List of stars in Auriga - AbsoluteAstronomy.com

This is the list of notable star

Star

A star is a massive, luminous sphere of plasma held together by gravity. At the end of its lifetime, a star can also contain a proportion of degenerate matter. The nearest star to Earth is the Sun, which is the source of most of the energy on Earth...

s in the constellation

Constellation

In modern astronomy, a constellation is an internationally defined area of the celestial sphere. These areas are grouped around asterisms, patterns formed by prominent stars within apparent proximity to one another on Earth's night sky....

Auriga
Auriga (constellation)
Auriga is a constellation in the northern sky. Its name is Latin for 'charioteer' and its stars form a shape that has been associated with the pointed helmet of a charioteer. It was one of the 48 constellations listed by the 2nd century astronomer Ptolemy, and remains among the 88 modern...

, sorted by decreasing brightness.

Name	B Bayer designation A Bayer designation is a stellar designation in which a specific star is identified by a Greek letter, followed by the genitive form of its parent constellation's Latin name...	F Flamsteed designation Flamsteed designations for stars are similar to Bayer designations, except that they use numbers instead of Greek letters. Each star is assigned a number and the Latin genitive of the constellation it lies in...	HD Henry Draper Catalogue The Henry Draper Catalogue is an astronomical star catalogue published between 1918 and 1924, giving spectroscopic classifications for 225,300 stars; it was later expanded by the Henry Draper Extension , published between 1925 and 1936, which gave classifications for 46,850 more stars, and by the...	HIP	vis. mag. Apparent magnitude The apparent magnitude of a celestial body is a measure of its brightness as seen by an observer on Earth, adjusted to the value it would have in the absence of the atmosphere...	abs. mag. Absolute magnitude Absolute magnitude is the measure of a celestial object's intrinsic brightness. it is also the apparent magnitude a star would have if it were 32.6 light years away from Earth...	Dist. (ly)	Sp. class Stellar classification In astronomy, stellar classification is a classification of stars based on their spectral characteristics. The spectral class of a star is a designated class of a star describing the ionization of its chromosphere, what atomic excitations are most prominent in the light, giving an objective measure...	Notes
Capella Capella (star) Capella is the brightest star in the constellation Auriga, the sixth brightest star in the night sky and the third brightest star in the northern celestial hemisphere, after Arcturus and Vega. Although it appears to be a single star to the naked eye, it is actually a star system of four stars in...	α	13	34029	24608	0.08	−0.48	42	G8III / G0III	Alhajoth, Alhaior, Althaiot, Alhaiset, Alhatod, Alhojet, Alanac, Alanat, Alioc; quadruple star Multiple star A multiple star consists of three or more stars which appear from the Earth to be close to one another in the sky. This may result from the stars being physically close and gravitationally bound to each other, in which case it is physical, or this closeness may be merely apparent, in which case... , spectroscopic binary; 11th and 14th brightest stars
β Aur Beta Aurigae Beta Aurigae , traditionally named Menkalinan, is a white subgiant ternary star system approximately 85 light-years away in the constellation Auriga.- Nomenclature :...	β	34	40183	28360	1.90	−0.10	82	A2V	Menkalinan, Menkalina; eclipsing spectroscopic binary; Algol variable Algol variable Algol variables or Algol-type binaries are a class of eclipsing binary stars where the orbital plane of the stars are coincident with the line of sight from Earth. When the cooler component passes in front of the hotter one, part of the latter's light is blocked, and the total brightness of the...
θ Aur Theta Aurigae Theta Aurigae is a binary star in the constellation Auriga. It is approximately 173 light-years from Earth. Rarely used proper names for this star include Bogardus and Mahasim, the latter from the Arabic المِعْصَم al-micşam "wrist" , which was also used for Eta Aurigae.The primary, θ Aurigae A,...	θ	37	40312	28380	2.65	−0.98	173	A0p Si	Mahasim, Maha-Sim, Manus; α² CVn variable
ι Aur Iota Aurigae Iota Aurigae is a star in the constellation Auriga. It has the traditional name Al Kab, short for Kabdhilinan, from the Arabic الكعب ذي العنان al-kacb ðīl-cinān "the ankle of the rein holder "...	ι	3	31398	23015	2.69	−3.29	512	K3IIvar	Kabdhilinan, Hassaleh
ε Aur Epsilon Aurigae Epsilon Aurigae is a star in the constellation Auriga. It is traditionally known as Almaaz, Haldus, or Al Anz. Epsilon Aurigae is an unusual eclipsing binary system comprising an F0 supergiant and a companion which is generally accepted to be a huge dark disk orbiting an unknown object, possibly a...	ε	7	31964	23416	3.03	−5.95	2037	F0Ia	Almaaz, Maaz, Al Maz, Al Anz; long period eclipsing binary; Algol variable
η Aur Eta Aurigae Eta Aurigae is a star in the constellation Auriga. Along with ζ Aurigae it represents one of the Kids of the she-goat Capella, from which it gets its Latin traditional name Hoedus II or Haedus II, from the Latin hædus "kid"; Zeta Aurigae is Hoedus I...	η	10	32630	23767	3.18	−0.96	219	B3V	Haedus II, Hoedus II, Haedus, Maha-Sim
ζ Aur Zeta Aurigae Zeta Aurigae is a star in the constellation Auriga. It has the traditional names Haedus and Sadatoni . It is one of the two hædi of the she-goat Capella, the other being Hoedus II, Eta Aurigae...	ζ	8	32068	23453	3.69	−3.22	787	K4II comp	Sadatoni, Saclateni, Haedus I, Hoedus I; eclipsing binary; Algol variable
δ Aur	δ	33	40035	28358	3.72	0.55	140	K0III	Prijipati, Praja
ν Aur	ν	32	39003	27673	3.97	−0.13	215	K0III
π Aur Pi Aurigae Pi Aurigae is a star in the constellation Auriga.Pi Aurigae is a red M-type bright giant with a mean apparent magnitude of +4.30. It is approximately 840 light-years from Earth. It is classified as an irregular variable star and its brightness varies from magnitude +4.24 to +4.34.-References:* *...	π	35	40239	28404	4.30	−2.76	840	M3IIvar
κ Aur	κ	44	43039	29696	4.32	0.75	169	G8IIIvar
τ Aur	τ	29	38656	27483	4.51	0.44	213	G8III
16 Aur 16 Aurigae 16 Aurigae is a star in the constellation Auriga. Its apparent magnitude is 4.54.-References:* * *...		16	34334	24727	4.54	0.26	234	K3III...
λ Aur Lambda Aurigae Lambda Aurigae is a binary star in the constellation Auriga. It is approximately 41.2 light-years from Earth.The primary component, λ Aurigae A, is a yellow G-type subgiant with an apparent magnitude of +4.69. Its companion, λ Aurigae B, is 29 arcseconds away and has an apparent magnitude of +13.4...	λ	15	34411	24813	4.69	4.18	41	G0V	Al Hurr
χ Aur Chi Aurigae Chi Aurigae is a binary star in the constellation Auriga. It is at least 2000 light-years from Earth.Chi Aurigae is a spectroscopic binary which is classified as a blue-white B-type supergiant with an apparent magnitude of +4.71. The binary has an orbital period of 655.16 days.-References:* *...	χ	25	36371	25984	4.71	−5.77	4075	B5Iab
υ Aur Upsilon Aurigae Upsilon Aurigae is a star in the constellation Auriga.Upsilon Aurigae is a M-type red giant with an apparent magnitude of +4.72. It is approximately 475 light-years from Earth.-References:* *...	υ	31	38944	27639	4.72	−1.10	475	M1III
2 Aur 2 Aurigae 2 Aurigae is a star in the constellation Auriga. Its apparent magnitude is 4.79.It forms an attractive four-star asterism when viewed in a low power eyepiece, together with the nearby Hip 22647 and another very loose visual pair, Hip 22776 and Hip 22744, all above magnitude 8.-References:* *...		2	30834	22678	4.79	−1.39	561	K3III
ψ² Aur	ψ²	50	47174	31832	4.80	−0.81	432	K3III	part of Dolones (ψ Aur)
μ Aur Mu Aurigae Mu Aurigae is a star in the constellation Auriga.μ Aurigae is a white A-type main sequence dwarf with an apparent magnitude of +4.82. It is approximately 162 light-years from Earth.-Name:...	μ	11	33641	24340	4.82	1.33	162	A4m
63 Aur 63 Aurigae 63 Aurigae is a star in the constellation Auriga. Its apparent magnitude is 4.91.-References:* *...		63	54716	34752	4.91	−0.86	464	K4II-III
ψ¹ Aur Psi1 Aurigae Psi1 Aurigae is a star in the constellation Auriga.ψ1 Aurigae is an orange K-type supergiant with a mean apparent magnitude of +4.92. It is approximately 3837 light-years from Earth. It is classified as an irregular variable star and its brightness varies from magnitude +4.75 to...	ψ¹	46	44537	30520	4.92	−5.43	3835	K5Iabvar	part of Dolones (ψ Aur)
ω Aur Omega Aurigae 4 Aurigae or Omega Aurigae is a star in the constellation Auriga. Its apparent magnitude is 4.93. Its distance from the Sun is 1,324,300 km. Its luminosity is 20.6 x the Sun. Its apparent diameter is 154 deg. 48' 4.6. Associated with EUVE J0459+37.8 is UV-emission source .-References:* * *...	ω	4	31647	23179	4.93	1.49	159	A1V	Binary, associated to EUVE J0459+37.8 is UV-emission source
ξ Aur Xi Aurigae Xi Aurigae is a star in the constellation Auriga.ξ Aurigae is a white A-type main sequence dwarf with an apparent magnitude of +4.96. It is approximately 241 light-years from Earth.-References:* *...	ξ	30	39283	27949	4.96	0.62	241	A2V
9 Aur 9 Aurigae 9 Aurigae or V398 Aurigae is a star in the constellation Auriga. Its apparent magnitude is 4.98.-Components:-References:* * *...		9	32537	23783	4.98	2.89	85	F0V	V398 Aurigae, Gamma Doradus variable Gamma Doradus variable Gamma Doradus variables are variable stars which display variations in luminosity due to non-radial pulsations of their surface. The stars are typically young, early F or late A type main sequence stars, and typical brightness fluctuations are 0.1 magnitudes with periods on the order of one day...
ψ⁷ Aur	ψ⁷	58	49520	32844	4.99	−0.25	364	K3III	part of Dolones (ψ Aur)
KW Aur 14 Aurigae 14 Aurigae or KW Aurigae is a star in the constellation Auriga. Its apparent magnitude is 5.01.-Components:-References:* * *...		14	33959	24504	5.01	0.43	269	A9IV	δ Sct variable Delta Scuti variable A Delta Scuti variable is a variable star which exhibits variations in its luminosity due to both radial and non-radial pulsations of the star's surface. Typical brightness fluctuations are from 0.003 to 0.9 magnitudes in V over a period of a few hours, although the amplitude and period of the... ; multiple star system
σ Aur	σ	21	35186	25292	5.02	−0.97	513	K4III
ψ⁴ Aur Psi4 Aurigae Psi4 Aurigae is a star in the constellation Auriga.ψ4 Aurigae is an orange K-type giant with an apparent magnitude of +5.04. It is approximately 306 light-years from Earth.-References:* *...	ψ⁴	55	47914	32173	5.04	0.18	306	K5III	part of Dolones (ψ Aur)
19 Aur 19 Aurigae 19 Aurigae is a star in the constellation Auriga. Its apparent magnitude is 5.05.-References:* *...		19	34578	24879	5.05	−4.82	3075	A5IIvar
φ Aur	φ	24	35620	25541	5.08	−0.37	400	K4IIIp
65 Aur		65	57264	35710	5.12	0.84	235	K0III
ρ Aur Rho Aurigae Rho Aurigae is a star in the constellation Auriga, spectroscopic binary.ρ Aurigae is a blue-white B-type main sequence dwarf with an apparent magnitude of +5.22. It is approximately 642 light-years from Earth.-Name:...	ρ	20	34759	25048	5.22	−1.25	642	B5V
ψ⁶ Aur Psi6 Aurigae Psi6 Aurigae is a star in the constellation Auriga.ψ6 Aurigae is an orange K-type giant with an apparent magnitude of +5.22. It is approximately 424 light-years from Earth.-References:* *...	ψ⁶	57	48781	32562	5.22	−0.35	424	K1III	part of Dolones (ψ Aur)
66 Aur 66 Aurigae 66 Aurigae is a star in the constellation Auriga. Its apparent magnitude is 5.2.-References:* *...		66	57669	35907	5.23	−1.51	728	K0III
ψ⁵ Aur	ψ⁵	56	48682	32480	5.24	4.15	54	G0V	part of Dolones (ψ Aur)
49 Aur 49 Aurigae 49 Aurigae is a star in the constellation Auriga. Its apparent magnitude is 5.26.-References:* *...		49	46553	31434	5.26	−0.42	447	A0Vnn
45 Aur 45 Aurigae 45 Aurigae or PLX 1468.2 is a star in the constellation Auriga. Its apparent magnitude is 5.34.-References:* * -Components:...		45	43905	30247	5.34	1.56	186	F5III...
ψ³ Aur Psi3 Aurigae Psi3 Aurigae is a star in the constellation Auriga.ψ3 Aurigae is a blue-white B-type giant with an apparent magnitude of +5.34. It is approximately 760 light-years from Earth.-References:* *...	ψ³	52	47100	31789	5.34	−1.49	758	B8III	part of Dolones (ψ Aur)
40 Aur 40 Aurigae 40 Aurigae is a star in the constellation Auriga. Its apparent magnitude is 5.36.-References:* * *...		40	41357	28946	5.36	0.01	380	A4m
IQ Aur IQ Aurigae IQ Aurigae is variable star.-References:* *...			34452	24799	5.38	−0.31	448	A0p...	α² CVn variable
26 Aur 26 Aurigae 26 Aurigae is a star in the constellation Auriga. Its apparent magnitude is 5.40.-References:* * * -Components:...		26	37269	26536	5.40	−0.29	447	A2V + GIII
UU Aur UU Aurigae UU Aurigae is a carbon star and binary star in the constellation Auriga. It is approximately 1810 light-years from Earth.UU Aurigae is a carbon-rich C-type giant, with a mean apparent magnitude of +5.4...			46687	31579	5.40	−3.32	1811	C5II	semiregular variable
			34557	24902	5.46	0.60	306	A3V
ο Aur Omicron Aurigae Omicron Aurigae is a star in the constellation Auriga. Its apparent magnitude is 5.46. It is approximately 482 light-years away from Earth, which makes it barely visible to the naked eye despite the fact that it gives off more energy than Sirius, the brightest star in the sky. ο Aurigae is a...	ο	27	38104	27196	5.46	−0.39	482	A0p...
			34904	25143	5.54	0.72	300	A3V
PU Aur PU Aurigae PU Aurigae is a variable star.-References:* *...			34269	24738	5.55	−1.09	694	M4III	variable star
			30454	22393	5.57	1.29	235	K2III
			30557	22545	5.64	0.67	321	G9III
			34790	25001	5.66	1.00	278	A1Vs
			33167	24109	5.67	2.35	151	F5V
			30823	22699	5.68	−0.32	517	A3III
			35600	25492	5.69	−3.56	2312	B9Ib
51 Aur 51 Aurigae 51 Aurigae is a star in the constellation Auriga. Its apparent magnitude is 5.70.-References:* *...		51	47070	31771	5.70	0.76	317	K5III
36 Aur 36 Aurigae 36 Aurigae or V444 Aurigae is a star in the constellation Auriga. Its apparent magnitude is 5.71.-References:* *...		36	40394	28499	5.71	−1.77	1022	B9.5p SiFe	V444 Aur; α² CVn variable
			36678	26344	5.74	−1.06	746	M0III
RT Aur RT Aurigae RT Aurigae is a star in the constellation Auriga.RT Aurigae is a yellow-white F-type supergiant with a mean apparent magnitude of +5.75. It is approximately 1561 light-years from Earth. It is classified as a Cepheid variable star and its brightness varies from magnitude +5.00 to +5.82 with a...		48	45412	30827	5.75	−2.65	1560	F5.5Ibv	Cepheid variable Cepheid variable A Cepheid is a member of a class of very luminous variable stars. The strong direct relationship between a Cepheid variable's luminosity and pulsation period, secures for Cepheids their status as important standard candles for establishing the Galactic and extragalactic distance scales.Cepheid...
53 Aur 53 Aurigae 53 Aurigae is a star in the constellation Auriga. Its apparent magnitude is 5.76.-References:* * * -Components:...		53	47152	31737	5.76	0.20	421	B9npe...
41 Aur A 41 Aurigae 41 Aurigae is a binary star in the constellation Auriga. Its apparent magnitude is 5.64. It is approximately 323 light years form Earth.-References:* * *...		41	42126	29388	5.78	0.88	311	A3V+...	binary star Binary star A binary star is a star system consisting of two stars orbiting around their common center of mass. The brighter star is called the primary and the other is its companion star, comes, or secondary...
			42471	29451	5.78	−2.40	1411	M1III
WW Aur WW Aurigae WW Aurigae is an eclipsing binary in the constellation Auriga. It is approximately 275 light-years from Earth.Both components, WW Aurigae A and WW Aurigae B, are detached white A-type main sequence dwarfs with a mean apparent magnitude of +5.82...			46052	31173	5.82	1.19	275	A3m + A3m
			30453	22407	5.84	0.78	336	A8m
ψ⁹ Aur Psi9 Aurigae Psi9 Aurigae is a star in the constellation Auriga.ψ9 Aurigae is a blue-white B-type giant with an apparent magnitude of +5.85. It is approximately 826 light-years from Earth.-References:* *...	ψ⁹		50658	33377	5.85	−1.17	825	B8III	part of Dolones (ψ Aur)
64 Aur 64 Aurigae 64 Aurigae is a star in the constellation Auriga. Its apparent magnitude is 5.87....		64	56221	35341	5.87	1.30	268	A5Vn
47 Aur 47 Aurigae 47 Aurigae is a star in the constellation Auriga. Its apparent magnitude is 5.88....		47	45466	30972	5.88	−0.18	530	K4III
			50763	33415	5.88	0.83	334	K0III:
			39586	27973	5.90	1.42	256	A5IV
			40084	28343	5.90	−1.79	1124	G5III
39 Aur 39 Aurigae 39 Aurigae is a star in the constellation Auriga. Its apparent magnitude is 5.90....		39	41074	28823	5.90	2.34	168	F3V
			35520	25471	5.92	−2.06	1289	A1p
			35239	25291	5.94	−1.07	821	B9III
5 Aur 5 Aurigae 5 Aurigae is a star in the constellation Auriga. Its apparent magnitude is 5.98.-References:* * *...		5	31761	23261	5.95	2.33	173	F5V
V433 Aur V433 Aurigae V433 Aurigae is a variable star.-References:* *...			37367	26606	5.98	−1.81	1177	B2IV-V
			40486	28562	5.98	−0.64	686	K0
AE Aur AE Aurigae AE Aurigae is a runaway star in the constellation Auriga; it lights the Flaming Star Nebula.AE Aurigae is a blue O-type main sequence dwarf with a mean apparent magnitude of +5.99. It is classified as an Orion type variable star and its brightness varies irregularly between magnitudes +5.78 and...			34078	24575	5.99	−2.26	1455	O9.5Vvar	runaway star; Orion variable Orion variable An Orion variable is a variable star which exhibits irregular and eruptive variations in its luminosity and is typically associated with diffuse nebulae. It is thought that these are young stars which will later become regular, non-variable stars on the zero-age main sequence...
			36040	25816	5.99	0.62	386	K0IIIp
V394 Aur			41429	28930	6.01	−1.18	893	M3II comp
			33203	24072	6.02	−2.97	2050	B2II: comp
54 Aur 54 Aurigae 54 Aurigae is a star in the constellation Auriga. Its apparent magnitude is 6.02.-References:* * *...		54	47395	31852	6.02	−0.67	709	B7III
62 Aur 62 Aurigae 62 Aurigae is a star in the constellation Auriga. Its apparent magnitude is 6.02....		62	51440	33614	6.02	−0.31	603	K2III
			50056	33044	6.03	−0.62	698	K3III:
			37519	26712	6.04	0.10	502	B9.5III-IVp
			39225	27778	6.04	−0.75	744	M2II:
			40626	28637	6.04	0.54	410	B9.5IV
			31069	22842	6.06	0.97	340	A0V
			42466	29569	6.07	0.61	403	K1III
			36891	26363	6.08	−3.38	2547	G3Ib
38 Aur 38 Aurigae 38 Aurigae is a star in the constellation Auriga. Its apparent magnitude is 6.08. It is approximately 71.84 light years from Earth....		38	40801	28677	6.08	1.56	261	K0III
41 Aur B 41 Aurigae 41 Aurigae is a binary star in the constellation Auriga. Its apparent magnitude is 5.64. It is approximately 323 light years form Earth.-References:* * *...		41	42127		6.09				component of the 41 Aur system
			31327	22955	6.10	−6.66	11643	B2Ib
			36719	26315	6.10	1.05	333	F0V:
59 Aur 59 Aurigae 59 Aurigae or OX Aurigae is a star in the constellation Auriga. Its apparent magnitude is 6.10.-Components:-References:* * *...		59	50018	33041	6.10	0.04	530	F2V	OX Aur; δ Sct variable
			32188	23511	6.11	−2.87	2037	A2sh
			41330	28908	6.12	4.01	86	G0V
			32406	23583	6.14	−0.12	581	K0II-III
			40083	28390	6.14	1.04	341	K2III
AR Aur AR Aurigae AR Aurigae is an eclipsing binary in the constellation Auriga. It is approximately 398 light-years from Earth.Both components are blue-white B-type or main sequence dwarfs which do not fill their Roche lobes...		17	34364	24740	6.15	0.72	398	B9.5V	eclipsing binary
			41467	29025	6.15	−0.89	834	K0III
			33654	24451	6.16	−2.45	1716	A0V
V352 Aur V352 Aurigae V352 Aurigae is a variable star.-References:* *...			50420	33269	6.16	−0.97	869	A9III	δ Sct variable
HD 35519 HD 35519 HD 35519 is a star in star clusters NGC 1912 and NGC 1907.-References:* *...			35519	25476	6.17	−0.31	644	K2	Star in Cluster NGC 1912 and NGC 1907 NGC 1907 NGC 1907 is a open star cluster around 4,500 light years from Earth. It contains around 30 stars and is over 500 million years old. With a magnitude of 8.2 it is visible as part of the constellation Auriga.- Sources :**...
			35521	25475	6.18	1.06	344	K0
			40588	28517	6.18	1.70	256	A2V
			53925	34462	6.19	−0.45	695	K1III
			32655	23799	6.20	−0.91	860	F2IIp...
			35984	25730	6.20	1.45	290	F6III
V538 Aur V538 Aurigae V538 Aurigae is variable of BY Dra type. It has a spectral class of K1e and is located 39.9 light-years from Earth. The stars diameter is 0.84 times the sun and it has a metallicity 63% that of the Sun making it relatively metal poor....			37394	26779	6.21	5.77	40	K1V	BY Draconis variable BY Draconis variable BY Draconis variables are main sequence variable stars of late spectral types, usually K or M. The name comes from the archetype for this category of variable star system, BY Draconis. They exhibit variations in their luminosity due to rotation of the star coupled with star spots, and other...
			40325	28438	6.21	0.97	365	K2III...
			48073	32190	6.21	0.38	478	K0
			34332	24771	6.22	−0.36	676	K0
NO Aur			37536	26718	6.23	−1.89	1370	M2SIab	S star type
			40832	28644	6.23	2.74	163	F4V
			41269	28861	6.23	−1.06	937	B9sp...
			49949	33056	6.24	1.03	359	A8Vn
			36499	26071	6.27	0.78	408	A3IV
V440 Aur			39045	27661	6.28	0.03	580	M3III
			42083	29404	6.28	1.27	327	A5m
			38765	27625	6.29	1.62	281	K1III
			35238	25290	6.30	−0.49	744	K1III...
			38358	27319	6.30	−0.42	720	K0
			50384	33271	6.31	0.96	383	K0III-IV
			41162	28820	6.32	−0.50	755	K0III+...
60 Aur		60	50037	33064	6.32	2.23	214	F5V:
43 Aur 43 Aurigae 43 Aurigae is a star in the constellation Auriga. Its apparent magnitude is 6.33....		43	43380	29949	6.33	1.20	346	K2III
			56941	35623	6.33	−0.63	805	K0
			41636	29114	6.34	0.99	384	G9III
			39866	28117	6.35	−3.88	3622	A2II
			47270	31889	6.35	−0.19	663	K1III
			37138	26463	6.36	0.44	498	K0
			48272	32268	6.37	−0.85	908	A2V
			36041	25810	6.38	0.63	460	G9III
			40722	28642	6.38	0.88	410	K0
			40873	28765	6.39	0.98	394	A7III
			37646	26781	6.40	0.46	502	B8IV
			39182	27777	6.40	−0.14	661	A2V
			57263	35725	6.40	0.33	533	K0
			35681	25580	6.41	3.76	110	F5
			44092	30200	6.41	1.33	338	A1Vs
			33463	24193	6.42	−1.31	1144	M2III
			40062	28385	6.42	1.32	342	A5m
			45192	30741	6.43	0.80	435	K0
			37250	26592	6.44	2.02	250	K0
22 Aur 22 Aurigae 22 Aurigae is a star in the constellation Auriga. Its apparent magnitude is 6.45....		22	35076	25192	6.45	0.15	593	B9Vs
6 Aur 6 Aurigae 6 Aurigae is a star in the constellation Auriga. Its apparent magnitude is 6.46....		6	31780	23268	6.46	−1.45	1244	K5III
ψ⁸ Aur Psi8 Aurigae Psi8 Aurigae is a star in the constellation Auriga.ψ8 Aurigae is a blue-white B-type main sequence dwarf with an apparent magnitude of +6.46. It is approximately 826 light-years from Earth.-References:* *...	ψ⁸	61	50204	33133	6.46	−0.56	825	B9.5sp...	part of Dolones (ψ Aur)
			38229	27293	6.47	0.63	481	G5
V403 Aur			39743	28162	6.47		583	G8III	RS CVn variable RS Canum Venaticorum variable RS Canum Venaticorum variables are a type of variable star. They are close binary stars having active chromospheres which can cause large stellar spots. These spots are believed to cause variations in their observed luminosity...
			33632	24332	6.48	4.41	85	F8
			47703	32040	6.48	2.00	256	F8III
			51021	33453	6.48	−0.94	994	M3
			56171	35317	6.48	0.45	524	K0
			29867	22003	6.49	2.20	235	A8V
			32608	23724	6.49	1.91	269	A5V
18 Aur 18 Aurigae 18 Aurigae is a star in the constellation Auriga. Its apparent magnitude is 6.49.-References:* * *...		18	34499	24832	6.49	2.20	235	A7V
			34498	24881	6.49	−0.83	948	K0
			35202	25301	6.49	−1.82	1495	K2
			40650	28634	6.49	4.22	93	F5
			49364	32746	6.49	−0.33	753	K5
			36484	26054	6.50	1.70	297	A2m
			38200	27164	6.50	−0.94	1003	K0
42 Aur 42 Aurigae 42 Aurigae is a star in the constellation Auriga. Its apparent magnitude is 6.53.The star was discovered in 1983 by amateur astronomers....		42	43244	29884	6.53	2.24	235	F0V
HD 40979 HD 40979 HD 40979 is a yellow-white dwarf star about 109 light-years away in the constellation of Auriga. The star is a member of a multiple system: it has a companion HD 40979B which shares its proper motion and is located at a projected distance of 6400 AU from the primary...			40979	28767	6.74	4.13	109	F8V	has a planet Extrasolar planet An extrasolar planet, or exoplanet, is a planet outside the Solar System. A total of such planets have been identified as of . It is now known that a substantial fraction of stars have planets, including perhaps half of all Sun-like stars... (b HD 40979 b HD 40979 b is an extrasolar planet orbiting the star HD 40979, was detected from the Lick and Keck observatories and photometric observations at Fairborn Observatory reveal low-amplitude brightness variations in HD 40979. It is thought to be a large gas giant planet. It was discovered in 2002 by... )
12 Aur 12 Aurigae 12 Aurigae is a star in the constellation Auriga. Its apparent magnitude is 6.9.-References:*...		12	33988		6.90			B5
AB Aur AB Aurigae AB Aurigae is a star in the Auriga constellation. It is better known for hosting a dust disk that may harbour a condensing planet or brown dwarf. The star could host a possible substellar companion in wide orbit.-A planetary system?:...			31293	22910	7.06		469	A0Vpe	has a dust disk in which planets or brown dwarves may be forming
HD 45350 HD 45350 HD 45350 is an 8th magnitude star located approximately 160 light-years away in the constellation of Auriga. It is a yellow subgiant , a Sun-like star that is finishing hydrogen fusion in its core. Although slightly cooler, it is brighter, although not much considering its subgiant status...			45350	30860	7.88	4.43	160	G5IV	has a planet (b HD 45350 b HD 45350 b is an extrasolar planet located approximately 160 light-years away in the constellation of Auriga. It has a minimum mass about 1.79 times that of Jupiter... )
HD 43691 HD 43691 HD 43691 is a G-type star with magnitude +8.03 located approximately 260 light-years away in the constellation Auriga. This yellow star is about to stop thermonuclear hydrogen-fusion in its core and eventually expand to become a red giant....			43691	30057	8.03	3.18	304	G0IV-V	has a planet (b HD 43691 b HD 43691 b is a massive jovian planet located approximately 304 light-years away in the constellation of Auriga. Because the inclination is unknown, only the minimum mass is known. The planet orbits close to the star, closer than Mercury to the Sun.... )
HD 49674 HD 49674 HD 49674 is an 8th magnitude G-type main-sequence star located approximately 144 light years away in the constellation of Auriga. It has a very similar mass to our Sun...			49674	32916	8.10	5.05	133	G5V	has a planet (b HD 49674 b HD 49674 b is an extrasolar planet located approximately 134 light-years away in the constellation of Auriga, orbiting the star HD 49674. This planet was discovered orbiting the star in 2002. The planet is a gas giant and orbits extremely close to its star, which takes only 4.95 days to... )
GD 66 GD 66 GD 66 or V361 Aurigae is a 0.64 solar mass pulsating white dwarf star located 170 light years from Earth in the Auriga constellation. The estimated cooling age of the white dwarf is 500 million years...					15.56	12.02	166	DA	white dwarf White dwarf A white dwarf, also called a degenerate dwarf, is a small star composed mostly of electron-degenerate matter. They are very dense; a white dwarf's mass is comparable to that of the Sun and its volume is comparable to that of the Earth. Its faint luminosity comes from the emission of stored... , has a possible planet
EO Aur EO Aurigae EO Aurigae is an eclipsing binary of Algol type.-References:* *...			34333	24744	7.83		1200	B5	Algol variable
MZ Aur MZ Aurigae MZ Aurigae is a variable star.-References:* *...			34626	24938	8.16		4000	B1.5IVnp	variable star Variable star A star is classified as variable if its apparent magnitude as seen from Earth changes over time, whether the changes are due to variations in the star's actual luminosity, or to variations in the amount of the star's light that is blocked from reaching Earth...
V420 Aur V420 Aurigae V420 Aurigae is high mass X-ray binary star.-References:* *...			34921	25114	7.45		8000	B0IVpe	high mass X-ray Binary
V423 Aur V423 Aurigae V423 Aurigae is semi-regular variable pulsating star.-References:* *...			34986	25178	8.68		9000	B8	semi-regular pulsating star
IU Aur IU Aurigae IU Aurigae is a spectroscopic binary.-References:* *...			35652	25565	8.39		700	B3Vnne	spectroscopic binary
LY Aur LY Aurigae LY Aurigae is an eclipsing binary hypergiant of Beta Lyr type in the constellation Auriga.-References:* * * *...			35921	25733	6.85		2000	O9.5+O9.5eaII-III	Beta Lyrae variable Beta Lyrae variable Beta Lyrae variables are a class of close binary stars. Their total brightness is variable because the two component stars orbit each other, and in this orbit one component periodically passes in front of the other one, thereby blocking its light. The two component stars of Beta Lyrae systems are...
HAT-P-9 HAT-P-9 \|- bgcolor="#FFFAFA"\| Equatorial [ g ] \|\| 201,21 m/s2HAT-P-9 is a magnitude 12 star approximately 1560 light years away in the constellation Auriga.-Planetary system:...					12.34		1564.8	F	has a transiting planet HAT-P-9b HAT-P-9b HAT-P-9b is an extrasolar planet approximately 1560 light years away in the constellation Auriga. This planet was found by the transit method on June 26, 2008. It has mass 78% that of Jupiter and radius 140% that of Jupiter...
NX Aur NX Aurigae NX Aurigae is pre-main sequence star candidate.-References:* *...					14.1		13000	B4Ve	PMS star in NGC 1893 NGC 1893 NGC 1893 is an open cluster in the constellation Auriga.-References:* *...

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