaku are the offspring of Puanga (Rigel) which is the brightest star of the Orion constellation and Ruhua (Antares) the most shining star of the Scorpion constellation the rising of these two stars in the morning signals the approach of summer and the time between the two events from June to November happens at the same time as when the Puawananga flowers bloom. They also use the flowering of the plant as an indicator as that the season of spring has started and that the eels have started to migrate up the rivers to spawn therefore it was time to harvest them as this is a spring event, so the two events of the flowering and eel migrating coincided. The woman would also use the Puawananga to make decorative pieces for wreaths and garlands they would make for their hair.
Fans of Williams created makeshift memorials at his star on the Hollywood Walk of Fame and at locations from his television and film career, such as the bench in Boston's Public Garden featured in Good Will Hunting; the Pacific Heights, San Francisco, home used in Mrs. Doubtfire; the sign for Parrish Shoes in Keene, New Hampshire, where parts of Jumanji were filmed; and the Boulder, Colorado, home used for Mork & Mindy. During the 66th Primetime Emmy Awards on August 25, 2014, close friend and fellow comedian Billy Crystal presented a tribute to Williams, referring to him as "the brightest star in our comedy galaxy". Afterwards, some of Williams' best comedy moments were shown, including his first ever The Tonight Show appearance, indicating his great life in making people laugh."Billy Crystal Emmys Tribute to Robin Williams Expected to Honor Humor", Guardianlv, August 22, 2014 Talk show hosts including David Letterman, Conan O'Brien, Seth Meyers, Jimmy Kimmel, and Jimmy Fallon paid tribute to Williams on their respective shows. On September 9, 2014, PBS aired a one-hour special devoted to his career,"Robin Williams Tribute Special to Air on PBS", Variety, September 2, 2014.
Puckett wrote the score for the film Before I Go (Starring Annabella Sciorra, 2021), AwesomenessTV series Guidance, Gravity (Starz) and for the films Caught (Lifetime Network, Dial a Prayer (Vertical Entertainment), Brightest Star and Boy Meets Girl Directed by Eric Schaeffer (GLAAD Outstanding Film Nominee, 2016). His songs, themes, and scores have been featured in Riverdale (2017 TV series), Lucifer (TV series), NY Med (ABC Series), After Fall, Winter (Showtime), She Wants Me, 2BR/2BA (Lionsgate), Best Friends Forever, Particles of Truth (75 Films), Hooking Up (ABC), Lisa Williams Show (Lifetime), and Crazy Sexy Cancer (TLC). Additional film and television credits include: Being Human (Syfy) which featured Puckett's cover version of The Psychedelic Furs "The Ghost In You", the score and end title song for Some Boys Don't Leave (Winner of Best Short at the 2010 Tribeca Film Festival) starring Jesse Eisenberg, score and songs for Particles Of Truth (75 Films, Sundance Channel), Colin Fitz (IFC / Official Selection Sundance), Never Again (Focus Features), Starved (FX) and Make It or Break It (Disney). His music was also featured in the ABC show Hopkins, in which he is credited for the theme song, "So Much To Say" and other music and songs for the series.
It omits the petitions, and consists of seventy-five praises joined to the usual invocation, "Sancta Maria". Here is a short specimen, showing the praises to be met with most frequently also in other litanies of that or of later times: "Holy Mary, Mother and Spouse of Christ, pray for me [other MSS. have "pray for us"-the "pray" is always repeated]; Holy Mary, Mother inviolate; Holy Mary, Temple of the Holy Ghost; Holy Mary, Queen of Heaven; Holy Mary, Mistress of the Angels; Holy Mary, Star of Heaven; Holy Mary, Gate of Paradise; Holy Mary, Mother of True Counsel; Holy Mary, Gate of Celestial Life; Holy Mary, Our Advocate; Holy Mary, brightest Star of Heaven; Holy Mary, Fountain of True Wisdom; Holy Mary, unfailing Rose; Holy Mary, Beauty of Angels; Holy Mary, Flower of Patriarchs; Holy Mary, Desire of Prophets; Holy Mary, Treasure of Apostles; Holy Mary, Praise of Martyrs; Holy Mary, Glorification of Priests; Holy Mary, Immaculate Virgin; Holy Mary, Splendour of Virgins", etc. The first Marian litanies must have been composed to foster private devotion, as it is not at all probable that they were written for use in public, by reason of their drawn-out and heavy style.

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