1916:. It became visible to the naked eye by December 10, 1891, as shown on photographic plates examined after the nova's discovery. It then brightened by a factor of 2.5 from December 11 to December 20, when it reached a maximum magnitude of 4.4. T Aurigae faded slowly in January and February 1892, then faded quickly during March and April, reaching a magnitude of 15 in late April. However, its brightness began to increase in August, reaching magnitude 9.5, where it stayed until 1895. Over the subsequent two years, its brightness decreased to 11.5, and by 1903, it was approximately 14th magnitude. By 1925, it had reached its current magnitude of 15.5. When the nova was discovered, its spectrum showed material moving at a high speed towards Earth. However, when the spectrum was examined again in August 1892, it appeared to be a planetary nebula. Observations at the Lick Observatory by Edward Emerson Barnard showed it to be disc-shaped, with clear nebulosity in a diameter of 3 arcseconds. The shell had a diameter of 12 arcseconds in 1943. T Aurigae is classified as a
564:
2524:—those that have a shallow angle of entry and seem to rise from the horizon—were observed in California. The meteors were tinted blue and green, moved slowly, and left trails at least 45° long. Because they had such a shallow angle of entry, some 1994 Aurigids lasted up to 2 seconds. Though there were only a few visual observers for part of the outburst, the 1994 Aurigids peak, which lasted less than two hours, was later confirmed by Finnish amateur radio astronomer Ilkka Yrjölä. The connection with Comet Kiess was finally confirmed in 1994. The 2007 outburst of the Aurigids was predicted by
729:
1828:, the reason it appears so bright at such a great distance. Epsilon Aurigae is the longest-period eclipsing binary currently known. The first observed eclipse of Epsilon Aurigae occurred in 1821, though its variable status was not confirmed until the eclipse of 1847–48. From that time forward, many theories were put forth as to the nature of the eclipsing component. Epsilon Aurigae has a noneclipsing component, which is visible as a 14th magnitude companion separated from the primary by 28.6 arcseconds. It was discovered by
2412:, partially because of its diameter of 40 arcminutes. It appears in an amateur telescope with brighter areas in the north and south; the brighter southern patch shows a pattern of darker and lighter spots in a large instrument. NGC 1893, of magnitude 7.5, is classified as a Trumpler Class II 3 r n or II 2 m n cluster, meaning that it is not very large and is somewhat bright. The cluster possesses approximately 30 stars of magnitude 9–12. In an amateur instrument, IC 410 is only visible with an Oxygen-III filter.
2485:
1799:
2083:), U Aurigae is of type M9, and X Aurigae is of type K2. R Aurigae, with a period of 457.5 days, ranges in magnitude from a minimum of 13.9 to a maximum of 6.7. UV Aurigae, with a period of 394.4 days, ranges in magnitude from a minimum of 10.6 to a maximum of 7.4. U Aurigae, with a period of 408.1 days, ranges in magnitude from a minimum of 13.5 to a maximum of 7.5. X Aurigae, with a particularly short period of 163.8 days, ranges in magnitude from a minimum of 13.6 to a maximum of 8.0.
2018:
1153:
2421:
8746:
7904:
2396:-shaped object in a telescope and contains approximately 100 stars; its overall magnitude is 6.4. M38, like M36, was discovered by Guillaume Le Gentil in 1749. It has an apparent diameter of approximately 20 arcseconds and a true diameter of about 25 light-years. Unlike M36 or M37, M38 has a varied stellar population. 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
2384:
9438:
2404:, a smaller and dimmer cluster that lies half a degree south-southwest of M38; it is at a distance of 4,200 light-years. The smaller cluster has an overall magnitude of 8.2 and a diameter of 6.0 arcminutes, making it about a third the size of M38. However, NGC 1907 is a rich cluster, classified as a Trumpler Class I 1 m n cluster. It has approximately 12 stars of magnitude 9–10, and at least 25 stars of magnitude 9–12.
52:
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9450:
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632:, who tricked his father into letting him drive his chariot for a day. Phaethon crashed and burned, scorching the earth. He was then placed in the night sky as the Auriga. Regardless of Auriga's specific representation, it is likely that the constellation was created by the ancient Greeks to commemorate the importance of the chariot in their society.
1492:. About 12 times the radius of the Sun, Delta weighs only two solar masses and rotates with a period of almost one year. Though it is often listed as a single star, it actually has three very widely spaced optical companions. One is a double star of magnitude 11, two arcminutes apart; the other is a star of magnitude 10, three arcminutes apart.
2512:. The Aurigid outburst on September 1, 1935, prompted the investigation of a connection with Comet Kiess, though the 24-year delay between the comet's return caused doubt in the scientific community. However, the outburst in 1986 erased much of this doubt. Istvan Teplickzky, a Hungarian amateur meteor observer, observed many bright meteors
1851:; its period is 972 days. The secondary is a B7V-type star, a B-type main-sequence star. Zeta Aurigae's maximum magnitude is 3.7 and its minimum magnitude is 4.0. The full eclipse of the small blue star by the orange giant lasts 38 days, with two partial phases of 32 days at the beginning and end. The primary has a diameter of 150
2032:(IC 405), which it illuminates. However, AE Aurigae likely entered the nebula only recently, as determined through the discrepancy between the radial velocities of the star and the nebula, 36 miles (58 km) per second and 13 miles (21 km) per second, respectively. It has been hypothesized that AE Aurigae is a "
1042:. She told her sons that the first to reach an eastern island would become the King of the Stars, and asked Dümur to let her come in his canoe. He refused, as did each of her sons in turn, except for Pleiades. Pleiades won the race with the help of Ligedaner, and became the King of the Stars. Elsewhere in the central
874:, although like all modern constellations, it is now defined as a specific region of the sky that includes both the ancient pattern and the surrounding stars. In 1922, the IAU designated its recommended three-letter abbreviation, "Aur". The official boundaries of Auriga were created in 1930 by Belgian astronomer
2324:
M36 (NGC 1960) is a young galactic open cluster with approximately 60 stars, most of which are relatively bright; however, only about 40 stars are visible in most amateur instruments. It is at a distance of 3,900 light-years and has an overall magnitude of 6.0; it is 14 light-years wide. Its apparent
1821:, and the secondary may be itself a binary star within a large dusty disk. Its maximum magnitude is 3.0, but it stays at a minimum magnitude of 3.8 for around a year; its most recent eclipse began in 2009. The primary has an absolute magnitude of −8.5 and an unusually high luminosity of 200,000
2443:
is a nebula in Auriga, slightly more than one degree to the west of M36. It is considered to be a difficult target for an amateur telescope. NGC 1931 has an approximate integrated magnitude of 10.1; it is 3 by 3 arcminutes. However, it appears to be elongated in an amateur telescope. Some observers
1551:
and an absolute magnitude of 0.2. Nu is a giant star with a radius of 20–21 solar radii and a mass of approximately 3 solar masses. It may technically be a binary star; its companion, sometimes listed as optical and separated by 56 arcseconds, is a dwarf star of spectral type K6 and magnitude 11.4.
4359:
Hill, Michelle L.; Mocnik, Teo; Kane, Stephen R.; Henry, Gregory W.; Pepper, Joshua; Hinkel, Natalie R.; Dalba, Paul A.; Fulton, Benjamin J.; Stassun, Keivan G.; Rosenthal, Lee J.; Howard, Andrew W.; Howell, Steve B.; Everett, Mark E.; Boyajian, Tabetha S.; Fischer, Debra A.; Rodriguez, Joseph E.;
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and was observed by astronomers worldwide. Despite some predictions that there would be no Alpha
Aurigid outburst, many bright meteors were observed throughout the shower, which peaked on September 1 as predicted. Much like in the 1994 outburst, the 2007 Aurigids were very bright and often colored
746:
under his left arm; he holds the reins to the chariot in his right hand. However, depictions of Auriga have been inconsistent over the years. The reins in his right hand have also been drawn as a whip, though
Capella is almost always over his left shoulder and the Kids under his left arm. The 1488
2178:
was discovered through radial velocity measurements in 2004. It has a mass of 1.79 Jupiter masses and orbits every 890.76 days at a distance of 1.92 AU. Its parent star is faint, at an apparent magnitude of 7.88, a G5IV type star 49 parsecs away. It has a mass of 1.02 solar masses and a radius of
2352:
M37 (NGC 2099) is an open cluster, larger than M36 and at a distance of 4,200 light-years. It has 150 stars, making it the richest cluster in Auriga; the most prominent member is an orange star that appears at the center. M37 is approximately 25 light-years in diameter. It is the brightest open
1960:
which ranges between magnitudes 5.0 and 5.8 over a period of 3.7 days. A yellow-white supergiant, it lies at a distance of 1,600 light-years. It was discovered to be variable by
English amateur T.H. Astbury in 1905. It has a spectral class of F81bv, meaning that it is an F-type supergiant star.
524:
astronomers created constellations that were groups of animals, where each star represented one animal. The stars of Auriga comprised a herd of goats, an association also present in Greek mythology. The association with goats carried into the Greek astronomical tradition, though it later became
4299:
da Silva, Ronaldo; Udry, Stéphane; Bouchy, François; Moutou, Claire; Mayor, Michel; Beuzit, Jean-Luc; Bonfils, Xavier; Delfosse, Xavier; Desort, Morgan; Forveille, Thierry; Galland, Franck; Hébrard, Guillaume; Lagrange, Anne-Marie; Loeillet, Benoit; Lovis, Christophe; Pepe, Francesco; Perrier,
2005:
in 1907, it is almost always at its minimum magnitude of 15, but brightens to a maximum up to 60 times brighter than the minimum an average of every 55 days, though the period can range from 50 days to more than 100 days. It takes about 24 hours for the star to go from its minimum to maximum
2416:
is a small open cluster at a distance of 1,500 light-years. It contains 30 stars in a crescent shape. 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
2187:. Discovered in 2007 from radial velocity measurements, it orbits at a distance of 0.24 AU with a period of 36.96 days. HD 43691 has a radius identical to the Sun's, though it is more dense—its mass is 1.38 solar masses. It is a G0IV type star of magnitude 8.03, 93.2 parsecs from Earth.
2193:
is a star in Auriga with one planet orbiting it. This G3V type star is faint, at magnitude 8.1, and fairly distant, at 40.7 parsecs from Earth. Like the other stars, it is similar in size to the Sun, with a mass of 1.07 solar masses and a radius of 0.94 solar radii. Its planet,
2225:, 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
2444:
may note a green hue in the nebula; a large telescope will easily show the nebula's "peanut" shape, as well as the quartet of stars that are engulfed by the nebula. The open cluster portion of NGC 1931 is classed as a I 3 p n cluster; the nebula portion is classed as both an
2379:
in the cluster as well. M37's
Trumpler class is given as both I 2 r and II 1 r. The stars visible in a telescope range in magnitude from 9.0 to 13.0; there are two 9th magnitude stars in the center of the cluster and an east to west chain of 10th and 11th magnitude stars.
1538:. Like Delta, it has several optical companions and is often categorized as a single star. The brightest companions are of magnitude 10, separated by 175 and 203 arcseconds. The dimmer companions are of magnitude 13 and 14, 87 and 310 arcseconds from Lambda, respectively.
1847:(Sadatoni), an eclipsing binary star at a distance of 776 light-years with a period of 2 years and 8 months. It has an absolute magnitude of −2.3. The primary is an orange-hued K5II-type star (K-type bright giant) and the secondary is a smaller blue star similar to
1180:
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
2564:. There is another faint stream of meteors called the "Aurigids", unrelated to the September shower. This shower lasts from January 31 to February 23, peaking from February 5 through February 10; its slow meteors peak at a rate of approximately 2 per hour. The
2516:
from Auriga in a fashion very similar to the confirmed 1935 outburst. Because the position of
Teplickzky's observed radiant and the 1935 radiant were close to the position of Comet Kiess, the comet was confirmed as the source of the Aurigid meteor stream.
6890:
560:. His chariot was created in the image of the Sun's chariot, the reason Zeus placed him in the heavens. The Athenian hero then dedicated himself to Athena and, soon after, Zeus raised him into the night sky in honor of his ingenuity and heroic deeds.
2391:
M38 is a diffuse open cluster at a distance of 3,900 light-years, the least concentrated of the three main open clusters in Auriga; it is classified as a
Trumpler Class II 2 r or III 2 r cluster because of this. It appears as a cross-shaped or
916:
was one of three constellations which represented poles for horses to be tethered. They were formed by the triplets of
Epsilon, Zeta, and Eta Aurigae; Nu, Tau, and Upsilon Aurigae; and Chi and 26 Aurigae, with one other undetermined star.
1467:. Though its proper motion is just 0.02 arcseconds per year, it has a radial velocity of 10.5 miles (16.9 km) per second in recession. The traditional name Kabdhilinan, sometimes shortened to "Alkab", comes from the Arabic phrase
1485:, the northernmost bright star in Auriga, is a K0III-type star (K-type giant), 126 light-years from Earth and approximately 1.3 billion years old. It has a magnitude of 3.72, an absolute magnitude of 0.2, and a luminosity of 60
413:, Auriga is only visible in its entirety as far south as -34°; 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,
1201:, more specifically, the primary is a G-type star and the secondary is between a G-type and F-type star in its evolution. The secondary is formally classified as a G0III class star (G-type giant). The primary has a radius of 11.87
761:
of 1535 as a charioteer with a two-wheeled cart, powered by two horses and two oxen. Arabic and
Turkish depictions of Auriga varied wildly from those of the European Renaissance; one Turkish atlas depicted the stars of Auriga as a
1436:) of magnitude 2.69; it is about 494 light-years away from Earth. It evolved from a B-type star to K-type over the estimated 30–45 million years since its birth. It has an absolute magnitude of −2.3 and a luminosity of 700
2006:
magnitude. SS Aurigae is a very close binary star with a period of 4 hours and 20 minutes. Both components are small subdwarf stars; there has been dispute in the scientific community about which star originates the outbursts.
2110:. It is the eastern vertex of the constellation's pentagon. Theta Aurigae is moving away from Earth at a rate of 17.5 miles (28.2 km) per second. Theta Aurigae additionally has a second optical companion, discovered by
2472:, a small cluster, is slightly brighter at magnitude 7.0. It has a diameter of 6 arcminutes and contains 40 stars, making it far more concentrated than the similar-sized NGC 1778. Far dimmer than the other open clusters is
597:. The association of Auriga and Myrtilus is supported by depictions of the constellation, which rarely show a chariot. Myrtilus's chariot was destroyed in a race intended for suitors to win the heart of Oenomaus's daughter
1125:(Beta Aquilae), would rise soon. Aagjuuk, which represented the dawn following the winter solstice, was an incredibly important constellation in the Inuit mythos. It was also used for navigation and time-keeping at night.
2463:
NGC 1664 is a fairly large open cluster, with a diameter of 18 arcminutes, and moderately bright, with a magnitude of 7.6, comparable to several other open clusters in Auriga. One open cluster with a similar magnitude is
1952:, which ranges between magnitudes 4.8 and 5.7, though not with a regular period. It has a spectral class of K5Iab, an average magnitude of 4.91, and an absolute magnitude of −5.7. Dolones is 3,976 light-years from Earth.
2551:
are a weak shower with a northern and southern branch lasting from December 11 to January 21. The shower peaks on January 1 and has very slow meteors, with a maximum rate of 1–5 meteors per hour. It was discovered by
1521:
at 83 km/second. Though older than the Sun, it is similar in many ways; its mass is 1.07 solar masses, a radius of 1.3 solar radii, and a rotational period of 26 days. However, it differs from the Sun in its
2407:
IC 410, a faint nebula, is accompanied by the bright open cluster NGC 1893. The cluster is thin, with a diameter of 12 arcminutes and a population of approximately 20 stars. Its accompanying nebula has very low
2325:
diameter is 12.0 arcminutes. Of the three open clusters in Auriga, M36 is both the smallest and the most concentrated, though its brightest stars are approximately 9th magnitude. It was discovered in 1749 by
1898:
located 243 light-years from Earth with a magnitude of 3.17. It is a B3V class star, meaning that it is a blue-white hued main-sequence star. Eta Aurigae has an absolute magnitude of −1.7 and a luminosity of
2496:, named for the entire constellation and formerly called the "Alpha Aurigids", are renowned for their intermittent outbursts, such as those in 1935, 1986, 1994, and 2007. They are associated with the comet
475:
In Chinese mythology, Auriga's stars were incorporated into several constellations, including the celestial emperors' chariots, made up of the modern constellation's brightest stars. Auriga is home to the
1332:, meaning "shoulder of the charioteer" and is a reference to Beta Aurigae's location in the constellation. Menkalinan is 81 light-years away and has a magnitude of 1.90. Like Epsilon Aurigae, it is an
1817:
with an unusually long period of 27 years; its last minima occurred in 1982–1984 and 2009–2011. The distance to the system is disputed, variously cited as 4600 and 2,170 light-years. The primary is a
647:, as they journeyed home, Medea killed her brother and dismembered him, flinging the parts of his body into the sea, represented by the Milky Way. Each individual star represents a different limb.
5154:
Binary Stars as Critical Tools and Tests in Contemporary Astrophysics: Proceedings of the 240th Symposium of the International Astronomical Union Held in Prague, Czech Republic, August 22–25, 2006
908:, the five chariots of the celestial emperors and the representation of the grain harvest, was a constellation formed by Alpha Aurigae, Beta Aurigae, Beta Tauri, Theta Aurigae, and Iota Aurigae.
1886:. The two stars orbit each other about 500,000,000 miles (800,000,000 km) apart. Zeta Aurigae is moving away from Earth at a rate of 8 miles (13 km) per second. The second of the two
5291:
Kashyap, V.; Rosner, R.; Harnden, F.R. Jr.; Maggio, A.; Micela, G.; Sciortino, S. (1994). "X-ray emission on hybrid α stars: ROSAT observations of alpha Trianguli Australis and IOTA Aurigae".
4218:
Table 2, combined solution, Determination of the Orbit of the Planetary Companion to the Metal-Rich Star HD 45350, Michael Endl, William D. Cochran, Robert A. Wittenmyer, and Artie P. Hatzes,
1936:, it is a very close binary with a very short period. T Aurigae's period of 4.905 hours is comparable to DQ Herculis's period of 4.65 hours, and it has a partial eclipse period of 40 minutes.
2162:
F8V star of magnitude 6.74 — just past the limit of visibility to the naked eye. It is of similar size to the Sun, at 1.1 solar masses and 1.21 solar radii. The planet, with a mass of 3.83
2102:. It has an absolute magnitude of 0.1 and is 165 light-years from Earth. The secondary is a yellow star of magnitude 7.1, which requires a telescope of 100 millimetres (3.9 in) in
605:, killed him, despite his complicity in helping Pelops win her hand. After his death, Myrtilus's father Hermes placed him in the sky. Yet another mythological association of Auriga is
4252:
Dynamical and Observational Constraints on Additional Planets in Highly Eccentric Planetary Systems, Robert A. Wittenmyer, Michael Endl, William D. Cochran, and Harold F. Levison,
1237:. The two components are separated by 110 million kilometers, almost 75% of the distance between the Earth and the Sun. The star's status as a binary was discovered in 1899 at the
2198:, is a smaller planet, at 0.115 Jupiter masses. It orbits very close to its star, at 0.058 AU, every 4.94 days. HD 49674 b was discovered by radial velocity observations in 2002.
2540:
is 2–5 meteors per hour, the Aurigids are fast, with an entry velocity of 67 kilometres (42 mi)/sec. The annual Aurigids have a radiant located about two degrees north of
2387:
A photograph of M38; its characteristic shape, clearly visible to an observer in a telescope, is obscured by the greater number of stars revealed by a long-exposure photograph.
512:
or crook. However, this may have represented just Capella (Alpha Aurigae) or the modern constellation as a whole; this figure was alternatively called Gamlum or MUL.GAM in the
2249:; it is the edge of the galactic plane roughly nearest to the solar system. Ignoring nearby bright stars in the foreground this is a smaller and less luminous part of the
516:. The crook of Auriga stood for a goat-herd or shepherd. It was formed from most of the stars of the modern constellation; all of the bright stars were included except for
9279:
2573:
1359:. The component of its motion in the direction of Earth is 18 kilometres (11 mi) per second. Beta Aurigae may be associated with a stream of about 70 stars including
9199:
8476:
6458:
6278:
9244:
9063:
6218:
2028:
is a blue-hued main-sequence variable star. It is normally of magnitude 6.0, but its magnitude varies irregularly. AE Aurigae is associated with the 9-light-year-wide
6718:
6418:
6338:
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6198:
6115:
2536:
The Aurigids are normally a placid Class II meteor shower that peaks in the early morning hours of September 1, beginning on August 28 every year. Though the maximum
2210:
in 2008. It has a mass of 0.67 Jupiter masses and orbits just 0.053 AU from its parent star, with a period of 3.92 days; its radius is 1.4 Jupiter radii, making it a
9239:
6518:
6478:
6178:
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in that the Delta Aurigids last longer and have a dearth of bright meteors. They too have a hypothesized connection to an unknown short period retrograde comet. The
1086:
was the name for Capella but may have been the name for the whole constellation; the name means "Star-wreath" and refers to one of the wives of the Pleiades, called
573:
6538:
6498:
6258:
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6658:
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6598:
6578:
6558:
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6398:
6298:
6238:
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both described its color as red, a phenomenon attributed not to a change in Capella's color but to the idiosyncrasies of their color sensitivities. Capella has an
6698:
6678:
6638:
6378:
6358:
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9189:
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and has a very low peak rate. The Delta Aurigids last from September 22 through October 23, peaking between October 6 and October 15. They may be related to the
2371:]...with sparkling gold-dust". The stars of M37 are older than those of M36; they are approximately 200 million years old. Most of the constituent stars are
9274:
6855:
2118:
of Theta Aurigae, 0.1 arcseconds per year. The separation of this magnitude 9.2 component was 2.2 arcminutes (130.7 arcseconds) in 2007 with an angle of 350°.
2544:, a third-magnitude star in the center of the constellation. The Aurigids end on September 4. Some years, the maximum rate has reached 9–30 meteors per hour.
1965:
is a Cepheid variable as well; it varies in magnitude from a minimum of 8.0 to a maximum of 7.3; its spectral class is G0Iabv. It has a period of 11.62 days.
2509:
2277:, all of which are visible in binoculars or a small telescope in suburban skies. A larger telescope resolves individual stars. Three other open clusters are
1375:, though the connection is only hypothesized. Besides its close eclipsing companion, Menkalinan has two other stars associated with it. One is an unrelated
2400:. 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
975:
is the head. This constellation arose because of the prominence of caymans in daily Amazonian life. There is evidence that Capella was significant to the
5670:
Torres, Guillermo; Claret, Antonio; Young, Patrick A. (August 2009). "Binary Orbit, Physical Properties, and Evolutionary State of Capella (α Aurigae)".
2497:
2214:. Its parent star, HAT-P-9, is an F-type star approximately 480 parsecs from Earth. It has a mass of 1.28 solar masses and a radius of 1.32 solar radii.
2130:
star. The primary is of magnitude 5.0 and is at a distance of 270 light-years; the secondary is of magnitude 7.9 and is at a distance of 82 light-years.
2056:. IC 410 obtained its name from its appearance in long exposure astrophotographs; it has extensive filaments that make AE Aurigae appear to be on fire.
2002:
4300:
Christian; Pont, Frédéric; Queloz, Didier; Santos, Nuno C.; Ségransan, Damien; Sivan, Jean-Pierre; Vidal-Madjar, Alfred; Zucker, Shay (October 2007).
8440:
3489:
1003:
also noticed the bright pattern of Auriga's stars. To them, the constellation's bright stars formed a curve that was represented in crescent-shaped
6925:
6123:
1011:
of North America recognized a constellation with the same major stars as modern Auriga: Alpha, Beta, Gamma (Beta Tauri), Theta, and Iota Aurigae.
8469:
7938:
2581:
2548:
1970:
493:
485:
742:
Traditionally, illustrations of Auriga represent it as a chariot and its driver. The charioteer holds a goat over his left shoulder and has two
9056:
5369:
Lucas, Gene A.; Hopkins, Jeffrey L.; Stencel, Robert E. (23 May 2006). "Long-Period Eclipsing Binary System Epsilon Aurigae Eclipse Campaign".
2329:, the first of Auriga's major open clusters to be discovered. M36 features a 10-arcminute-wide knot of bright stars in its center, anchored by
1336:
star that varies in magnitude by 0.1. The two components are blue-white stars that have a period of 3.96 days. Its double nature was revealed
753:
deviated from this typical depiction by showing a four-wheeled cart driven by Auriga, who holds the reins of two oxen, a horse, and a zebra.
8775:
2330:
2068:
1994:
1962:
1882:. Zeta Aurigae was spectroscopically determined to be a double star by Antonia Maury in 1897 and was confirmed as a binary star in 1908 by
4421:"Radial Velocities from the N2K Project: Six New Cold Gas Giant Planets Orbiting HD 55696, HD 98736, HD 148164, HD 203473, and HD 211810"
2585:
2076:
2072:
1917:
1098:
1039:
1035:
803:
research finds it likely the group was equally named Agitator in about the 15th century and provides a quotation as late as 1623, from a
4302:"ELODIE metallicity-biased search for transiting Hot Jupiters IV. Intermediate period planets orbiting the stars HD 43691 and HD 132406"
8462:
2473:
2469:
2465:
1019:
9492:
9049:
8749:
1110:
4681:
Beatty, Thomas G.; et al. (2012). "KELT-2Ab: A Hot Jupiter Transiting the Bright (V = 8.77) Primary Star of a Binary System".
2341:
is given as both I 3 r and II 3 m. Besides the central knot, most of the cluster's other stars appear in smaller knots and groups.
2142:
There are several stars with confirmed planetary systems in Auriga; there is also a white dwarf with a suspected planetary system.
8768:
440:, a nearby eclipsing binary with an unusually long period, has been studied intensively. Because of its position near the winter
2533:
was 100 meteors per hour, observed at 4:15 am, California time (12:15 UTC) by a team of astronomers flying on NASA planes.
2476:
at magnitude 10.2. Despite its dimness, NGC 2126 is as concentrated as NGC 1857, having 40 stars in a diameter of 6 arcminutes.
6030:
17:
2014:
star at a distance of 2,000 light-years. It has a period of approximately 234 days and ranges between magnitudes 5.0 and 7.0.
8433:
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5660:
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5481:
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5403:
5359:
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5281:
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1502:) of magnitude 4.71. It has an absolute magnitude of 4.4 and is 41 light-years from Earth. It has very weak emissions in the
5865:
6918:
2134:
is spectroscopic binary of magnitude 5.9, with a spectral type assessed as either A8m or F0m, and a period of seven days.
2122:
is a double star at a distance of 159 light-years. The primary is of magnitude 5.0 and the secondary is of magnitude 8.1.
1510:
observations of Epsilon, an unusual variable, Lambda is commonly used as a comparison star. It is reaching the end of its
1451:" (blocked) by intra-galactic dust clouds — astronomers estimate by these it appears 0.6 magnitudes fainter. It is also a
7931:
2353:
cluster in Auriga with a magnitude of 5.6; it has an apparent diameter of 23.0 arcminutes. M37 was discovered in 1764 by
685:. The myth of the nymph says that the goat's hideous appearance, resembling a Gorgon, was partially responsible for the
5224:
Hopkins, Jeffrey L.; Stencel, Robert E. (23 May 2006). "Single Channel UBV and JH Band Photometry of Epsilon Aurigae".
992:
929:, representing chairs for the emperor and other officials, was made up of nine stars in the east of the constellation.
2253:
than looking towards the rest of its arms or central bar and has dust bands of the outer spiral arms. Auriga has many
925:, a pond, bridge, or pier, were other constellations in Auriga, though the stars that composed them are undetermined.
9314:
721:, all of which relate to its status as the "goat star". Zeta Aurigae and Eta Aurigae were first called the "Kids" by
598:
2206:. Unlike the other exoplanets in Auriga, detected by radial velocity measurements, HAT-P-9 b was detected using the
1062:), meaning "north of Aldebaran". Different names were noted for Auriga and Capella in Eastern Pacific societies. On
9497:
8426:
6013:
5991:
5969:
5947:
5925:
5903:
5130:
871:
200:
194:
2547:
The other meteor showers radiating from Auriga are far less prominent and capricious than the Alpha Aurigids. The
7907:
6911:
5611:
2357:, the first of many astronomers to laud its beauty. It was described as "a virtual cloud of glittering stars" by
2183:
is a significantly larger planet, with a mass of 2.49 Jupiter masses; it is also far closer to its parent star,
1101:, meaning "collar-bones", was a constellation that included Capella (Alpha Aurigae), Menkalinan (Beta Aurigae),
7924:
5048:
Davis, George A. Jr. (1944). "The Pronunciations, Derivations, and Meanings of a Selected List of Star Names".
2021:
The Flaming Star Nebula (IC 405), and its neighbor IC 410, along with AE Aurigae, which illuminates the nebula.
1544:
is a G9.5III (G-type giant) star of magnitude 3.97, 230 light-years from Earth. It has a luminosity of 60
681:). Though most often associated with Amalthea, Capella has sometimes been associated with Amalthea's owner, a
7948:
5430:
Meng, H. (October 2002). "Activity of Iota-Aurigids in 2001 and the possible orbit of the meteoroid stream".
1403:
Besides particularly bright stars of Alpha and Beta Aurigae, Auriga has many dimmer naked-eye visible stars.
371:
2079:, all of which are type M stars. More specifically, R Aurigae is of type M7III, UV Aurigae is of type C6 (a
9319:
6808:
887:
563:
2588:, but this connection is highly disputed. The hypothesized Iota Aurigids may instead be a faint stream of
2233:
KELT-2. KELT-2B is an early K-dwarf about 295 AU away, and was discovered the same time as the exoplanet.
1418:). At about +1.65 it would rank a clear third in apparent magnitude if still co-placed in Auriga. It is a
9289:
9164:
8698:
8314:
6945:
4613:
Shporer, Avi; et al. (2009). "HAT-P-9b: A Low-Density Planet Transiting a Moderately Faint F Star".
4301:
2569:
2095:(Bogardus, Mahasim) is a blue-white A0p class binary star of magnitude 2.62 with a luminosity of 75
2229:, similar to HAT-P-9b. The star KELT-2A is a late F-dwarf and is one member of the common-proper-motion
9404:
9387:
8978:
8558:
8159:
8044:
4306:
2601:
2561:
2114:
in 1852. The separation was at 52 arcseconds in 1978 and has been increasing since then because of the
1250:
899:
6898:
4362:"Orbital Refinement and Stellar Properties for the HD 9446, HD 43691, and HD 179079 Planetary Systems"
3030:
8498:
7959:
7325:
2372:
2334:
1969:
is the prototype of its class of irregular variable stars. Its variability was discovered in 1906 by
800:
5126:
The Mythology of the Night Sky: An Amateur Astronomer's Guide to the Ancient Greek and Roman Legends
2468:, with a magnitude of 7.7. This small cluster has a diameter of 7 arcminutes and contains 25 stars.
9299:
9294:
9284:
9174:
9129:
9114:
9094:
9084:
9018:
8628:
8618:
8503:
8324:
8154:
8134:
7974:
5588:
Rogers, John H. (1998). "Origins of the Ancient Constellations: II. The Mediterranean Traditions".
1883:
1829:
1027:
870:
Since the time of Ptolemy, Auriga has remained a constellation and is officially recognized by the
6793:
5245:
Hopkins, Jeffrey L.; Stencel, Robert E. (May 2007). "Recent UBVJH Photometry of Epsilon Aurigae".
4579:
2320:
A photograph of M36, clearly showing its characteristic knot of bright stars and its concentration
2048:, other runaway stars from the Orion cluster. Its spectral class is O9.5Ve, meaning that it is an
9487:
8891:
8867:
8678:
8673:
8568:
8407:
8274:
8269:
8264:
8074:
8054:
6950:
5567:
Rogers, John H. (1998). "Origins of the Ancient Constellations: I. The Mesopotamian Traditions".
5028:
4266:
4232:
2513:
2429:
2245:, about 3.5° to the east of Beta Aurigae. This is the point on the celestial sphere opposite the
2111:
1395:. It has a separation of 12.6 arcseconds, and is around 350 astronomical units from the primary.
1372:
1147:
477:
318:
56:
31:
617:, who committed suicide as a result. He was killed when his chariot was wrecked, but revived by
9309:
9229:
9184:
9169:
9154:
9104:
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8934:
8790:
8713:
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8329:
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6934:
4574:
4554:
2753:
2722:
1507:
1448:
1419:
1392:
1345:
1344:, making it the second spectroscopic binary discovered, and its variable nature was discovered
1295:
1246:
964:
860:
838:
812:
610:
578:
533:
391:
375:
328:
323:
5609:
Russell, Henry Norris (October 1922). "The New International Symbols for the Constellations".
2737:
867:
combined Hell's constellations into Telescopium Herschelii in 1801, located mostly in Auriga.
9334:
9234:
9209:
9144:
9134:
9089:
9072:
8993:
8983:
8852:
8733:
8668:
8653:
8648:
8643:
8633:
8608:
8523:
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8254:
8239:
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8204:
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8164:
8124:
7989:
7706:
7458:
7145:
5882:
5149:
5120:
2669:
2667:
2665:
2452:. NGC 1931 is approximately 6,000 light-years from Earth and could easily be confused with a
1913:
1814:
1287:
972:
968:
856:
808:
414:
222:
4329:
937:
representing different types of crops, included the northern stars of Delta and Xi Aurigae.
9367:
9119:
9099:
9028:
8929:
8862:
8842:
8379:
8259:
8209:
8149:
6899:
Warburg Institute Iconographic Database (ca 160 medieval and early modern images of Auriga)
6833:
6771:
5689:
5620:
5597:
5576:
5439:
5418:
5378:
5300:
5260:
5233:
5107:
5098:
Dubietis, Audrius; Arlt, Rainer (October 2002). "The current Delta-Aurigid meteor shower".
5078:
5057:
4700:
4632:
4566:
4513:
4442:
4383:
4325:
4262:
4254:
4228:
4220:
4179:
3942:
3915:
3498:
2537:
2530:
2362:
2333:, a double star with components separated by 10.7 arcseconds. Most of the stars in M36 are
2262:
1833:
1388:
1242:
1194:
842:
728:
658:
654:
406:
333:
208:
3906:
Copeland, Ralph; Becker, L. (August 1892). "On the new star in the constellation Auriga".
2662:
1387:. The other is likely associated gravitationally with the primary, as determined by their
8:
9466:
9159:
8809:
8638:
8513:
8359:
8184:
7984:
5203:
Higgins, David (1992). "The Ghostly Glow of Gaseous Nebulae". In Eicher, David J. (ed.).
4168:"A Planetary Companion to HD 40979 and Additional Planets Orbiting HD 12661 and HD 38529"
2846:
2844:
2842:
2840:
2838:
2584:
are a hypothesized shower occurring in mid-November; its parent body may be the asteroid
2568:
are a faint shower radiating from Auriga. It was discovered by a group of researchers at
2501:
2433:
2358:
2326:
2242:
2029:
1906:. Eta Aurigae is moving away from Earth at a rate of 4.5 miles (7.2 km) per second.
794:
614:
465:
399:
349:
6837:
6775:
5745:
5693:
5624:
5601:
5580:
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5304:
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4446:
4387:
4183:
3946:
3919:
3502:
1552:
Its period is more than 120,000 years and it orbits at least 3,700 AU from the primary.
693:. The asterism containing the goat and kids had been a separate constellation; however,
9454:
9442:
9254:
7887:
5705:
5701:
5679:
5392:
5250:
5204:
5183:
5182:
Harrington, Phil (1992). "The Challenge of Winter Nebulae". In Eicher, David J. (ed.).
4724:
4690:
4648:
4644:
4622:
4592:
4503:
4460:
4432:
4401:
4373:
4341:
4315:
2409:
2230:
1978:
1974:
1499:
1254:
734:
4712:
2835:
980:
875:
613:. He was ejected from Athens after he refused the romantic advances of his stepmother
9329:
9304:
9204:
9149:
9071:
6969:
5845:
5722:
5656:
5637:
5553:
5534:
5515:
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5458:
5452:
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5355:
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5277:
5210:
5189:
5157:
5134:
5090:
5034:
5013:
5007:
4965:
4959:
4728:
4464:
4405:
2449:
2167:
1933:
1514:
1307:
1185:, meaning "the goat", and in Sumerian, it was called mul.ÁŠ.KAR, "the goat star". On
804:
686:
568:
218:
6034:
5783:
5709:
4596:
4345:
1475:, but because it is close to the mass limit for such stars, it may instead become a
963:; its southern stars represent the end of the animal's tail. The eastern portion of
9418:
9324:
9259:
8688:
8578:
8289:
8084:
7830:
7620:
6841:
6779:
5804:
5697:
5349:
5308:
5086:
4992:
4716:
4708:
4640:
4584:
4521:
4450:
4391:
4333:
4270:
4236:
4187:
3506:
2525:
2505:
2053:
1957:
1929:
1912:(Nova Aurigae 1891) was a nova discovered at magnitude 5.0 on January 23, 1892, by
1863:
1818:
1498:(Al Hurr) is a G1.5IV-V-type star (G-type star intermediate between a subgiant and
1380:
1333:
1262:
1238:
1043:
1015:
820:
774:. One unusual representation of Auriga, from 17th-century France, showed Auriga as
390:
for '(the) charioteer', associating it with various mythological beings, including
124:
90:
6880:
6087:
6067:
5942:
4997:
4980:
4652:
2683:
9482:
9269:
8583:
8089:
7075:
7050:
6997:
6051:
5825:
5124:
5069:
Drummond, Jack D. (September 1982). "A note on the Delta Aurigid meteor stream".
4337:
2577:
2553:
2521:
2445:
2354:
2348:
A photograph of M37, showing its obviously larger size and its notable brightness
2290:
2246:
2151:
1807:
1640:
1518:
1511:
1094:
1071:
988:
956:
941:
879:
816:
706:
702:
662:
529:
437:
168:
5920:
5371:
The Society for Astronomical Sciences 25th Annual Symposium on Telescope Science
5226:
The Society for Astronomical Sciences 25th Annual Symposium on Telescope Science
5172:
2484:
9224:
9139:
8914:
8886:
8818:
8079:
8019:
8009:
7916:
7879:
7615:
7027:
5986:
5964:
5898:
4455:
4420:
4396:
4361:
2565:
2338:
2207:
2159:
2127:
1852:
1495:
1460:
1376:
1364:
1165:
934:
754:
650:
601:. Myrtilus earned his position in the sky when Hippodamia's successful suitor,
489:
421:
403:
313:
295:
272:
264:
3933:
Huggins, William; Huggins, Margaret Lindsay (August 1892). "On Nova Aurigae".
2557:
2305:, the Flaming Star Nebula, found about midway between M38 and ι Aurigae.
1798:
984:
9476:
9264:
9219:
9194:
9179:
7135:
7065:
7022:
7012:
6992:
6784:
6759:
6008:
2541:
2115:
2092:
2060:
1982:
1735:
1716:
1583:
1482:
1368:
1349:
1341:
1299:
1106:
1102:
1008:
790:
460:, popular targets for amateur astronomers. In addition, it has one prominent
433:
379:
282:
72:
4526:
4491:
2040:, leaving the cluster approximately 2.7 million years ago. It is similar to
959:
incorporate the stars of Auriga into a massive constellation representing a
948:
and was important religiously. Ancient Peruvian peoples saw Capella, called
51:
9430:
9124:
8988:
8791:
The 41 additional constellations added in the 16th, 17th and 18th centuries
8224:
7695:
7448:
7443:
7438:
7433:
7423:
7130:
7125:
7120:
7115:
7110:
7105:
7100:
7095:
7090:
7017:
7002:
6982:
3511:
3484:
2397:
2310:
2282:
2257:
and other objects; rich star-forming arms of the Milky Way - including the
2254:
2163:
2052:
main-sequence star. The Flaming Star Nebula, is located near IC 410 in the
2037:
2033:
1945:
1844:
1464:
1444:
1433:
1425:
1360:
1337:
1317:
1291:
1198:
976:
904:
The stars of Auriga were incorporated into several Chinese constellations.
771:
666:
445:
429:
6903:
4534:
4471:
2417:
approximately 12 stars of magnitude 9–10 and 20 stars of magnitude 11–13.
2017:
1352:. Menkalinan has an absolute magnitude of 0.6 and a luminosity of 50
738:, a set of constellation cards illustrated by Sidney Hall, London c. 1825.
552:, the four-horse chariot, which he used in the battle against the usurper
9023:
8553:
8548:
8543:
8349:
8034:
8029:
8024:
7085:
7080:
7070:
7060:
7007:
5320:
Krupp, E.C. (May 2007). "Rambling through the stars: Designated driver".
4720:
4659:
4280:
4200:
3485:"Statistical analysis from recent abundance determinations in HgMn stars"
2606:
2393:
2258:
2226:
2211:
2202:
is the first transiting exoplanet confirmed in Auriga, orbiting the star
2080:
2049:
2045:
1925:
1921:
1895:
1891:
1811:
1659:
1621:
1523:
1476:
1452:
1429:
1411:
1321:
1202:
1186:
1169:
1152:
883:
864:
782:
722:
670:
635:
An incidental appearance of Auriga in Greek mythology is as the limbs of
505:
425:
410:
184:
8418:
2420:
743:
9249:
9109:
8832:
8728:
8723:
8718:
8518:
8374:
8369:
8354:
8064:
7861:
7765:
7760:
7755:
7671:
7666:
7661:
7656:
7595:
7418:
7413:
7408:
7398:
7393:
7388:
7383:
7378:
7373:
7368:
7363:
7358:
7353:
7348:
7343:
7308:
7303:
7298:
7293:
7288:
7283:
7278:
7273:
7268:
7263:
7258:
7253:
7248:
7243:
7238:
7233:
7228:
7223:
7218:
7213:
7208:
7203:
7198:
7193:
7188:
7183:
7178:
7173:
7055:
7045:
7040:
7035:
6987:
3415:
3413:
3411:
3409:
3407:
3405:
3403:
3401:
3399:
3397:
3395:
3393:
3391:
3389:
3387:
3385:
3383:
2306:
2274:
2270:
2266:
2195:
2180:
2175:
2147:
2123:
2041:
2025:
2007:
1966:
1953:
1949:
1859:
1754:
1697:
1602:
1541:
1415:
1407:
1311:
1258:
1213:
1177:
1173:
1004:
996:
807:
multi-topic work. Some of the stars of Auriga were incorporated into a
553:
541:
517:
469:
457:
453:
449:
345:
6885:
6085:
4122:
4120:
4118:
4116:
4114:
3553:
3381:
3379:
3377:
3375:
3373:
3371:
3369:
3367:
3365:
3363:
3036:
2488:
The 2007 Aurigid outburst observed from 47,000 feet by a NASA mission.
2313:, is a bright variable star currently within the Flaming Star Nebula.
2221:
is the brightest star in Auriga known to host a transiting exoplanet,
1156:
A size comparison of the four stars in the Capella system and the Sun.
701:. Before that, Capella was sometimes seen as its own constellation—by
9372:
9362:
8944:
8924:
8905:
8896:
8663:
8603:
8563:
8394:
8304:
8249:
8229:
8189:
8114:
8049:
7770:
7643:
7338:
7333:
7168:
7163:
7158:
7153:
6846:
6821:
6033:. Research Consortium on Nearby Stars. 1 January 2012. Archived from
5152:. In Hartkopf, William I.; Guinan, Edward F.; Harmanec, Petr (eds.).
4112:
4110:
4108:
4106:
4104:
4102:
4100:
4098:
4096:
4094:
2376:
2250:
2199:
2119:
2107:
2064:
2011:
2001:-type variable star, classified as an explosive dwarf. Discovered by
1909:
1773:
1678:
1472:
1384:
1303:
778:
kneeling on the Milky Way, with a goat wrapped around his shoulders.
644:
618:
441:
235:
8533:
8484:
7999:
4492:"Chemo-kinematics of the Milky Way from the SDSS-III MARVELS survey"
2383:
827:. Originally, it included two constellations, Tubus Hershelii Major
797:
pitied Bellerophon for his foolishness and placed him in the stars.
8968:
8703:
8613:
8319:
8129:
8069:
7804:
7799:
7739:
7734:
7729:
7724:
7719:
7714:
7681:
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7651:
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7554:
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7471:
7466:
7403:
7314:
5312:
4588:
4508:
4437:
4378:
4274:
4240:
4192:
4167:
3360:
2493:
2457:
2440:
2425:
2413:
2401:
2298:
2286:
2278:
2222:
2190:
2184:
2171:
2143:
2131:
2103:
1998:
1990:
1531:
1503:
1325:
1249:
telescope. It appears with a golden-yellow hue, though Ptolemy and
1063:
1031:
698:
625:
594:
586:
549:
537:
513:
509:
481:
395:
290:
5684:
5514:. Maps and charts by Wil Tirion (4th ed.). Houghton Mifflin.
5255:
4695:
4627:
4320:
4091:
2966:
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2956:
2954:
2952:
2950:
2948:
2946:
2798:
2796:
2794:
2792:
2091:
Auriga is home to several less prominent binary and double stars.
1944:
There are many other variable stars of different types in Auriga.
8939:
8919:
8708:
8693:
8486:
8339:
8334:
8309:
8179:
7825:
7625:
7610:
7600:
7531:
7511:
6977:
5030:
Sky vistas: astronomy for binoculars and richest-field telescopes
4781:
4779:
4777:
3743:
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3425:
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2780:
2778:
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2218:
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1986:
1848:
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content is 1.15 times that of the Sun and it has relatively less
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1118:
1023:
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694:
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383:
161:
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2759:
2728:
1302:. Capella has one more companion, Capella H, which is a pair of
548:. Erichthonius was generally credited to be the inventor of the
9377:
9008:
9003:
8998:
8973:
8958:
8953:
8877:
8872:
8847:
8837:
8389:
8364:
8294:
8279:
8244:
8169:
8139:
8119:
8004:
7964:
7856:
7848:
7820:
7784:
7605:
6107:
5566:
3815:
3813:
3800:
3798:
3698:
3696:
3654:
3593:
3591:
3258:
3256:
2743:
2504:. The association was discovered after the outburst in 1935 by
2302:
2294:
2155:
1535:
1114:
1109:(Alpha Geminorum). Its rising signalled that the constellation
1030:
represents Dümur, the oldest son of the stars' mother, and the
1000:
960:
945:
824:
629:
602:
590:
557:
545:
461:
4774:
4735:
3958:
3956:
3874:
3872:
3870:
3855:
3738:
3524:
3522:
3442:
3440:
3323:
3321:
3319:
3317:
3315:
3313:
3311:
3309:
3307:
3305:
3303:
3301:
3299:
3297:
3295:
3293:
3291:
2923:
2825:
2823:
2821:
2819:
2817:
2815:
2813:
2811:
2769:
1517:
at an age of 6.2 billion years. It also has an unusually high
952:, as a star intimately connected to the affairs of shepherds.
142:
9013:
8857:
8573:
8299:
8234:
8059:
7428:
5963:
5941:
5919:
5897:
4540:
4477:
4286:
4206:
3889:
3887:
3728:
3726:
3615:
3289:
3287:
3285:
3283:
3281:
3279:
3277:
3275:
3273:
3271:
2453:
1456:
690:
682:
640:
636:
387:
127:
93:
5985:
5765:
Jenniskens, Peter; Kemp, Christopher C. (11 December 2007).
5651:
Thompson, Robert Bruce; Thompson, Barbara Fritchman (2007).
4796:
4794:
4665:
4132:
4079:
3830:
3828:
3810:
3795:
3785:
3783:
3713:
3711:
3693:
3683:
3681:
3588:
3253:
3157:
3058:
2901:
2899:
2436:
of recently formed stars is surrounded by the nebula IC 410.
2316:
1137:
The constellation Auriga as it can be seen by the naked eye.
532:, Auriga is often identified as the mythological Greek hero
9382:
8827:
8804:
8658:
8214:
8104:
7969:
6960:
5766:
5744:
4833:
4821:
4811:
4809:
3953:
3867:
3845:
3843:
3770:
3768:
3519:
3437:
3348:
3135:
3133:
3018:
2808:
2673:
2520:
The Aurigids had a spectacular outburst in 1994, when many
1527:
1471:, meaning "shoulder of the rein holder". Iota may end as a
1133:
775:
763:
689:' defeat, because Zeus skinned the goat and wore it as his
678:
520:, traditionally assigned to both Taurus and Auriga. Later,
136:
108:
102:
9425:
6007:
5866:"Meteor Activity Outlook for August 27- September 2, 2011"
5415:
The Morning Star Rises: an account of Polynesian astronomy
5290:
4845:
3884:
3753:
3723:
3642:
3630:
3559:
3268:
3229:
3070:
2996:
2994:
781:
Occasionally, Auriga is seen not as the Charioteer but as
402:, as are five other constellations that have stars in the
139:
6881:
The Deep Photographic Guide to the Constellations: Auriga
4893:
4791:
4680:
4043:
4021:
4019:
4004:
3992:
3980:
3968:
3825:
3780:
3708:
3678:
3464:
2981:
2979:
2896:
2367:
1383:; it has a magnitude of 10.5 and has a separation of 184
849:
831:
398:. Auriga is most prominent during winter evenings in the
105:
6856:"Beta Tauri (Elnath, El Nath, or Alnath, النطح an-naţħ)"
6809:"Nova Auriga – Evidence of the Theory of Partile Impact"
4857:
4806:
4298:
4067:
4055:
4031:
3840:
3765:
3603:
3145:
3130:
3118:
3094:
2265:- run through it. The three brightest open clusters are
1038:, is represented by Capella; she lived on the island of
4752:
4750:
3241:
3217:
3205:
3193:
3181:
3169:
2991:
2652:
2650:
2648:
2646:
2644:
2642:
2640:
2638:
697:
merged the Charioteer and the Goats in the 2nd-century
6065:
5394:
The Arctic Sky: Inuit astronomy, star lore, and legend
4762:
4612:
4552:
4418:
4165:
4144:
4016:
2976:
2850:
2344:
525:
associated with a charioteer along with the shepherd.
9402:
5432:
WGN, Journal of the International Meteor Organization
5150:"Spectroscopic Binary Candidates for Interferometers"
5100:
WGN, Journal of the International Meteor Organization
4905:
4489:
2884:
2623:
2365:
commented that the star field was "strewed [
1391:. This 14th-magnitude star was discovered in 1901 by
1034:
represent her youngest son. The mother of the stars,
5247:
Proceedings of the Society for Astronomical Sciences
4881:
4869:
4747:
3578:
3576:
3574:
3572:
3570:
3568:
3543:
3541:
3539:
3537:
3452:
3338:
3336:
3106:
3046:
2911:
2635:
2556:
in 1886 and was discovered to be the source of rare
1802:
An artist's rendering of the Epsilon Aurigae system.
1022:, which tells the story of the creation of the sky.
133:
99:
6049:
5398:. Royal Ontario Museum/Nunavut Research Institute.
5368:
4483:
4358:
3660:
3082:
3006:
2872:
2710:
2698:
2689:
1197:with a period of 104 days; the components are both
356:Best visible at 21:00 (9 p.m.) during the month of
130:
96:
6819:
6457:
6277:
5391:
3861:
3747:
2154:measurements on the parent star. HD 40979 is 33.3
27:Constellation in the northern celestial hemisphere
6764:Monthly Notices of the Royal Astronomical Society
6217:
5669:
4917:
4496:Monthly Notices of the Royal Astronomical Society
3666:
3624:
3565:
3534:
3490:Monthly Notices of the Royal Astronomical Society
3431:
3333:
2860:
1836:, and is about 0.5 light-years from the primary.
732:Auriga carrying the goat and kids as depicted in
9474:
7946:
6717:
6417:
6337:
6317:
6197:
6114:
5719:The Stargazer's Guide: How to Read Our Night Sky
5650:
5636:. The McDonald and Woodward Publishing Company.
4555:"Seven New Keck Planets Orbiting G and K Dwarfs"
4126:
4085:
3819:
3804:
3702:
3597:
3482:
3262:
1839:Another eclipsing binary in Auriga, part of the
1459:producing giant star that emits x-rays from its
1422:, with some large signatures of heavy elements.
1406:Gamma Aurigae, now known under its once co-name
6745:. Centre de données astronomiques de Strasbourg
6725:. Centre de données astronomiques de Strasbourg
6705:. Centre de données astronomiques de Strasbourg
6685:. Centre de données astronomiques de Strasbourg
6665:. Centre de données astronomiques de Strasbourg
6645:. Centre de données astronomiques de Strasbourg
6625:. Centre de données astronomiques de Strasbourg
6605:. Centre de données astronomiques de Strasbourg
6585:. Centre de données astronomiques de Strasbourg
6565:. Centre de données astronomiques de Strasbourg
6545:. Centre de données astronomiques de Strasbourg
6525:. Centre de données astronomiques de Strasbourg
6517:
6505:. Centre de données astronomiques de Strasbourg
6485:. Centre de données astronomiques de Strasbourg
6477:
6465:. Centre de données astronomiques de Strasbourg
6445:. Centre de données astronomiques de Strasbourg
6425:. Centre de données astronomiques de Strasbourg
6405:. Centre de données astronomiques de Strasbourg
6385:. Centre de données astronomiques de Strasbourg
6365:. Centre de données astronomiques de Strasbourg
6345:. Centre de données astronomiques de Strasbourg
6325:. Centre de données astronomiques de Strasbourg
6305:. Centre de données astronomiques de Strasbourg
6285:. Centre de données astronomiques de Strasbourg
6265:. Centre de données astronomiques de Strasbourg
6245:. Centre de données astronomiques de Strasbourg
6225:. Centre de données astronomiques de Strasbourg
6205:. Centre de données astronomiques de Strasbourg
6185:. Centre de données astronomiques de Strasbourg
6177:
6145:. Centre de données astronomiques de Strasbourg
6137:
5590:Journal of the British Astronomical Association
5569:Journal of the British Astronomical Association
4608:
4606:
3962:
3878:
3528:
3446:
2137:
2106:to resolve; the two stars are separated by 3.6
556:, the event that made Erichthonius the king of
7878:
6815:. Professor A. W. Bickerton. 6 September 1893.
6537:
6497:
6257:
6165:. Centre de donnés astronomiques de Strasbourg
5863:
5764:
5331:David Levy's Guide to Observing Meteor Showers
5244:
5223:
5026:
4981:"Stars and Constellations of a Pawnee Sky Map"
4839:
4827:
4741:
4676:
4674:
4161:
4159:
3932:
3905:
3893:
3759:
3732:
3648:
3636:
1977:. RW Aurigae's spectrum indicates a turbulent
1806:The most prominent variable star in Auriga is
1168:(Capella), the brightest star in Auriga, is a
933:, a constellation mostly formed from stars in
657:, who breast-fed the infant Zeus. It forms an
508:as a constellation called GAM, representing a
9057:
8776:
8470:
8434:
7932:
6919:
6657:
6617:
6597:
6577:
6557:
6437:
6397:
6297:
6237:
6157:
6124:Centre de données astronomiques de Strasbourg
5880:
5547:
5528:
4851:
4049:
4010:
3998:
3986:
3974:
3834:
3789:
3717:
3687:
3470:
2970:
2829:
1428:, also called Hasseleh and Kabdhilinan, is a
653:is associated with the mythological she-goat
6794:"Nova Auriga – Evidence in Favour of Impact"
6697:
6677:
6637:
6377:
6357:
5552:(8th ed.). Cambridge University Press.
5533:(3rd ed.). Princeton University Press.
5457:(2nd ed.). Cambridge University Press.
5097:
4899:
4603:
4292:
4073:
4061:
4037:
3849:
3774:
1078:("Great Valley"). Capella itself was called
428:among the brightest stars in the night sky.
6933:
5769:. Ames Research Center & Seti Institute
5450:
5148:Fekel, Francis C.; Tomkin, Jocelyn (2007).
5147:
4671:
4546:
4360:Beatty, Thomas G.; James, David J. (2020).
4156:
4138:
2802:
1443:. It is classed as a particularly luminous
1371:of this group is comparable to that of the
1223:); the secondary has a radius of 8.75
893:
673:, the latter two of which are known as the
585:Auriga, however, is sometimes described as
9064:
9050:
8783:
8769:
8477:
8463:
8441:
8427:
7939:
7925:
6926:
6912:
6822:"Nova Aurigæ – The Genesis of Nova Aruigæ"
6737:
5716:
5271:
5181:
5170:
4800:
4785:
4490:Grieves, N.; et al. (December 2018).
4150:
4025:
3354:
3163:
3151:
2905:
2492:Auriga is home to two meteor showers. The
2086:
863:; both represented Herschel's telescopes.
504:The first record of Auriga's stars was in
50:
8448:
7642:
6845:
6813:The Philosophical Institute of Canterbury
6801:The Philosophical Institute of Canterbury
6783:
5683:
5653:Illustrated Guide to Astronomical Wonders
5509:
5389:
5254:
5174:Native Astronomy in the Central Carolines
4996:
4978:
4961:The Cambridge Guide to the Constellations
4694:
4626:
4578:
4525:
4507:
4454:
4436:
4412:
4395:
4377:
4319:
4191:
3510:
3247:
3235:
3223:
3124:
3100:
3064:
2656:
1793:
1328:). Its Arabic name comes from the phrase
1286:). It may be loosely associated with the
1066:, the figure of modern Auriga was called
5412:
5068:
5027:Crossen, Craig; Rhemann, Gerald (2004).
4911:
3211:
3199:
3187:
3175:
2483:
2419:
2382:
2343:
2315:
2166:, orbits with a semi-major axis of 0.83
2016:
1797:
1151:
1132:
845:, and Auriga, and Tubus Hershelii Minor
727:
562:
499:
7847:
6757:
5608:
5202:
5118:
5005:
4756:
4166:Fischer, Debra A.; et al. (2003).
3327:
3076:
2890:
2629:
1939:
1241:; its period was determined in 1919 by
1082:("Unique Sovereign") in the Societies.
815:. This constellation was introduced by
14:
9475:
5490:
5274:Meteor Showers and their Parent Comets
4957:
4261:, #3 (September 2007), pp. 1276–1284,
3052:
3000:
2716:
2704:
2576:, though they are more similar to the
9045:
8764:
8458:
8422:
7920:
6907:
5843:
5823:
5781:
5631:
5471:
5319:
5047:
4948:
4939:
4553:Butler, R. Paul; et al. (2003).
3672:
3609:
3582:
3547:
3458:
3419:
3342:
3139:
3112:
3088:
3012:
2985:
2917:
2878:
2866:
2301:), a cluster with nebulosity next to
1871:; the secondary has a diameter of 4 D
1398:
1320:(Menkalinan, Menkarlina) is a bright
882:is between 4 37.5 and 7 30.5 and its
382:listed by the 2nd-century astronomer
5881:Lunsford, Robert (16 January 2012).
5493:Star Lore: Myths, Legends, and Facts
5454:Cambridge Guide to Stars and Planets
5451:Moore, Patrick; Tirion, Wil (1997).
5429:
5347:
5328:
5012:(2nd ed.). Dover Publications.
4923:
4887:
4875:
4863:
4815:
4768:
3926:
3899:
3476:
2337:with rapid rates of rotation. M36's
2150:. It was discovered in 2002 through
1070:("The house of Tutakaiolo"); in the
468:, associated with the variable star
9255:Psalterium Georgianum/Harpa Georgii
6803:. A. W. Bickerton. 1 November 1893.
5864:Lunsford, Robert (25 August 2011).
5803:
5476:. Institute of Physics Publishing.
3024:
2236:
1506:spectrum, like Epsilon Aurigae. In
944:, Capella represented the heart of
24:
9150:Honores Friderici/Gloria Frederici
5752:. International Astronomical Union
5548:Ridpath, Ian; Tirion, Wil (2009).
5529:Ridpath, Ian; Tirion, Wil (2001).
4942:Star Names: Their Lore and Meaning
4419:Ment, Kristo; et al. (2018).
886:is between 27.9° and 56.2° in the
25:
9509:
6874:
6820:Richard A. Gregory (4 May 1893).
5737:
5413:Makemson, Maud Worcester (1941).
4683:The Astrophysical Journal Letters
4541:Exoplanet Encyclopedia HD 49674 b
4478:Exoplanet Encyclopedia HD 43691 b
4287:Exoplanet Encyclopedia HD 45350 b
4227:, #6 (June 2006), pp. 3131–3134,
4207:Exoplanet Encyclopedia HD 40979 b
3661:Lucas, Hopkins & Stencel 2006
3483:Ghazaryan, S; Alecian, G (2016).
2479:
921:, the pond where the sun set and
878:as a polygon of 20 segments. Its
624:Auriga is also said to represent
189:56.1648331°–27.8913116°
9493:Constellations listed by Ptolemy
9460:
9448:
9436:
9424:
9412:
9075:(including Ptolemy's Argo Navis)
8745:
8744:
7903:
7902:
6014:Extrasolar Planets Encyclopaedia
5992:Extrasolar Planets Encyclopaedia
5970:Extrasolar Planets Encyclopaedia
5948:Extrasolar Planets Encyclopaedia
5926:Extrasolar Planets Encyclopaedia
5904:Extrasolar Planets Encyclopaedia
4940:Allen, Richard Hinckley (1899).
4666:Exoplanet Encyclopedia HAT-P-9 b
3422:, pp. 338–340, Table 14.12.
2036:" from the young cluster in the
872:International Astronomical Union
581:and Auriga are often associated.
253:Stars within 10.00 pc (32.62 ly)
123:
89:
8801:Vespucci or Corsalius early 16c
6758:Roberts, Issac (January 1893).
5811:. Oxford University Press. 2012
5746:"Auriga constellation boundary"
5131:Springer Science+Business Media
4932:
4352:
4246:
4212:
3432:Torres, Claret & Young 2009
2375:, though there are at least 12
1160:
1121:(Gamma Aquilae), and sometimes
1093:The stars of Auriga feature in
1018:featured Auriga in the myth of
967:is the rest of the tail, while
793:. In this version of the tale,
725:, an ancient Greek astronomer.
6031:"The 100 Nearest Star Systems"
5844:Kaler, Jim (4 February 2011).
5824:Kaler, Jim (17 October 2009).
5782:Kaler, Jim (1 February 2008).
5495:. Courier Dover Publications.
5491:Olcott, William Tyler (2004).
5333:. Cambridge University Press.
5276:. Cambridge University Press.
5156:. Cambridge University Press.
4964:. Cambridge University Press.
1993:. Its spectral type is G5V:e.
1843:asterism with Eta Aurigae, is
544:who was raised by the goddess
344:Visible at latitudes between +
13:
1:
4998:10.1525/aa.1927.29.2.02a00110
2612:
1875:and a luminosity of 140
1279:and the secondary is 70
593:'s son and the charioteer of
372:northern celestial hemisphere
9349:obsolete constellation names
8485:48 constellations listed by
5702:10.1088/0004-637X/700/2/1349
5171:Goodenough, Ward H. (1953).
5091:10.1016/0019-1035(82)90153-1
5009:Burnham's Celestial Handbook
5006:Burnham, Robert Jr. (1978).
4979:Buckstaff, Ralph N. (1927).
4953:. University of Texas Press.
4645:10.1088/0004-637X/690/2/1393
4127:Thompson & Thompson 2007
2731:The 100 Nearest Star Systems
2617:
2529:blue and green. The maximum
2170:and a period of 263.1 days.
2138:Stars with planetary systems
1948:(Dolones) is an orange-hued
987:has a marker for the star's
888:equatorial coordinate system
358:late February to early March
7:
9290:Sceptrum et Manus Iustitiae
6946:Auriga in Chinese astronomy
5634:The New Patterns in the Sky
5632:Staal, Julius D.W. (1988).
5121:"The Winter Constellations"
4958:Bakich, Michael E. (1995).
4713:10.1088/2041-8205/756/2/L39
3935:Astronomy and Astro-Physics
3908:Astronomy and Astro-Physics
2595:
2570:New Mexico State University
1771:
1752:
1733:
1714:
1695:
1676:
1657:
1638:
1619:
1600:
1581:
1298:, because of their similar
1128:
639:'s brother. In the myth of
10:
9514:
6860:C.D.S. – SIMBAD4 rel 1.197
5717:Winterburn, Emily (2009).
5510:Pasachoff, Jay M. (2006).
5474:The Data Book of Astronomy
5272:Jenniskens, Peter (2006).
5119:Falkner, David E. (2011).
4949:Aveni, Anthony F. (1977).
4828:Jenniskens & Kemp 2007
4742:Crossen & Rhemann 2004
4338:10.1051/0004-6361:20077314
4307:Astronomy and Astrophysics
3649:Hopkins & Stencel 2006
3637:Hopkins & Stencel 2007
2602:Auriga (Chinese astronomy)
2574:September Epsilon Perseids
2562:Alexander Stewart Herschel
1447:but its light is in part "
1251:Giovanni Battista Riccioli
1145:
900:Auriga (Chinese astronomy)
897:
448:in its borders, including
409:. Because of its northern
370:is a constellation in the
29:
9358:
9343:
9080:
9041:
8796:
8760:
8742:
8494:
8454:
8403:
7955:
7900:
7874:
7843:
7813:
7792:
7783:
7748:
7705:
7694:
7638:
7588:
7545:
7457:
7324:
7144:
6968:
6959:
6941:
5885:. American Meteor Society
5883:"2012 Meteor Shower List"
5868:. American Meteor Society
5809:Oxford English Dictionary
5672:The Astrophysical Journal
5417:. Yale University Press.
5293:The Astrophysical Journal
4951:Native American Astronomy
4615:The Astrophysical Journal
4559:The Astrophysical Journal
4172:The Astrophysical Journal
2971:Ridpath & Tirion 2001
2830:Ridpath & Tirion 2009
809:now-defunct constellation
444:, Auriga has many bright
342:
304:
281:
271:
260:
252:
244:
233:
217:
207:
193:
183:
167:
156:
81:
71:
63:
49:
44:
9285:Sceptrum Brandenburgicum
7949:88 modern constellations
6088:"Telescopium Herschelii"
5390:MacDonald, John (1998).
4900:Dubietis & Arlt 2002
4456:10.3847/1538-3881/aae1f5
4425:The Astronomical Journal
4397:10.3847/1538-3881/ab7d33
4366:The Astronomical Journal
2762:Mediterranean Traditions
2500:, discovered in 1911 by
2174:has one planet as well.
1884:William Wallace Campbell
1830:Sherburne Wesley Burnham
1379:, discovered in 1783 by
1272:(the primary is 90
1230:and a mass of 2.44
1141:
894:In non-Western astronomy
376:88 modern constellations
245:Stars brighter than 3.00
9498:Northern constellations
9073:Obsolete constellations
8824:Keyser & de Houtman
8408:Lists of constellations
6951:List of stars in Auriga
6935:Constellation of Auriga
5531:Stars and Planets Guide
5472:Moore, Patrick (2000).
5348:Levy, David H. (2005).
5329:Levy, David H. (2008).
5209:. Kalmbach Publishing.
5188:. Kalmbach Publishing.
4985:American Anthropologist
4330:2007A&A...473..323D
4139:Fekel & Tomkin 2007
2803:Moore & Tirion 1997
2746:Mesopotamian Traditions
2430:Spitzer Space Telescope
2112:Otto Wilhelm von Struve
2087:Binary and double stars
1410:(El Nath, Alnath) is a
1373:Ursa Major Moving Group
1148:List of stars in Auriga
757:depicted Auriga in his
574:Finding of Erichthonius
492:, and the hypothesized
57:List of stars in Auriga
32:Auriga (disambiguation)
9310:Telescopium Herschelii
6785:10.1093/mnras/53.3.123
5850:STARS/Star of the Week
5830:STARS/Star of the Week
5788:STARS/Star of the Week
3862:SIMBAD Epsilon Aurigae
3748:SIMBAD Upsilon Aurigae
3041:Telescopium Herschelii
2489:
2437:
2388:
2349:
2321:
2022:
1803:
1794:Eclipsing binary stars
1420:mercury-manganese star
1393:Edward Emerson Barnard
1314:) from the main pair.
1247:Mt. Wilson Observatory
1157:
1138:
1105:(Beta Geminorum), and
813:Telescopium Herschelii
789:who dared to approach
785:, the mortal rider of
739:
582:
534:Erichthonius of Athens
436:in the constellation;
378:; it was among the 48
18:Auriga (constellation)
9235:Officina Typographica
8449:Constellation history
7575:45350 (Lucilinburhuc)
6086:Ridpath, Ian (1988).
6066:Ridpath, Ian (1988).
5550:The Monthly Sky Guide
4527:10.1093/mnras/sty2431
3625:SIMBAD Lambda Aurigae
2487:
2423:
2386:
2347:
2319:
2020:
1914:Thomas David Anderson
1815:eclipsing binary star
1810:(Al Maz, Almaaz), an
1801:
1306:stars located 11,000
1263:luminosity of the Sun
1212:) and a mass of 2.47
1189:, Capella was called
1155:
1146:Further information:
1136:
1046:, Capella was called
731:
566:
500:History and mythology
6886:The clickable Auriga
5721:. Harper Perennial.
5354:. Prometheus Books.
5177:. University Museum.
4255:Astronomical Journal
4221:Astronomical Journal
4086:SIMBAD Theta Aurigae
3820:SIMBAD Omega Aurigae
3805:SIMBAD Sigma Aurigae
3703:SIMBAD Kappa Aurigae
3598:SIMBAD Delta Aurigae
3512:10.1093/mnras/stw911
3263:SIMBAD Alpha Aurigae
2538:zenithal hourly rate
2531:zenithal hourly rate
2363:Charles Piazzi Smyth
2289:, which is close to
1981:, and has prominent
1940:Other variable stars
1924:. Like DQ Herculis,
1834:Dearborn Observatory
1389:common proper motion
1195:spectroscopic binary
1095:Inuit constellations
1068:Te Wale-o-Tutakaiolo
1050:(variations include
426:multiple star system
420:Its brightest star,
30:For other uses, see
9160:Globus Aerostaticus
8810:Triangulum Australe
8360:Triangulum Australe
6838:1893Natur..48....6G
6776:1893MNRAS..53..123R
5694:2009ApJ...700.1349T
5625:1922PA.....30..469R
5602:1998JBAA..108...79R
5581:1998JBAA..108....9R
5444:2002JIMO...30..175M
5423:1941msra.book.....M
5383:2006SASS...25...25L
5322:Sky & Telescope
5305:1994ApJ...431..402K
5265:2007arXiv0706.0891H
5238:2006SASS...25...13H
5112:2002JIMO...30..168D
5083:1982Icar...51..655D
5062:1944PA.....52....8D
4866:, pp. 103–104.
4818:, pp. 117–118.
4788:, pp. 175–178.
4705:2012ApJ...756L..39B
4637:2009ApJ...690.1393S
4571:2003ApJ...582..455B
4518:2018MNRAS.481.3244G
4447:2018AJ....156..213M
4388:2020AJ....159..197H
4267:2007AJ....134.1276W
4233:2006AJ....131.3131E
4184:2003ApJ...586.1394F
3963:SIMBAD Psi1 Aurigae
3947:1892AstAp..11..571H
3920:1892AstAp..11..593C
3879:SIMBAD Zeta Aurigae
3612:, pp. 338–340.
3560:Kashyap et al. 1994
3529:SIMBAD Iota Aurigae
3503:2016MNRAS.460.1912G
3447:SIMBAD Beta Aurigae
3330:, pp. 261–296.
3142:, pp. 221–222.
3079:, pp. 469–471.
3067:, pp. 128–129.
2510:Arthur Teichgraeber
2502:Carl Clarence Kiess
2359:Robert Burnham, Jr.
2327:Guillaume Le Gentil
2243:galactic anticenter
2219:KELT-2A (HD 42176A)
2030:Flaming Star Nebula
1330:mankib dhu al-'inan
466:Flaming Star Nebula
400:northern Hemisphere
374:. It is one of the
267:(α Aur) (0.08)
41:
5973:. 22 December 2010
5951:. 27 November 2007
5929:. 22 December 2010
5750:The Constellations
5655:. O'Reilly Media.
5206:Stars and Galaxies
5185:Stars and Galaxies
4840:Lunsford, Activity
4129:, pp. 94–101.
3894:SIMBAD Eta Aurigae
3760:SIMBAD Chi Aurigae
3733:SIMBAD Tau Aurigae
3166:, pp. 26, 43.
2805:, p. 130–131.
2676:The Constellations
2490:
2438:
2410:surface brightness
2398:G type giant stars
2389:
2350:
2322:
2231:binary star system
2179:1.27 solar radii.
2023:
1979:stellar atmosphere
1975:Moscow Observatory
1804:
1500:main-sequence star
1399:Other bright stars
1348:20 years later by
1308:astronomical units
1255:absolute magnitude
1158:
1139:
1014:The people of the
993:Indigenous peoples
740:
583:
432:is an interesting
39:
9400:
9399:
9396:
9395:
9330:Turdus Solitarius
9305:Taurus Poniatovii
9300:Tarandus/Rangifer
9205:Machina Electrica
9037:
9036:
8756:
8755:
8416:
8415:
7914:
7913:
7896:
7895:
7888:MACS J0717.5+3745
7870:
7869:
7839:
7838:
7779:
7778:
7690:
7689:
7634:
7633:
6459:"Epsilon Aurigae"
6279:"Upsilon Aurigae"
6017:. 25 January 2008
5728:978-0-06-178969-4
5662:978-0-596-52685-6
5643:978-0-939923-04-5
5612:Popular Astronomy
5559:978-0-521-13369-2
5540:978-0-691-08913-3
5521:978-0-395-93432-6
5512:Stars and Planets
5502:978-0-486-43581-7
5483:978-0-7503-0620-1
5464:978-0-521-58582-8
5405:978-0-88854-427-8
5361:978-1-59102-361-6
5340:978-0-521-69691-3
5283:978-0-521-85349-1
5216:978-0-913135-05-1
5195:978-0-913135-05-1
5163:978-0-521-86348-3
5140:978-1-4614-0137-7
5040:978-3-211-00851-5
5019:978-0-486-24063-3
4971:978-0-521-44921-2
4852:Lunsford, Showers
4771:, pp. 97–99.
4141:, pp. 59–60.
4050:SIMBAD UV Aurigae
4011:SIMBAD AE Aurigae
3999:SIMBAD RW Aurigae
3987:SIMBAD RX Aurigae
3975:SIMBAD RT Aurigae
3835:SIMBAD Xi Aurigae
3790:SIMBAD Mu Aurigae
3718:SIMBAD Pi Aurigae
3688:SIMBAD Nu Aurigae
3471:SIMBAD Beta Tauri
3357:, pp. 13–14.
3238:, pp. 44–51.
3003:, pp. 65–69.
2988:, pp. 83–91.
2973:, pp. 86–88.
2498:Kiess (C/1911 N1)
2450:reflection nebula
2281:, lying close to
2063:stars in Auriga:
1934:Nova Aquilae 1918
1791:
1790:
1469:al-kab dh'il inan
1377:optical companion
1338:spectroscopically
1261:of 160 times the
1117:(Alpha Aquilae),
1007:. The indigenous
805:Gerard de Malynes
768:Mulus clitellatus
628:, son of the sun
569:Peter Paul Rubens
365:
364:
16:(Redirected from
9505:
9465:
9464:
9463:
9453:
9452:
9451:
9441:
9440:
9439:
9429:
9428:
9417:
9416:
9415:
9408:
9325:Triangulum Minus
9260:Quadrans Muralis
9066:
9059:
9052:
9043:
9042:
8785:
8778:
8771:
8762:
8761:
8748:
8747:
8689:Piscis Austrinus
8579:Corona Australis
8479:
8472:
8465:
8456:
8455:
8443:
8436:
8429:
8420:
8419:
8290:Piscis Austrinus
8085:Corona Australis
7941:
7934:
7927:
7918:
7917:
7906:
7905:
7876:
7875:
7845:
7844:
7831:Westbrook Nebula
7790:
7789:
7703:
7702:
7640:
7639:
6966:
6965:
6928:
6921:
6914:
6905:
6904:
6869:
6867:
6866:
6851:
6849:
6847:10.1038/048006b0
6816:
6804:
6798:
6789:
6787:
6754:
6752:
6750:
6734:
6732:
6730:
6714:
6712:
6710:
6694:
6692:
6690:
6674:
6672:
6670:
6654:
6652:
6650:
6634:
6632:
6630:
6614:
6612:
6610:
6594:
6592:
6590:
6574:
6572:
6570:
6554:
6552:
6550:
6534:
6532:
6530:
6514:
6512:
6510:
6494:
6492:
6490:
6474:
6472:
6470:
6454:
6452:
6450:
6434:
6432:
6430:
6414:
6412:
6410:
6394:
6392:
6390:
6374:
6372:
6370:
6354:
6352:
6350:
6334:
6332:
6330:
6314:
6312:
6310:
6294:
6292:
6290:
6274:
6272:
6270:
6254:
6252:
6250:
6234:
6232:
6230:
6219:"Lambda Aurigae"
6214:
6212:
6210:
6194:
6192:
6190:
6174:
6172:
6170:
6154:
6152:
6150:
6134:
6132:
6130:
6102:
6100:
6098:
6082:
6080:
6078:
6062:
6060:
6058:
6052:"Constellations"
6046:
6044:
6042:
6026:
6024:
6022:
6004:
6002:
6000:
5982:
5980:
5978:
5960:
5958:
5956:
5938:
5936:
5934:
5916:
5914:
5912:
5907:. 10 August 2012
5894:
5892:
5890:
5877:
5875:
5873:
5860:
5858:
5856:
5846:"Lambda Aurigae"
5840:
5838:
5836:
5820:
5818:
5816:
5805:"Agitator, noun"
5798:
5796:
5794:
5778:
5776:
5774:
5761:
5759:
5757:
5732:
5713:
5687:
5678:(2): 1349–1381.
5666:
5647:
5628:
5605:
5584:
5563:
5544:
5525:
5506:
5487:
5468:
5447:
5426:
5409:
5397:
5386:
5365:
5351:Deep Sky Objects
5344:
5325:
5316:
5287:
5268:
5258:
5241:
5220:
5199:
5178:
5167:
5144:
5115:
5094:
5065:
5044:
5023:
5002:
5000:
4975:
4954:
4945:
4927:
4921:
4915:
4909:
4903:
4897:
4891:
4885:
4879:
4873:
4867:
4861:
4855:
4849:
4843:
4837:
4831:
4825:
4819:
4813:
4804:
4798:
4789:
4783:
4772:
4766:
4760:
4754:
4745:
4739:
4733:
4732:
4698:
4678:
4669:
4663:
4657:
4656:
4630:
4621:(2): 1393–1400.
4610:
4601:
4600:
4582:
4550:
4544:
4538:
4532:
4531:
4529:
4511:
4502:(3): 3244–3265.
4487:
4481:
4475:
4469:
4468:
4458:
4440:
4416:
4410:
4409:
4399:
4381:
4356:
4350:
4349:
4323:
4296:
4290:
4284:
4278:
4250:
4244:
4216:
4210:
4204:
4198:
4197:
4195:
4178:(2): 1394–1408.
4163:
4154:
4148:
4142:
4136:
4130:
4124:
4089:
4083:
4077:
4074:SIMBAD X Aurigae
4071:
4065:
4062:SIMBAD U Aurigae
4059:
4053:
4047:
4041:
4038:SIMBAD R Aurigae
4035:
4029:
4023:
4014:
4008:
4002:
3996:
3990:
3984:
3978:
3972:
3966:
3960:
3951:
3950:
3930:
3924:
3923:
3903:
3897:
3891:
3882:
3876:
3865:
3859:
3853:
3850:SIMBAD 9 Aurigae
3847:
3838:
3832:
3823:
3817:
3808:
3802:
3793:
3787:
3778:
3775:SIMBAD 2 Aurigae
3772:
3763:
3757:
3751:
3745:
3736:
3730:
3721:
3715:
3706:
3700:
3691:
3685:
3676:
3670:
3664:
3658:
3652:
3646:
3640:
3634:
3628:
3622:
3613:
3607:
3601:
3595:
3586:
3580:
3563:
3557:
3551:
3545:
3532:
3526:
3517:
3516:
3514:
3480:
3474:
3468:
3462:
3456:
3450:
3444:
3435:
3429:
3423:
3417:
3358:
3352:
3346:
3340:
3331:
3325:
3266:
3260:
3251:
3245:
3239:
3233:
3227:
3221:
3215:
3209:
3203:
3197:
3191:
3185:
3179:
3173:
3167:
3161:
3155:
3149:
3143:
3137:
3128:
3122:
3116:
3110:
3104:
3098:
3092:
3086:
3080:
3074:
3068:
3062:
3056:
3050:
3044:
3034:
3028:
3022:
3016:
3010:
3004:
2998:
2989:
2983:
2974:
2968:
2921:
2915:
2909:
2903:
2894:
2888:
2882:
2876:
2870:
2864:
2858:
2848:
2833:
2827:
2806:
2800:
2767:
2757:
2751:
2741:
2735:
2726:
2720:
2714:
2708:
2702:
2696:
2687:
2681:
2671:
2660:
2654:
2633:
2627:
2526:Peter Jenniskens
2506:Cuno Hoffmeister
2460:of a telescope.
2428:obtained by the
2263:Orion–Cygnus Arm
2237:Deep-sky objects
2146:has one planet,
2054:celestial sphere
2003:Emil Silbernagel
1958:Cepheid variable
1930:Nova Persei 1901
1819:white supergiant
1555:
1554:
1412:B7III class star
1381:William Herschel
1334:eclipsing binary
1245:at the 100-inch
1239:Lick Observatory
1170:G8III class star
1074:, it was called
1044:Caroline Islands
1016:Marshall Islands
971:is its body and
823:'s discovery of
821:William Herschel
424:, is an unusual
359:
179:
175:
149:
148:
145:
144:
141:
138:
135:
132:
129:
115:
114:
111:
110:
107:
104:
101:
98:
95:
54:
42:
38:
21:
9513:
9512:
9508:
9507:
9506:
9504:
9503:
9502:
9473:
9472:
9471:
9461:
9459:
9449:
9447:
9437:
9435:
9423:
9413:
9411:
9403:
9401:
9392:
9354:
9339:
9270:Robur Carolinum
9076:
9070:
9033:
8792:
8789:
8752:
8738:
8584:Corona Borealis
8490:
8483:
8450:
8447:
8417:
8412:
8399:
8090:Corona Borealis
7951:
7945:
7915:
7910:
7892:
7880:Galaxy clusters
7866:
7835:
7809:
7775:
7744:
7697:
7686:
7652:HAT-P-9b (Alef)
7630:
7621:UGPS J0521+3640
7601:HAT-P-9 (Tevel)
7584:
7541:
7453:
7320:
7140:
6955:
6937:
6932:
6877:
6872:
6864:
6862:
6854:
6807:
6796:
6792:
6748:
6746:
6728:
6726:
6719:"Theta Aurigae"
6708:
6706:
6688:
6686:
6668:
6666:
6648:
6646:
6628:
6626:
6608:
6606:
6588:
6586:
6568:
6566:
6548:
6546:
6528:
6526:
6508:
6506:
6488:
6486:
6468:
6466:
6448:
6446:
6428:
6426:
6419:"Sigma Aurigae"
6408:
6406:
6388:
6386:
6368:
6366:
6348:
6346:
6339:"Omega Aurigae"
6328:
6326:
6319:"Kappa Aurigae"
6308:
6306:
6288:
6286:
6268:
6266:
6248:
6246:
6228:
6226:
6208:
6206:
6199:"Delta Aurigae"
6188:
6186:
6168:
6166:
6148:
6146:
6128:
6126:
6116:"Alpha Aurigae"
6096:
6094:
6076:
6074:
6056:
6054:
6040:
6038:
6020:
6018:
5998:
5996:
5976:
5974:
5954:
5952:
5932:
5930:
5910:
5908:
5888:
5886:
5871:
5869:
5854:
5852:
5834:
5832:
5814:
5812:
5792:
5790:
5784:"Delta Aurigae"
5772:
5770:
5755:
5753:
5740:
5735:
5729:
5663:
5644:
5560:
5541:
5522:
5503:
5484:
5465:
5406:
5362:
5341:
5284:
5217:
5196:
5164:
5141:
5050:Popular Science
5041:
5020:
4972:
4935:
4930:
4922:
4918:
4910:
4906:
4898:
4894:
4886:
4882:
4874:
4870:
4862:
4858:
4850:
4846:
4838:
4834:
4826:
4822:
4814:
4807:
4801:Jenniskens 2006
4799:
4792:
4786:Jenniskens 2006
4784:
4775:
4767:
4763:
4755:
4748:
4740:
4736:
4679:
4672:
4664:
4660:
4611:
4604:
4551:
4547:
4539:
4535:
4488:
4484:
4476:
4472:
4417:
4413:
4357:
4353:
4297:
4293:
4285:
4281:
4251:
4247:
4217:
4213:
4205:
4201:
4164:
4157:
4149:
4145:
4137:
4133:
4125:
4092:
4084:
4080:
4072:
4068:
4060:
4056:
4048:
4044:
4036:
4032:
4026:Harrington 1992
4024:
4017:
4009:
4005:
3997:
3993:
3985:
3981:
3973:
3969:
3961:
3954:
3931:
3927:
3904:
3900:
3892:
3885:
3877:
3868:
3860:
3856:
3848:
3841:
3833:
3826:
3818:
3811:
3803:
3796:
3788:
3781:
3773:
3766:
3758:
3754:
3746:
3739:
3731:
3724:
3716:
3709:
3701:
3694:
3686:
3679:
3671:
3667:
3659:
3655:
3647:
3643:
3635:
3631:
3623:
3616:
3608:
3604:
3596:
3589:
3581:
3566:
3558:
3554:
3546:
3535:
3527:
3520:
3481:
3477:
3469:
3465:
3457:
3453:
3445:
3438:
3434:, p. 1365.
3430:
3426:
3418:
3361:
3355:Goodenough 1953
3353:
3349:
3341:
3334:
3326:
3269:
3261:
3254:
3246:
3242:
3234:
3230:
3222:
3218:
3210:
3206:
3198:
3194:
3186:
3182:
3174:
3170:
3164:Goodenough 1953
3162:
3158:
3152:Goodenough 1953
3150:
3146:
3138:
3131:
3123:
3119:
3111:
3107:
3099:
3095:
3087:
3083:
3075:
3071:
3063:
3059:
3051:
3047:
3035:
3031:
3027:, agitator, n..
3023:
3019:
3011:
3007:
2999:
2992:
2984:
2977:
2969:
2924:
2916:
2912:
2906:Winterburn 2009
2904:
2897:
2889:
2885:
2877:
2873:
2865:
2861:
2849:
2836:
2828:
2809:
2801:
2770:
2758:
2754:
2742:
2738:
2727:
2723:
2715:
2711:
2703:
2699:
2688:
2684:
2672:
2663:
2655:
2636:
2628:
2624:
2620:
2615:
2598:
2578:Coma Berenicids
2554:William Denning
2522:grazing meteors
2482:
2355:Charles Messier
2247:Galactic Center
2241:Auriga has the
2239:
2152:radial velocity
2140:
2101:
2098:
2089:
2059:There are four
1942:
1905:
1902:
1881:
1878:
1874:
1869:
1866:
1856:
1832:in 1891 at the
1827:
1824:
1808:Epsilon Aurigae
1796:
1641:Upsilon Aurigae
1577:
1572:
1567:
1562:
1550:
1547:
1519:radial velocity
1512:hydrogen-fusing
1491:
1488:
1463:and has a cool
1442:
1439:
1430:K3II class star
1401:
1358:
1355:
1346:photometrically
1322:A2IV class star
1285:
1282:
1278:
1275:
1271:
1268:
1236:
1233:
1229:
1226:
1222:
1219:
1211:
1208:
1193:. Capella is a
1163:
1150:
1144:
1131:
1072:Society Islands
989:heliacal rising
955:In Brazil, the
942:Hindu astronomy
902:
896:
880:right ascension
876:Eugène Delporte
817:Maximilian Hell
735:Urania's Mirror
703:Pliny the Elder
663:Epsilon Aurigae
661:with the stars
530:Greek mythology
502:
438:Epsilon Aurigae
357:
354:
338:
306:
300:
273:Messier objects
225:
177:
173:
169:Right ascension
152:
126:
122:
92:
88:
59:
35:
28:
23:
22:
15:
12:
11:
5:
9511:
9501:
9500:
9495:
9490:
9488:Constellations
9485:
9470:
9469:
9457:
9445:
9433:
9421:
9398:
9397:
9394:
9393:
9391:
9390:
9385:
9380:
9375:
9370:
9368:Phoenicopterus
9365:
9359:
9356:
9355:
9353:
9352:
9344:
9341:
9340:
9338:
9337:
9332:
9327:
9322:
9317:
9312:
9307:
9302:
9297:
9292:
9287:
9282:
9277:
9272:
9267:
9262:
9257:
9252:
9247:
9242:
9237:
9232:
9227:
9225:Musca Borealis
9222:
9217:
9212:
9207:
9202:
9197:
9192:
9187:
9182:
9177:
9172:
9167:
9162:
9157:
9152:
9147:
9142:
9140:Custos Messium
9137:
9132:
9127:
9122:
9117:
9112:
9107:
9102:
9097:
9092:
9087:
9081:
9078:
9077:
9069:
9068:
9061:
9054:
9046:
9039:
9038:
9035:
9034:
9032:
9031:
9026:
9021:
9016:
9011:
9006:
9001:
8996:
8991:
8986:
8981:
8976:
8971:
8966:
8961:
8956:
8947:
8942:
8937:
8932:
8927:
8922:
8917:
8915:Canes Venatici
8908:
8899:
8894:
8889:
8887:Camelopardalis
8880:
8875:
8870:
8865:
8860:
8855:
8850:
8845:
8840:
8835:
8830:
8821:
8819:Coma Berenices
8812:
8807:
8797:
8794:
8793:
8788:
8787:
8780:
8773:
8765:
8758:
8757:
8754:
8753:
8743:
8740:
8739:
8737:
8736:
8731:
8726:
8721:
8716:
8711:
8706:
8701:
8696:
8691:
8686:
8681:
8676:
8671:
8666:
8661:
8656:
8651:
8646:
8641:
8636:
8631:
8626:
8621:
8616:
8611:
8606:
8601:
8596:
8591:
8586:
8581:
8576:
8571:
8566:
8561:
8556:
8551:
8546:
8541:
8536:
8531:
8526:
8521:
8516:
8511:
8506:
8501:
8495:
8492:
8491:
8482:
8481:
8474:
8467:
8459:
8452:
8451:
8446:
8445:
8438:
8431:
8423:
8414:
8413:
8411:
8410:
8404:
8401:
8400:
8398:
8397:
8392:
8387:
8382:
8377:
8372:
8367:
8362:
8357:
8352:
8347:
8342:
8337:
8332:
8327:
8322:
8317:
8312:
8307:
8302:
8297:
8292:
8287:
8282:
8277:
8272:
8267:
8262:
8257:
8252:
8247:
8242:
8237:
8232:
8227:
8222:
8217:
8212:
8207:
8202:
8197:
8192:
8187:
8182:
8177:
8172:
8167:
8162:
8157:
8152:
8147:
8142:
8137:
8132:
8127:
8122:
8117:
8112:
8107:
8102:
8097:
8092:
8087:
8082:
8080:Coma Berenices
8077:
8072:
8067:
8062:
8057:
8052:
8047:
8042:
8037:
8032:
8027:
8022:
8020:Canes Venatici
8017:
8012:
8010:Camelopardalis
8007:
8002:
7997:
7992:
7987:
7982:
7977:
7972:
7967:
7962:
7956:
7953:
7952:
7944:
7943:
7936:
7929:
7921:
7912:
7911:
7901:
7898:
7897:
7894:
7893:
7891:
7890:
7884:
7882:
7872:
7871:
7868:
7867:
7865:
7864:
7859:
7853:
7851:
7841:
7840:
7837:
7836:
7834:
7833:
7828:
7823:
7817:
7815:
7811:
7810:
7808:
7807:
7802:
7796:
7794:
7787:
7781:
7780:
7777:
7776:
7774:
7773:
7768:
7763:
7758:
7752:
7750:
7746:
7745:
7743:
7742:
7737:
7732:
7727:
7722:
7717:
7711:
7709:
7700:
7692:
7691:
7688:
7687:
7685:
7684:
7679:
7674:
7669:
7664:
7659:
7654:
7648:
7646:
7636:
7635:
7632:
7631:
7629:
7628:
7623:
7618:
7613:
7608:
7603:
7598:
7592:
7590:
7586:
7585:
7583:
7582:
7580:49674 (Nervia)
7577:
7572:
7567:
7562:
7557:
7551:
7549:
7543:
7542:
7540:
7539:
7534:
7529:
7524:
7519:
7514:
7509:
7504:
7499:
7494:
7489:
7484:
7479:
7474:
7469:
7463:
7461:
7455:
7454:
7452:
7451:
7446:
7441:
7436:
7431:
7426:
7421:
7416:
7411:
7406:
7401:
7396:
7391:
7386:
7381:
7376:
7371:
7366:
7361:
7356:
7351:
7346:
7341:
7336:
7330:
7328:
7322:
7321:
7319:
7318:
7311:
7306:
7301:
7296:
7291:
7286:
7281:
7276:
7271:
7266:
7261:
7256:
7251:
7246:
7241:
7236:
7231:
7226:
7221:
7216:
7211:
7206:
7201:
7196:
7191:
7186:
7181:
7176:
7171:
7166:
7161:
7156:
7150:
7148:
7142:
7141:
7139:
7138:
7133:
7128:
7123:
7118:
7113:
7108:
7103:
7098:
7093:
7088:
7083:
7078:
7073:
7068:
7063:
7058:
7053:
7048:
7043:
7038:
7033:
7025:
7020:
7015:
7010:
7005:
7000:
6995:
6990:
6985:
6983:β (Menkalinan)
6980:
6974:
6972:
6963:
6957:
6956:
6954:
6953:
6948:
6942:
6939:
6938:
6931:
6930:
6923:
6916:
6908:
6902:
6901:
6896:
6888:
6883:
6876:
6875:External links
6873:
6871:
6870:
6852:
6817:
6805:
6790:
6770:(3): 123–124.
6755:
6735:
6715:
6695:
6675:
6655:
6635:
6615:
6595:
6575:
6555:
6535:
6519:"Psi1 Aurigae"
6515:
6495:
6479:"Zeta Aurigae"
6475:
6455:
6435:
6415:
6395:
6375:
6355:
6335:
6315:
6295:
6275:
6255:
6235:
6215:
6195:
6179:"Iota Aurigae"
6175:
6155:
6139:"Beta Aurigae"
6135:
6104:
6103:
6083:
6063:
6050:Ridpath, Ian.
6047:
6037:on 13 May 2012
6027:
6005:
5983:
5961:
5943:"HD 43691 A b"
5939:
5917:
5895:
5878:
5861:
5841:
5821:
5801:
5799:
5779:
5762:
5741:
5739:
5738:Online sources
5736:
5734:
5733:
5727:
5714:
5667:
5661:
5648:
5642:
5629:
5606:
5585:
5564:
5558:
5545:
5539:
5526:
5520:
5507:
5501:
5488:
5482:
5469:
5463:
5448:
5438:(5): 175–180.
5427:
5410:
5404:
5387:
5366:
5360:
5345:
5339:
5326:
5317:
5313:10.1086/174494
5299:(1): 402–415.
5288:
5282:
5269:
5242:
5221:
5215:
5200:
5194:
5179:
5168:
5162:
5145:
5139:
5133:. p. 41.
5116:
5106:(5): 168–174.
5095:
5077:(3): 655–659.
5066:
5045:
5039:
5024:
5018:
5003:
4991:(2): 279–285.
4976:
4970:
4955:
4946:
4936:
4934:
4931:
4929:
4928:
4916:
4904:
4892:
4890:, p. 119.
4880:
4878:, p. 106.
4868:
4856:
4844:
4832:
4820:
4805:
4790:
4773:
4761:
4746:
4744:, p. 177.
4734:
4670:
4658:
4602:
4589:10.1086/344570
4565:(1): 455–466.
4545:
4533:
4482:
4470:
4411:
4351:
4314:(1): 323–328.
4291:
4279:
4275:10.1086/520880
4245:
4241:10.1086/503746
4211:
4199:
4193:10.1086/367889
4155:
4151:SIMBAD HR 1528
4143:
4131:
4090:
4078:
4066:
4054:
4042:
4030:
4015:
4003:
3991:
3979:
3967:
3952:
3925:
3898:
3883:
3866:
3854:
3839:
3824:
3809:
3794:
3779:
3764:
3752:
3737:
3722:
3707:
3692:
3677:
3665:
3653:
3641:
3629:
3614:
3602:
3587:
3564:
3552:
3533:
3518:
3475:
3463:
3461:, p. 279.
3451:
3436:
3424:
3359:
3347:
3332:
3267:
3252:
3248:MacDonald 1998
3240:
3236:MacDonald 1998
3228:
3224:MacDonald 1998
3216:
3214:, p. 210.
3204:
3202:, p. 252.
3192:
3190:, p. 202.
3180:
3178:, p. 268.
3168:
3156:
3144:
3129:
3127:, p. 280.
3125:Buckstaff 1927
3117:
3115:, p. 193.
3105:
3103:, p. 225.
3101:MacDonald 1998
3093:
3081:
3069:
3065:Pasachoff 2006
3057:
3045:
3029:
3017:
3005:
2990:
2975:
2922:
2920:, p. 109.
2910:
2908:, p. 131.
2895:
2883:
2871:
2859:
2834:
2807:
2768:
2752:
2736:
2721:
2709:
2697:
2692:Constellations
2682:
2661:
2657:Pasachoff 2006
2634:
2632:, p. 469.
2621:
2619:
2616:
2614:
2611:
2610:
2609:
2604:
2597:
2594:
2566:Delta Aurigids
2481:
2480:Meteor showers
2478:
2339:Trumpler class
2238:
2235:
2208:transit method
2164:Jupiter masses
2160:spectral class
2158:from Earth, a
2139:
2136:
2128:optical binary
2099:
2096:
2088:
2085:
2010:is a variable
1983:emission lines
1941:
1938:
1903:
1900:
1879:
1876:
1872:
1867:
1864:
1854:
1825:
1822:
1795:
1792:
1789:
1788:
1785:
1782:
1779:
1776:
1770:
1769:
1766:
1763:
1760:
1757:
1751:
1750:
1747:
1744:
1741:
1738:
1732:
1731:
1728:
1725:
1722:
1719:
1713:
1712:
1709:
1706:
1703:
1700:
1694:
1693:
1690:
1687:
1684:
1681:
1675:
1674:
1671:
1668:
1665:
1662:
1656:
1655:
1652:
1649:
1646:
1643:
1637:
1636:
1633:
1630:
1627:
1624:
1618:
1617:
1614:
1611:
1608:
1605:
1599:
1598:
1595:
1592:
1589:
1586:
1580:
1579:
1578:(light-years)
1574:
1569:
1564:
1559:
1548:
1545:
1496:Lambda Aurigae
1489:
1486:
1440:
1437:
1400:
1397:
1365:Alpha Ophiuchi
1356:
1353:
1283:
1280:
1276:
1273:
1269:
1266:
1265:, or 160
1234:
1231:
1227:
1224:
1220:
1217:
1209:
1206:
1162:
1159:
1143:
1140:
1130:
1127:
935:Camelopardalis
895:
892:
755:Jacob Micyllus
567:A painting by
501:
498:
490:Delta Aurigids
404:Winter Hexagon
386:. Its name is
380:constellations
363:
362:
340:
339:
337:
336:
331:
326:
321:
316:
314:Camelopardalis
310:
308:
307:constellations
302:
301:
299:
298:
296:Delta Aurigids
293:
287:
285:
283:Meteor showers
279:
278:
275:
269:
268:
262:
261:Brightest star
258:
257:
254:
250:
249:
246:
242:
241:
238:
231:
230:
227:
215:
214:
211:
205:
204:
199:657 sq. deg. (
197:
191:
190:
187:
181:
180:
171:
165:
164:
158:
154:
153:
151:
150:
119:
85:
83:
79:
78:
75:
69:
68:
65:
61:
60:
55:
47:
46:
26:
9:
6:
4:
3:
2:
9510:
9499:
9496:
9494:
9491:
9489:
9486:
9484:
9481:
9480:
9478:
9468:
9458:
9456:
9446:
9444:
9434:
9432:
9427:
9422:
9420:
9410:
9409:
9406:
9389:
9388:Vultur volans
9386:
9384:
9383:Vultur cadens
9381:
9379:
9376:
9374:
9371:
9369:
9366:
9364:
9361:
9360:
9357:
9351:
9350:
9346:
9345:
9342:
9336:
9333:
9331:
9328:
9326:
9323:
9321:
9318:
9316:
9313:
9311:
9308:
9306:
9303:
9301:
9298:
9296:
9293:
9291:
9288:
9286:
9283:
9281:
9278:
9276:
9273:
9271:
9268:
9266:
9265:Ramus Pomifer
9263:
9261:
9258:
9256:
9253:
9251:
9248:
9246:
9243:
9241:
9238:
9236:
9233:
9231:
9228:
9226:
9223:
9221:
9220:Mons Maenalus
9218:
9216:
9213:
9211:
9208:
9206:
9203:
9201:
9198:
9196:
9195:Lochium Funis
9193:
9191:
9188:
9186:
9183:
9181:
9180:Leo Palatinus
9178:
9176:
9173:
9171:
9168:
9166:
9163:
9161:
9158:
9156:
9153:
9151:
9148:
9146:
9143:
9141:
9138:
9136:
9133:
9131:
9128:
9126:
9123:
9121:
9118:
9116:
9113:
9111:
9108:
9106:
9103:
9101:
9098:
9096:
9093:
9091:
9088:
9086:
9083:
9082:
9079:
9074:
9067:
9062:
9060:
9055:
9053:
9048:
9047:
9044:
9040:
9030:
9027:
9025:
9022:
9020:
9017:
9015:
9012:
9010:
9007:
9005:
9002:
9000:
8997:
8995:
8992:
8990:
8987:
8985:
8982:
8980:
8977:
8975:
8972:
8970:
8967:
8965:
8962:
8960:
8957:
8955:
8951:
8948:
8946:
8943:
8941:
8938:
8936:
8933:
8931:
8928:
8926:
8923:
8921:
8918:
8916:
8912:
8909:
8907:
8903:
8900:
8898:
8895:
8893:
8890:
8888:
8884:
8881:
8879:
8876:
8874:
8871:
8869:
8866:
8864:
8861:
8859:
8856:
8854:
8851:
8849:
8846:
8844:
8841:
8839:
8836:
8834:
8831:
8829:
8825:
8822:
8820:
8816:
8813:
8811:
8808:
8806:
8802:
8799:
8798:
8795:
8786:
8781:
8779:
8774:
8772:
8767:
8766:
8763:
8759:
8751:
8741:
8735:
8732:
8730:
8727:
8725:
8722:
8720:
8717:
8715:
8712:
8710:
8707:
8705:
8702:
8700:
8697:
8695:
8692:
8690:
8687:
8685:
8682:
8680:
8677:
8675:
8672:
8670:
8667:
8665:
8662:
8660:
8657:
8655:
8652:
8650:
8647:
8645:
8642:
8640:
8637:
8635:
8632:
8630:
8627:
8625:
8622:
8620:
8617:
8615:
8612:
8610:
8607:
8605:
8602:
8600:
8597:
8595:
8592:
8590:
8587:
8585:
8582:
8580:
8577:
8575:
8572:
8570:
8567:
8565:
8562:
8560:
8557:
8555:
8552:
8550:
8547:
8545:
8542:
8540:
8537:
8535:
8532:
8530:
8527:
8525:
8522:
8520:
8517:
8515:
8512:
8510:
8507:
8505:
8502:
8500:
8497:
8496:
8493:
8488:
8480:
8475:
8473:
8468:
8466:
8461:
8460:
8457:
8453:
8444:
8439:
8437:
8432:
8430:
8425:
8424:
8421:
8409:
8406:
8405:
8402:
8396:
8393:
8391:
8388:
8386:
8383:
8381:
8378:
8376:
8373:
8371:
8368:
8366:
8363:
8361:
8358:
8356:
8353:
8351:
8348:
8346:
8343:
8341:
8338:
8336:
8333:
8331:
8328:
8326:
8323:
8321:
8318:
8316:
8313:
8311:
8308:
8306:
8303:
8301:
8298:
8296:
8293:
8291:
8288:
8286:
8283:
8281:
8278:
8276:
8273:
8271:
8268:
8266:
8263:
8261:
8258:
8256:
8253:
8251:
8248:
8246:
8243:
8241:
8238:
8236:
8233:
8231:
8228:
8226:
8223:
8221:
8218:
8216:
8213:
8211:
8208:
8206:
8203:
8201:
8198:
8196:
8193:
8191:
8188:
8186:
8183:
8181:
8178:
8176:
8173:
8171:
8168:
8166:
8163:
8161:
8158:
8156:
8153:
8151:
8148:
8146:
8143:
8141:
8138:
8136:
8133:
8131:
8128:
8126:
8123:
8121:
8118:
8116:
8113:
8111:
8108:
8106:
8103:
8101:
8098:
8096:
8093:
8091:
8088:
8086:
8083:
8081:
8078:
8076:
8073:
8071:
8068:
8066:
8063:
8061:
8058:
8056:
8053:
8051:
8048:
8046:
8043:
8041:
8038:
8036:
8033:
8031:
8028:
8026:
8023:
8021:
8018:
8016:
8013:
8011:
8008:
8006:
8003:
8001:
7998:
7996:
7993:
7991:
7988:
7986:
7983:
7981:
7978:
7976:
7973:
7971:
7968:
7966:
7963:
7961:
7958:
7957:
7954:
7950:
7942:
7937:
7935:
7930:
7928:
7923:
7922:
7919:
7909:
7899:
7889:
7886:
7885:
7883:
7881:
7877:
7873:
7863:
7860:
7858:
7855:
7854:
7852:
7850:
7846:
7842:
7832:
7829:
7827:
7824:
7822:
7819:
7818:
7816:
7812:
7806:
7803:
7801:
7798:
7797:
7795:
7791:
7788:
7786:
7782:
7772:
7769:
7767:
7764:
7762:
7759:
7757:
7754:
7753:
7751:
7747:
7741:
7738:
7736:
7733:
7731:
7728:
7726:
7723:
7721:
7718:
7716:
7713:
7712:
7710:
7708:
7704:
7701:
7699:
7693:
7683:
7680:
7678:
7675:
7673:
7670:
7668:
7665:
7663:
7660:
7658:
7655:
7653:
7650:
7649:
7647:
7645:
7641:
7637:
7627:
7624:
7622:
7619:
7617:
7616:SGR 0501+4516
7614:
7612:
7609:
7607:
7604:
7602:
7599:
7597:
7594:
7593:
7591:
7587:
7581:
7578:
7576:
7573:
7571:
7568:
7566:
7563:
7561:
7558:
7556:
7553:
7552:
7550:
7548:
7544:
7538:
7535:
7533:
7530:
7528:
7525:
7523:
7520:
7518:
7515:
7513:
7510:
7508:
7505:
7503:
7500:
7498:
7495:
7493:
7490:
7488:
7485:
7483:
7480:
7478:
7475:
7473:
7470:
7468:
7465:
7464:
7462:
7460:
7456:
7450:
7447:
7445:
7442:
7440:
7437:
7435:
7432:
7430:
7427:
7425:
7422:
7420:
7417:
7415:
7412:
7410:
7407:
7405:
7402:
7400:
7397:
7395:
7392:
7390:
7387:
7385:
7382:
7380:
7377:
7375:
7372:
7370:
7367:
7365:
7362:
7360:
7357:
7355:
7352:
7350:
7347:
7345:
7342:
7340:
7337:
7335:
7332:
7331:
7329:
7327:
7323:
7317:
7316:
7312:
7310:
7307:
7305:
7302:
7300:
7297:
7295:
7292:
7290:
7287:
7285:
7282:
7280:
7277:
7275:
7272:
7270:
7267:
7265:
7262:
7260:
7257:
7255:
7252:
7250:
7247:
7245:
7242:
7240:
7237:
7235:
7232:
7230:
7227:
7225:
7222:
7220:
7217:
7215:
7212:
7210:
7207:
7205:
7202:
7200:
7197:
7195:
7192:
7190:
7187:
7185:
7182:
7180:
7177:
7175:
7172:
7170:
7167:
7165:
7162:
7160:
7157:
7155:
7152:
7151:
7149:
7147:
7143:
7137:
7134:
7132:
7129:
7127:
7124:
7122:
7119:
7117:
7114:
7112:
7109:
7107:
7104:
7102:
7099:
7097:
7094:
7092:
7089:
7087:
7084:
7082:
7079:
7077:
7074:
7072:
7069:
7067:
7064:
7062:
7059:
7057:
7054:
7052:
7049:
7047:
7044:
7042:
7039:
7037:
7034:
7032:
7031:
7026:
7024:
7021:
7019:
7016:
7014:
7011:
7009:
7006:
7004:
7003:ζ (Saclateni)
7001:
6999:
6996:
6994:
6991:
6989:
6986:
6984:
6981:
6979:
6976:
6975:
6973:
6971:
6967:
6964:
6962:
6958:
6952:
6949:
6947:
6944:
6943:
6940:
6936:
6929:
6924:
6922:
6917:
6915:
6910:
6909:
6906:
6900:
6897:
6895:
6893:
6889:
6887:
6884:
6882:
6879:
6878:
6861:
6857:
6853:
6848:
6843:
6839:
6835:
6832:(1227): 6–8.
6831:
6827:
6823:
6818:
6814:
6810:
6806:
6802:
6795:
6791:
6786:
6781:
6777:
6773:
6769:
6765:
6761:
6760:"Nova Aurigæ"
6756:
6744:
6740:
6736:
6724:
6720:
6716:
6704:
6700:
6696:
6684:
6680:
6676:
6664:
6660:
6656:
6644:
6640:
6636:
6624:
6620:
6616:
6604:
6600:
6596:
6584:
6580:
6576:
6564:
6560:
6556:
6544:
6540:
6539:"Chi Aurigae"
6536:
6524:
6520:
6516:
6504:
6500:
6499:"Eta Aurigae"
6496:
6484:
6480:
6476:
6464:
6460:
6456:
6444:
6440:
6436:
6424:
6420:
6416:
6404:
6400:
6396:
6384:
6380:
6376:
6364:
6360:
6356:
6344:
6340:
6336:
6324:
6320:
6316:
6304:
6300:
6296:
6284:
6280:
6276:
6264:
6260:
6259:"Tau Aurigae"
6256:
6244:
6240:
6236:
6224:
6220:
6216:
6204:
6200:
6196:
6184:
6180:
6176:
6164:
6160:
6156:
6144:
6140:
6136:
6125:
6121:
6117:
6113:
6112:
6111:
6110:
6109:
6093:
6089:
6084:
6073:
6069:
6064:
6053:
6048:
6036:
6032:
6028:
6016:
6015:
6010:
6006:
5995:. 20 May 2011
5994:
5993:
5988:
5984:
5972:
5971:
5966:
5962:
5950:
5949:
5944:
5940:
5928:
5927:
5922:
5918:
5906:
5905:
5900:
5896:
5884:
5879:
5867:
5862:
5851:
5847:
5842:
5831:
5827:
5822:
5810:
5806:
5802:
5800:
5789:
5785:
5780:
5768:
5763:
5751:
5747:
5743:
5742:
5730:
5724:
5720:
5715:
5711:
5707:
5703:
5699:
5695:
5691:
5686:
5681:
5677:
5673:
5668:
5664:
5658:
5654:
5649:
5645:
5639:
5635:
5630:
5626:
5622:
5618:
5614:
5613:
5607:
5603:
5599:
5595:
5591:
5586:
5582:
5578:
5574:
5570:
5565:
5561:
5555:
5551:
5546:
5542:
5536:
5532:
5527:
5523:
5517:
5513:
5508:
5504:
5498:
5494:
5489:
5485:
5479:
5475:
5470:
5466:
5460:
5456:
5455:
5449:
5445:
5441:
5437:
5433:
5428:
5424:
5420:
5416:
5411:
5407:
5401:
5396:
5395:
5388:
5384:
5380:
5376:
5372:
5367:
5363:
5357:
5353:
5352:
5346:
5342:
5336:
5332:
5327:
5323:
5318:
5314:
5310:
5306:
5302:
5298:
5294:
5289:
5285:
5279:
5275:
5270:
5266:
5262:
5257:
5252:
5248:
5243:
5239:
5235:
5231:
5227:
5222:
5218:
5212:
5208:
5207:
5201:
5197:
5191:
5187:
5186:
5180:
5176:
5175:
5169:
5165:
5159:
5155:
5151:
5146:
5142:
5136:
5132:
5128:
5127:
5122:
5117:
5113:
5109:
5105:
5101:
5096:
5092:
5088:
5084:
5080:
5076:
5072:
5067:
5063:
5059:
5055:
5051:
5046:
5042:
5036:
5032:
5031:
5025:
5021:
5015:
5011:
5010:
5004:
4999:
4994:
4990:
4986:
4982:
4977:
4973:
4967:
4963:
4962:
4956:
4952:
4947:
4943:
4938:
4937:
4925:
4920:
4913:
4912:Drummond 1982
4908:
4901:
4896:
4889:
4884:
4877:
4872:
4865:
4860:
4853:
4848:
4841:
4836:
4829:
4824:
4817:
4812:
4810:
4803:, p. 82.
4802:
4797:
4795:
4787:
4782:
4780:
4778:
4770:
4765:
4758:
4753:
4751:
4743:
4738:
4730:
4726:
4722:
4721:1969.1/178896
4718:
4714:
4710:
4706:
4702:
4697:
4692:
4688:
4684:
4677:
4675:
4667:
4662:
4654:
4650:
4646:
4642:
4638:
4634:
4629:
4624:
4620:
4616:
4609:
4607:
4598:
4594:
4590:
4586:
4581:
4580:10.1.1.7.6988
4576:
4572:
4568:
4564:
4560:
4556:
4549:
4542:
4537:
4528:
4523:
4519:
4515:
4510:
4505:
4501:
4497:
4493:
4486:
4479:
4474:
4466:
4462:
4457:
4452:
4448:
4444:
4439:
4434:
4430:
4426:
4422:
4415:
4407:
4403:
4398:
4393:
4389:
4385:
4380:
4375:
4371:
4367:
4363:
4355:
4347:
4343:
4339:
4335:
4331:
4327:
4322:
4317:
4313:
4309:
4308:
4303:
4295:
4288:
4283:
4276:
4272:
4268:
4264:
4260:
4257:
4256:
4249:
4242:
4238:
4234:
4230:
4226:
4223:
4222:
4215:
4208:
4203:
4194:
4189:
4185:
4181:
4177:
4173:
4169:
4162:
4160:
4152:
4147:
4140:
4135:
4128:
4123:
4121:
4119:
4117:
4115:
4113:
4111:
4109:
4107:
4105:
4103:
4101:
4099:
4097:
4095:
4087:
4082:
4075:
4070:
4063:
4058:
4051:
4046:
4039:
4034:
4027:
4022:
4020:
4012:
4007:
4000:
3995:
3988:
3983:
3976:
3971:
3964:
3959:
3957:
3948:
3944:
3940:
3936:
3929:
3921:
3917:
3913:
3909:
3902:
3895:
3890:
3888:
3880:
3875:
3873:
3871:
3863:
3858:
3851:
3846:
3844:
3836:
3831:
3829:
3821:
3816:
3814:
3806:
3801:
3799:
3791:
3786:
3784:
3776:
3771:
3769:
3761:
3756:
3749:
3744:
3742:
3734:
3729:
3727:
3719:
3714:
3712:
3704:
3699:
3697:
3689:
3684:
3682:
3674:
3669:
3662:
3657:
3650:
3645:
3638:
3633:
3626:
3621:
3619:
3611:
3606:
3599:
3594:
3592:
3584:
3579:
3577:
3575:
3573:
3571:
3569:
3561:
3556:
3549:
3544:
3542:
3540:
3538:
3530:
3525:
3523:
3513:
3508:
3504:
3500:
3496:
3492:
3491:
3486:
3479:
3472:
3467:
3460:
3455:
3448:
3443:
3441:
3433:
3428:
3421:
3416:
3414:
3412:
3410:
3408:
3406:
3404:
3402:
3400:
3398:
3396:
3394:
3392:
3390:
3388:
3386:
3384:
3382:
3380:
3378:
3376:
3374:
3372:
3370:
3368:
3366:
3364:
3356:
3351:
3344:
3339:
3337:
3329:
3324:
3322:
3320:
3318:
3316:
3314:
3312:
3310:
3308:
3306:
3304:
3302:
3300:
3298:
3296:
3294:
3292:
3290:
3288:
3286:
3284:
3282:
3280:
3278:
3276:
3274:
3272:
3264:
3259:
3257:
3250:, p. 66.
3249:
3244:
3237:
3232:
3226:, p. 65.
3225:
3220:
3213:
3212:Makemson 1941
3208:
3201:
3200:Makemson 1941
3196:
3189:
3188:Makemson 1941
3184:
3177:
3176:Makemson 1941
3172:
3165:
3160:
3154:, p. 43.
3153:
3148:
3141:
3136:
3134:
3126:
3121:
3114:
3109:
3102:
3097:
3091:, p. 70.
3090:
3085:
3078:
3073:
3066:
3061:
3055:, p. 11.
3054:
3049:
3042:
3040:
3033:
3026:
3021:
3015:, p. 29.
3014:
3009:
3002:
2997:
2995:
2987:
2982:
2980:
2972:
2967:
2965:
2963:
2961:
2959:
2957:
2955:
2953:
2951:
2949:
2947:
2945:
2943:
2941:
2939:
2937:
2935:
2933:
2931:
2929:
2927:
2919:
2914:
2907:
2902:
2900:
2893:, p. 41.
2892:
2887:
2881:, p. 79.
2880:
2875:
2868:
2863:
2856:
2854:
2847:
2845:
2843:
2841:
2839:
2832:, p. 67.
2831:
2826:
2824:
2822:
2820:
2818:
2816:
2814:
2812:
2804:
2799:
2797:
2795:
2793:
2791:
2789:
2787:
2785:
2783:
2781:
2779:
2777:
2775:
2773:
2765:
2763:
2756:
2749:
2747:
2740:
2733:
2732:
2725:
2719:, p. 26.
2718:
2713:
2707:, p. 54.
2706:
2701:
2694:
2693:
2686:
2679:
2677:
2670:
2668:
2666:
2658:
2653:
2651:
2649:
2647:
2645:
2643:
2641:
2639:
2631:
2626:
2622:
2608:
2605:
2603:
2600:
2599:
2593:
2591:
2587:
2583:
2582:Iota Aurigids
2579:
2575:
2571:
2567:
2563:
2559:
2555:
2550:
2549:Zeta Aurigids
2545:
2543:
2542:Theta Aurigae
2539:
2534:
2532:
2527:
2523:
2518:
2515:
2511:
2507:
2503:
2499:
2495:
2486:
2477:
2475:
2471:
2467:
2461:
2459:
2455:
2451:
2447:
2442:
2435:
2431:
2427:
2424:A picture of
2422:
2418:
2415:
2411:
2405:
2403:
2399:
2395:
2385:
2381:
2378:
2374:
2370:
2369:
2364:
2360:
2356:
2346:
2342:
2340:
2336:
2332:
2328:
2318:
2314:
2312:
2308:
2304:
2300:
2297:(surrounding
2296:
2292:
2288:
2284:
2280:
2276:
2272:
2268:
2264:
2260:
2256:
2255:open clusters
2252:
2248:
2244:
2234:
2232:
2228:
2224:
2220:
2215:
2213:
2209:
2205:
2201:
2197:
2192:
2188:
2186:
2182:
2177:
2173:
2169:
2165:
2161:
2157:
2153:
2149:
2145:
2135:
2133:
2129:
2125:
2121:
2117:
2116:proper motion
2113:
2109:
2105:
2094:
2093:Theta Aurigae
2084:
2082:
2078:
2074:
2070:
2066:
2062:
2061:Mira variable
2057:
2055:
2051:
2047:
2043:
2039:
2035:
2031:
2027:
2019:
2015:
2013:
2009:
2004:
2000:
1996:
1992:
1988:
1984:
1980:
1976:
1972:
1971:Lydia Ceraski
1968:
1964:
1959:
1955:
1951:
1947:
1937:
1935:
1931:
1927:
1923:
1920:, similar to
1919:
1915:
1911:
1907:
1897:
1896:B3 class star
1893:
1890:or "Kids" is
1889:
1885:
1870:
1861:
1857:
1850:
1846:
1842:
1837:
1835:
1831:
1820:
1816:
1813:
1809:
1800:
1786:
1783:
1780:
1777:
1775:
1772:
1767:
1764:
1761:
1758:
1756:
1753:
1748:
1745:
1742:
1739:
1737:
1736:Omega Aurigae
1734:
1729:
1726:
1723:
1720:
1718:
1717:Sigma Aurigae
1715:
1710:
1707:
1704:
1701:
1699:
1696:
1691:
1688:
1685:
1682:
1680:
1677:
1672:
1669:
1666:
1663:
1661:
1658:
1653:
1650:
1647:
1644:
1642:
1639:
1634:
1631:
1628:
1625:
1623:
1620:
1615:
1612:
1609:
1606:
1604:
1601:
1596:
1593:
1590:
1587:
1585:
1584:Kappa Aurigae
1582:
1575:
1570:
1565:
1560:
1557:
1556:
1553:
1543:
1539:
1537:
1533:
1529:
1525:
1520:
1516:
1513:
1509:
1505:
1501:
1497:
1493:
1484:
1483:Delta Aurigae
1480:
1478:
1474:
1470:
1466:
1462:
1458:
1454:
1450:
1446:
1435:
1431:
1427:
1423:
1421:
1417:
1413:
1409:
1404:
1396:
1394:
1390:
1386:
1382:
1378:
1374:
1370:
1369:proper motion
1366:
1362:
1351:
1350:Joel Stebbins
1347:
1343:
1342:Antonia Maury
1339:
1335:
1331:
1327:
1323:
1319:
1315:
1313:
1309:
1305:
1301:
1300:proper motion
1297:
1293:
1289:
1264:
1260:
1257:of 0.3 and a
1256:
1252:
1248:
1244:
1243:J.A. Anderson
1240:
1215:
1204:
1200:
1199:yellow giants
1196:
1192:
1188:
1184:
1179:
1175:
1171:
1167:
1166:Alpha Aurigae
1154:
1149:
1135:
1126:
1124:
1120:
1116:
1113:, made up of
1112:
1108:
1104:
1100:
1096:
1091:
1089:
1085:
1081:
1077:
1073:
1069:
1065:
1061:
1057:
1053:
1049:
1045:
1041:
1037:
1033:
1029:
1025:
1021:
1017:
1012:
1010:
1006:
1002:
998:
994:
990:
986:
982:
978:
974:
970:
966:
962:
958:
957:Bororo people
953:
951:
947:
943:
938:
936:
932:
928:
924:
920:
915:
911:
907:
901:
891:
889:
885:
881:
877:
873:
868:
866:
862:
858:
854:
851:
848:
844:
840:
836:
833:
830:
826:
822:
818:
814:
810:
806:
802:
798:
796:
792:
791:Mount Olympus
788:
784:
779:
777:
773:
769:
765:
760:
756:
752:
751:
745:
737:
736:
730:
726:
724:
720:
716:
712:
708:
704:
700:
696:
692:
688:
684:
680:
676:
672:
668:
664:
660:
656:
652:
648:
646:
642:
638:
633:
631:
627:
622:
620:
616:
612:
608:
604:
600:
596:
592:
588:
580:
576:
575:
570:
565:
561:
559:
555:
551:
547:
543:
539:
535:
531:
526:
523:
519:
515:
511:
507:
497:
495:
494:Iota Aurigids
491:
487:
486:Zeta Aurigids
483:
479:
473:
471:
467:
463:
459:
455:
451:
447:
446:open clusters
443:
439:
435:
434:variable star
431:
427:
423:
418:
416:
412:
408:
405:
401:
397:
393:
389:
385:
381:
377:
373:
369:
361:
353:
351:
347:
341:
335:
332:
330:
327:
325:
322:
320:
317:
315:
312:
311:
309:
303:
297:
294:
292:
289:
288:
286:
284:
280:
276:
274:
270:
266:
263:
259:
255:
251:
247:
243:
239:
237:
232:
228:
224:
220:
216:
212:
210:
206:
202:
198:
196:
192:
188:
186:
182:
178:07 30 56.1899
174:04 37 54.4293
172:
170:
166:
163:
159:
155:
147:
120:
118:
113:
87:
86:
84:
82:Pronunciation
80:
76:
74:
70:
66:
62:
58:
53:
48:
45:Constellation
43:
37:
33:
19:
9467:Solar System
9373:Serpentarius
9348:
9347:
9125:Cancer Minor
8989:Microscopium
8949:
8910:
8901:
8882:
8823:
8814:
8800:
8528:
8489:after 150 AD
8225:Microscopium
7994:
7313:
7029:
7018:ι (Hassaleh)
6891:
6863:. Retrieved
6859:
6829:
6825:
6812:
6800:
6767:
6763:
6747:. Retrieved
6742:
6727:. Retrieved
6722:
6707:. Retrieved
6702:
6687:. Retrieved
6682:
6667:. Retrieved
6662:
6659:"UV Aurigae"
6647:. Retrieved
6642:
6627:. Retrieved
6622:
6619:"AE Aurigae"
6607:. Retrieved
6602:
6599:"RW Aurigae"
6587:. Retrieved
6582:
6579:"RX Aurigae"
6567:. Retrieved
6562:
6559:"RT Aurigae"
6547:. Retrieved
6542:
6527:. Retrieved
6522:
6507:. Retrieved
6502:
6487:. Retrieved
6482:
6467:. Retrieved
6462:
6447:. Retrieved
6442:
6439:"Xi Aurigae"
6427:. Retrieved
6422:
6407:. Retrieved
6402:
6399:"Mu Aurigae"
6387:. Retrieved
6382:
6367:. Retrieved
6362:
6347:. Retrieved
6342:
6327:. Retrieved
6322:
6307:. Retrieved
6302:
6299:"Pi Aurigae"
6287:. Retrieved
6282:
6267:. Retrieved
6262:
6247:. Retrieved
6242:
6239:"Nu Aurigae"
6227:. Retrieved
6222:
6207:. Retrieved
6202:
6187:. Retrieved
6182:
6167:. Retrieved
6162:
6159:"Beta Tauri"
6147:. Retrieved
6142:
6127:. Retrieved
6119:
6106:
6105:
6095:. Retrieved
6091:
6075:. Retrieved
6071:
6055:. Retrieved
6039:. Retrieved
6035:the original
6019:. Retrieved
6012:
5997:. Retrieved
5990:
5975:. Retrieved
5968:
5965:"HD 49674 b"
5953:. Retrieved
5946:
5931:. Retrieved
5924:
5921:"HD 45350 b"
5909:. Retrieved
5902:
5899:"HD 40979 b"
5887:. Retrieved
5870:. Retrieved
5853:. Retrieved
5849:
5833:. Retrieved
5829:
5813:. Retrieved
5808:
5791:. Retrieved
5787:
5771:. Retrieved
5754:. Retrieved
5749:
5718:
5675:
5671:
5652:
5633:
5616:
5610:
5596:(2): 79–89.
5593:
5589:
5572:
5568:
5549:
5530:
5511:
5492:
5473:
5453:
5435:
5431:
5414:
5393:
5374:
5370:
5350:
5330:
5321:
5296:
5292:
5273:
5246:
5229:
5225:
5205:
5184:
5173:
5153:
5125:
5103:
5099:
5074:
5070:
5053:
5049:
5033:. Springer.
5029:
5008:
4988:
4984:
4960:
4950:
4941:
4919:
4907:
4895:
4883:
4871:
4859:
4847:
4835:
4823:
4764:
4757:Higgins 1992
4737:
4686:
4682:
4661:
4618:
4614:
4562:
4558:
4548:
4536:
4499:
4495:
4485:
4473:
4428:
4424:
4414:
4369:
4365:
4354:
4311:
4305:
4294:
4282:
4258:
4253:
4248:
4224:
4219:
4214:
4202:
4175:
4171:
4146:
4134:
4081:
4069:
4057:
4045:
4033:
4006:
3994:
3982:
3970:
3938:
3934:
3928:
3911:
3907:
3901:
3857:
3755:
3668:
3656:
3644:
3632:
3605:
3555:
3494:
3488:
3478:
3466:
3454:
3427:
3350:
3328:Burnham 1978
3243:
3231:
3219:
3207:
3195:
3183:
3171:
3159:
3147:
3120:
3108:
3096:
3084:
3077:Russell 1922
3072:
3060:
3048:
3038:
3032:
3020:
3008:
2913:
2891:Falkner 2011
2886:
2874:
2862:
2852:
2761:
2755:
2745:
2739:
2730:
2724:
2712:
2700:
2691:
2685:
2675:
2630:Russell 1922
2625:
2546:
2535:
2519:
2491:
2462:
2439:
2406:
2390:
2373:A type stars
2366:
2351:
2335:B type stars
2323:
2311:runaway star
2240:
2216:
2189:
2141:
2090:
2058:
2038:Orion Nebula
2034:runaway star
2024:
1943:
1908:
1887:
1862:of 700
1845:Zeta Aurigae
1840:
1838:
1805:
1540:
1494:
1481:
1468:
1465:stellar wind
1449:extinguished
1445:bright giant
1434:bright giant
1426:Iota Aurigae
1424:
1405:
1402:
1361:Delta Leonis
1329:
1318:Beta Aurigae
1316:
1292:open cluster
1214:solar masses
1190:
1182:
1164:
1161:Bright stars
1092:
1087:
1083:
1079:
1075:
1067:
1060:iefangel uul
1059:
1055:
1051:
1047:
1013:
981:Late Classic
977:Aztec people
954:
949:
939:
930:
926:
922:
918:
913:
909:
905:
903:
869:
852:
846:
834:
828:
799:
780:
772:Johann Bayer
767:
758:
748:
741:
733:
718:
714:
710:
674:
667:Zeta Aurigae
649:
634:
623:
584:
579:Erichthonius
572:
527:
503:
474:
430:Beta Aurigae
419:
392:Erichthonius
367:
366:
355:
343:
116:
64:Abbreviation
36:
9455:Outer space
9443:Spaceflight
9165:Hippocampus
9024:Telescopium
8950:de Lacaille
8699:Sagittarius
8554:Capricornus
8549:Canis Minor
8544:Canis Major
8350:Telescopium
8315:Sagittarius
8035:Capricornus
8030:Canis Minor
8025:Canis Major
7013:θ (Mahasim)
6978:α (Capella)
6892:WIKISKY.ORG
6699:"X Aurigae"
6679:"U Aurigae"
6639:"R Aurigae"
6379:"9 Aurigae"
6359:"2 Aurigae"
5987:"HAT-P-9 b"
5575:(1): 9–28.
3941:: 571–581.
3914:: 593–602.
3497:(2): 1912.
3053:Bakich 1995
3001:Olcott 2004
2717:Bakich 1995
2705:Bakich 1995
2607:Psi Aurigae
2434:association
2259:Perseus Arm
2227:hot Jupiter
2212:hot Jupiter
2126:is a white
2081:carbon star
2046:Mu Columbae
1926:WZ Sagittae
1922:DQ Herculis
1892:Eta Aurigae
1660:Chi Aurigae
1622:Tau Aurigae
1524:metallicity
1508:photometric
1477:white dwarf
1453:hybrid star
1340:in 1890 by
1312:light-years
1203:solar radii
1191:ngahalapolu
1187:Ontong Java
1178:light-years
1056:evang-el-ul
1048:Jefegen uun
1005:petroglyphs
985:Monte Albán
940:In ancient
884:declination
865:Johann Bode
783:Bellerophon
723:Cleostratus
671:Eta Aurigae
506:Mesopotamia
411:declination
234:Stars with
185:Declination
9477:Categories
9280:Scarabaeus
9250:Polophylax
9110:Argo Navis
8979:Horologium
8833:Chamaeleon
8729:Ursa Minor
8724:Ursa Major
8719:Triangulum
8559:Cassiopeia
8519:Argo Navis
8375:Ursa Minor
8370:Ursa Major
8355:Triangulum
8160:Horologium
8065:Chamaeleon
8045:Cassiopeia
7766:Messier 38
7761:Messier 37
7756:Messier 36
7672:HD 49674 b
7667:HD 45350 b
7662:HD 43691 b
7657:HD 40979 b
7644:Exoplanets
7596:Gliese 268
7008:η (Haedus)
6998:ε (Almaaz)
6988:γ (Elnath)
6865:2012-09-18
6092:Star Tales
6072:Star Tales
5767:"Aurigids"
4933:References
4689:(2). L39.
4509:1803.11538
4438:1809.01228
4431:(5). 213.
4379:2003.02385
4372:(5): 197.
3673:Kaler 2011
3610:Moore 2000
3583:Kaler 2008
3548:Kaler 2009
3459:Moore 2000
3420:Moore 2000
3343:Davis 1944
3140:Staal 1988
3113:Aveni 1977
3089:Staal 1988
3039:Star Tales
3013:Staal 1988
2986:Allen 1899
2918:Staal 1988
2879:Staal 1988
2867:Krupp 2007
2853:Star Tales
2613:References
2377:red giants
2331:Struve 737
2307:AE Aurigae
2196:HD 49674 b
2181:HD 43691 b
2176:HD 45350 b
2148:HD 40979 b
2124:14 Aurigae
2108:arcseconds
2069:UV Aurigae
2042:53 Arietis
2026:AE Aurigae
2008:UU Aurigae
1995:SS Aurigae
1967:RW Aurigae
1963:RX Aurigae
1954:RT Aurigae
1950:supergiant
1860:luminosity
1755:Xi Aurigae
1698:Mu Aurigae
1603:Pi Aurigae
1573:magnitude
1568:magnitude
1542:Nu Aurigae
1408:Beta Tauri
1385:arcseconds
1259:luminosity
1052:efang alul
997:California
898:See also:
847: [
829: [
611:Hippolytus
599:Hippodamia
589:, who was
554:Amphictyon
542:Hephaestus
470:AE Aurigae
209:Main stars
162:Charioteer
9419:Astronomy
9200:Lumbricus
8945:Vulpecula
8925:Leo Minor
8906:Reticulum
8897:Monoceros
8664:Ophiuchus
8604:Delphinus
8564:Centaurus
8499:Andromeda
8395:Vulpecula
8305:Reticulum
8250:Ophiuchus
8230:Monoceros
8190:Leo Minor
8115:Delphinus
8050:Centaurus
7960:Andromeda
7862:4C +41.17
7771:Palomar 2
7146:Flamsteed
6739:"HR 1528"
6709:20 August
6689:20 August
6669:20 August
6649:20 August
6629:20 August
6609:20 August
6589:20 August
6569:20 August
6549:20 August
6169:12 August
6149:20 August
6021:12 August
6009:"GD 66 b"
5999:12 August
5977:12 August
5955:12 August
5933:12 August
5911:12 August
5855:17 August
5835:16 August
5815:12 August
5793:17 August
5685:0906.0977
5377:: 25–30.
5256:0706.0891
5232:: 13–24.
4924:Meng 2002
4888:Levy 2008
4876:Levy 2008
4864:Levy 2008
4816:Levy 2008
4769:Levy 2005
4729:119249005
4696:1206.1592
4628:0806.4008
4575:CiteSeerX
4465:119243619
4406:212414679
4321:0707.0958
3037:Ridpath,
2851:Ridpath,
2690:Ridpath,
2618:Citations
2586:2000 NL10
2558:fireballs
2514:radiating
2291:ε Aurigae
2283:ψ Aurigae
2251:Milky Way
2217:The star
2200:HAT-P-9 b
2120:4 Aurigae
2077:X Aurigae
2073:U Aurigae
2065:R Aurigae
2012:red giant
1946:ψ Aurigae
1918:slow nova
1910:T Aurigae
1899:450
1774:9 Aurigae
1679:2 Aurigae
1588:G8.5IIIb
1473:supernova
1304:red dwarf
1183:al-'Ayyuq
1099:Quturjuuk
1080:Tahi-anii
1040:Alinablab
1036:Ligedaner
979:, as the
923:Tianhuang
819:to honor
766:, called
645:Argonauts
619:Asclepius
571:entitled
442:Milky Way
305:Bordering
223:Flamsteed
157:Symbolism
121:genitive
9295:Solarium
9245:Phaethon
9175:Jordanus
9130:Cerberus
9115:Asterion
9095:Antinous
9085:Anguilla
9019:Sculptor
8969:Circinus
8911:Hevelius
8902:Habrecht
8883:Plancius
8750:Category
8704:Scorpius
8629:Hercules
8619:Eridanus
8614:Equuleus
8504:Aquarius
8325:Sculptor
8320:Scorpius
8155:Hercules
8135:Eridanus
8130:Equuleus
8070:Circinus
7975:Aquarius
7908:Category
7849:Galaxies
7698:clusters
7682:WASP-12b
7677:KELT-2Ab
7326:Variable
7030:(Alhurr)
6894:: Auriga
6068:"Auriga"
5826:"Al Kab"
5710:16052567
5324:: 39–40.
4944:. Dover.
4597:17608922
4346:18805775
3025:OED 2012
2760:Rogers,
2744:Rogers,
2729:RECONS,
2678:, Auriga
2596:See also
2494:Aurigids
2474:NGC 2126
2470:NGC 1857
2466:NGC 1778
2458:eyepiece
2446:emission
2441:NGC 1931
2426:NGC 1893
2414:NGC 2281
2402:NGC 1907
2299:NGC 1893
2287:NGC 1664
2279:NGC 2281
2261:and the
2223:KELT-2Ab
2191:HD 49674
2185:HD 43691
2172:HD 45350
2144:HD 40979
2132:HD 30453
2104:aperture
2100:☉
1999:SS Cygni
1991:hydrogen
1904:☉
1880:☉
1868:☉
1826:☉
1812:F0 class
1576:Distance
1571:Absolute
1566:Apparent
1561:Spectral
1549:☉
1532:nitrogen
1515:lifespan
1504:infrared
1490:☉
1441:☉
1432:(K-type
1414:(B-type
1357:☉
1326:subgiant
1324:(A-type
1284:☉
1277:☉
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1228:☉
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1129:Features
1084:Hoku-lei
1064:Pukapuka
1032:Pleiades
1028:Scorpius
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699:Almagest
659:asterism
655:Amalthea
643:and the
626:Phaethon
595:Oenomaus
587:Myrtilus
550:quadriga
538:chthonic
514:MUL.APIN
510:scimitar
482:Aurigids
480:for the
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291:Aurigids
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9378:Xiphias
9315:Testudo
9240:Patella
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8920:Lacerta
8892:Columba
8868:Phoenix
8709:Serpens
8694:Sagitta
8679:Perseus
8674:Pegasus
8569:Cepheus
8487:Ptolemy
8340:Sextans
8335:Serpens
8310:Sagitta
8275:Phoenix
8270:Perseus
8265:Pegasus
8180:Lacerta
8075:Columba
8055:Cepheus
7826:IC 2149
7785:Nebulae
7626:WASP-12
7611:MWC 480
7379:AR (17)
7344:RT (48)
6834:Bibcode
6772:Bibcode
6749:17 July
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6529:27 June
6509:26 June
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2590:Taurids
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2156:parsecs
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759:Hyginus
750:Hyginus
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615:Phaedra
609:'s son
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540:son of
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265:Capella
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