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Multiple star system in the constellation Auriga
9 Aurigae (9 Aur) is a star system in the constellation Auriga. It has an apparent magnitude of about 5, making it visible to the naked eye in many suburban
9_Aurigae
Constellation in the northern celestial hemisphere
SIMBAD Sigma Aurigae. SIMBAD Omega Aurigae. SIMBAD Xi Aurigae. SIMBAD 9 Aurigae. SIMBAD Epsilon Aurigae. SIMBAD Zeta Aurigae. SIMBAD Eta Aurigae. Copeland
Auriga
Type of variable star
physical cause of the variations remains under investigation. The star 9 Aurigae was first noticed to be variable in 1990. However, none of the currently-accepted
Gamma_Doradus_variable
Star in the constellation Auriga
Iota Aurigae is a star in the northern constellation of Auriga. Its name is a Bayer designation that is Latinized from ι Aurigae, abbreviated Iota Aur
Iota_Aurigae
Multiple star system in the constellation of Auriga
consisting of Epsilon Aurigae, Zeta Aurigae, Eta Aurigae, Upsilon Aurigae, Nu Aurigae, Tau Aurigae, Chi Aurigae and 26 Aurigae. Consequently, the Chinese
Epsilon_Aurigae
Star in the constellation Auriga
AE Aurigae (abbreviated as AE Aur) is a runaway star in the constellation Auriga; it lights the Flaming Star Nebula. AE Aurigae is a blue O-type main sequence
AE_Aurigae
Lep b) 9 Aurigae C (V398 Aurigae) 87.65 ± 0.04 Auriga 05h 06m 40.62967s +51° 35′ 51.8025″ K5Ve 4.93 - 5.03 15 Pegasi 87.8 ± 0.12 F2V 5.53 9 Aurigae (V398
List of star systems within 85–90 light-years
List_of_star_systems_within_85–90_light-years
Star in the constellation Auriga
asterism consisting of Eta Aurigae, Epsilon Aurigae, Zeta Aurigae, Upsilon Aurigae, Nu Aurigae, Tau Aurigae, Chi Aurigae and 26 Aurigae. Consequently, the Chinese
Eta_Aurigae
Binary star system in the northern constellation of Auriga
Beta Aurigae is a binary star system in the northern constellation of Auriga. Its identifier is a Bayer designation that is Latinized from β Aurigae, and
Beta_Aurigae
Star in the constellation Auriga
AB Aurigae is a young Herbig Ae star in the Auriga constellation. It is located at a distance of approximately 509 light years from the Sun based on stellar
AB_Aurigae
Star in the constellation Auriga
Delta Aurigae, also named Bagu, is an astrometric binary star in the northern constellation of Auriga. This star is visible to the naked eye with an apparent
Delta_Aurigae
Star in the constellation Auriga
Psi9 Aurigae is a star in the northern constellation of Auriga. Its name is a Bayer designation that is Latinized from ψ9 Aurigae, and abbreviated Psi9
Psi9_Aurigae
Brightest star in the constellation Auriga
constellation of Auriga. It has the Bayer designation α Aurigae, which is Latinised to Alpha Aurigae and abbreviated Alpha Aur or α Aur. Capella is the sixth-brightest
Capella
T Tauri star in the Auriga constellation
GM Aurigae (GM Aur) is a K6V-type T Tauri star located 155 parsecs from Earth in the constellation of Auriga. It has a mass of 0.95 solar masses, a radius
GM_Aurigae
Star in the constellation Taurus
Tauri and abbreviated Beta Tau or β Tau. The original designation of Gamma Aurigae is now rarely used. It is a chemically peculiar B7 giant star, 134 light
Beta_Tauri
Brightest star in Earth's night sky
proposed Sirius Supercluster, along with other scattered stars such as Beta Aurigae, Alpha Coronae Borealis, Beta Crateris, Beta Eridani and Beta Serpentis
Sirius
Binary star in the constellation Auriga
Theta Aurigae is a binary star system in the constellation of Auriga. Its name is a Bayer designation that is Latinized from θ Aurigae, and abbreviated
Theta_Aurigae
Star in the constellation Auriga
V352 Aurigae is a variable star in the northern constellation of Auriga. It dimly visible to the naked eye with an apparent visual magnitude that ranges
V352_Aurigae
Binary star system in the constellation Auriga
asterism consisting of Zeta Aurigae, Epsilon Aurigae, Eta Aurigae, Upsilon Aurigae, Nu Aurigae, Tau Aurigae, Chi Aurigae and 26 Aurigae. Consequently, the Chinese
Zeta_Aurigae
Binary star system in the constellation Auriga
Chi Aurigae is a binary star system in the northern constellation of Auriga. Its name is a Bayer designation that is Latinized from χ Aurigae, and abbreviated
Chi_Aurigae
Emission and reflection nebula in the constellation Auriga
nebula around AE Aurigae Amateur photo of the Flaming Star Nebula taken with an AT72ED II telescope and ZWO ASI1600MM Pro camera—9 hours 30 minutes of
IC_405
Solar analog star in the constellation Auriga
Lambda Aurigae is a Sun-like star in the northern constellation of Auriga. Its name is a Bayer designation that is Latinized from λ Aurigae, and abbreviated
Lambda_Aurigae
Triple star system in the constellation Auriga
16 Aurigae is a triple star system located 340 light years away from the Sun in the northern constellation of Auriga. It is visible to the naked eye as
16_Aurigae
Star in constellation Auriga
V538 Aurigae is a single star in the northern constellation of Auriga. With an apparent visual magnitude of about 6.2, this star requires good dark sky
V538_Aurigae
Star in the constellation Auriga
Psi7 Aurigae, is a star in the northern constellation of Auriga. Its name is a Bayer designation that is Latinized from ψ7 Aurigae, and abbreviated Psi7
Psi7_Aurigae
Young binary star system in the constellation Auriga
Aurigae B was discovered in 1944. The two stars of the RW Aurigae system are separated by 1.448″, equivalent to 237 AU at the distance of RW Aurigae.
RW_Aurigae
Star in the constellation Auriga
IQ Aurigae is a (most likely) single, variable star in the northern constellation of Auriga. It is visible to the naked eye as a dim, white-hued star
IQ_Aurigae
British astronomer (1935–2021)
107 times. Krisciunas K, Griffin RF, Guinan EF, Luedeke KD, McCook GP. 9 Aurigae: strong evidence for non-radial pulsations. Monthly Notices of the Royal
Roger_Griffin_(astronomer)
Star in the constellation Perseus
1 Aurigae is the original name for a star now in the constellation Perseus. It was the first entry in John Flamsteed's catalogue of stars in Auriga. When
1_Aurigae
Star in the constellation Auriga
GD 66 or V361 Aurigae is a 0.64 solar mass (M☉) pulsating white dwarf star located 186 light years from Earth in the Auriga constellation. The estimated
GD_66
Substellar object orbiting AB Aurigae
AB Aurigae b is a directly imaged protoplanet or proto-brown dwarf embedded within the protoplanetary disk of the young, Herbig Ae/Be star AB Aurigae. The
AB_Aurigae_b
Star in the constellation Auriga
Phi Aurigae is a giant star in the northern constellation of Auriga. Its name is a Bayer designation that is Latinized from φ Aurigae, and abbreviated
Phi_Aurigae
Emission nebula in the constellation of Orion
which may have also created several known runaway stars, including AE Aurigae, Mu Columbae and 53 Arietis, which are believed to have been part of a
Barnard's_Loop
Open cluster in the constellation Auriga
conglomeration is positioned around half way between the brighter stars Beta Aurigae and Xi Aurigae. It is a challenge to find in a small telescope, having stars of
NGC_2126
Triple star system in the constellation Auriga
IU Aurigae is a triple star system in the constellation Auriga, consisting of an eclipsing binary pair orbiting a third component with a period of 335 years
IU_Aurigae
Star in the constellation Auriga
Psi4 Aurigae is a single, orange-hued star in the northern constellation of Auriga. Its name is a Bayer designation that is Latinized from ψ4 Aurigae, and
Psi4_Aurigae
Star in the constellation Auriga
63 Aurigae is a single star located around 395 light years away from the Sun in the northern constellation of Auriga. It is visible to the naked eye as
63_Aurigae
Binary star in the constellation Auriga
LY Aurigae is a multiple star system in the constellation Auriga. It is an eclipsing binary variable star, dropping in brightness by 0.7 magnitudes every
LY_Aurigae
Star in the constellation Auriga
39 Aurigae is a single star in the constellation of Auriga. The designation is from the star catalogue of English astronomer John Flamsteed, first published
39_Aurigae
Star in the constellation Auriga
Aurigae is a candidate binary star system in the northern constellation of Auriga. Its name is a Bayer designation that is Latinized from μ Aurigae,
Mu_Aurigae
Star in the constellation Auriga
SU Aurigae is a T Tauri-type variable star in the constellation Auriga. It is located about 500 light-years (150 parsecs) away in the Taurus-Auriga Star
SU_Aurigae
Binary star in the constellation Auriga
40 Aurigae is a binary star in the constellation Auriga. Its apparent magnitude is 5.345, meaning it can just barely be seen with the naked eye. Based
40_Aurigae
Binary star system in the constellation Auriga
60 Aurigae is a binary star system in the northern constellation of Auriga. The pair have a combined apparent visual magnitude of 6.319 and, based upon
60_Aurigae
Pattern of seven bright stars in the constellation Ursa Major
from Megrez (δ) to Dubhe (α) takes one in the direction of Capella (α Aurigae). A mnemonic for this is "Cap to Capella." Castor (α Geminorum) is reached
Big_Dipper
Diffuse nebula in the constellation Orion
the Orion Nebula cluster may have been the home of the runaway stars AE Aurigae, 53 Arietis, and Mu Columbae, which are currently moving away from the
Orion_Nebula
Red supergiant star in the constellation Orion
evidence that OB stars μ Columbae, AE Aurigae, and 53 Arietis all originated from such explosions in Ori OB1 2.2, 2.7, and 4.9 million years ago. A typical Type II-P
Betelgeuse
Star in the constellation Auriga
19 Aurigae is a single star located approximately 3,800 light years away from the Sun in the northern constellation Auriga. It is visible to the naked
19_Aurigae
including Antares and 119 Tauri. Examples of eclipsing binaries are Epsilon Aurigae (Almaaz), VV Cephei, and V766 Centauri (HR 5171). Angular diameter measurements
List_of_largest_stars
K-type giant star in the constellation Auriga
51 Aurigae is a single star in the northern constellation of Auriga. It is visible to the naked eye as a dim, orange-hued star with an apparent visual
51_Aurigae
Star in the constellation Auriga
V433 Aurigae is a variable star in the constellation Auriga. It is a slowly pulsating B star (SPB) that varies by a few hundredths of a magnitude over
V433_Aurigae
Binary star in the constellation Auriga
WW Aurigae is an eclipsing binary star system in the northern constellation of Auriga. It has a combined maximum apparent visual magnitude of 5.86, which
WW_Aurigae
Binary star in the constellation Auriga
Psi6 Aurigae is a spectroscopic binary star system in the northern constellation of Auriga. Its name is a Bayer designation that is Latinized from ψ6
Psi6_Aurigae
Multiple star system in the constellation Auriga
54 Aurigae is a multiple star system located around 800 light-years (51,000,000 AU) away from the Sun in the northern constellation of Auriga. It is visible
54_Aurigae
Star in the constellation of Auriga
UU Aurigae is a carbon star in the constellation Auriga. It is approximately 341 parsecs (1,110 light-years) from Earth. It is a variable star that is
UU_Aurigae
Star in the constellation Auriga
Psi8 Aurigae is a star in the northern constellation of Auriga. Its name is a Bayer designation that is Latinized from ψ8 Aurigae, and abbreviated Psi8
Psi8_Aurigae
Triple star system in the constellation Auriga
5 Aurigae is a triple star system in the northern constellation of Auriga, located about 178 light years away from the Sun based on parallax. It is just
5_Aurigae
Nova seen in 1964
QZ Aurigae, also known as Nova Aurigae 1964, was a nova which occurred in the constellation Auriga during 1964. It was discovered by Nicholas Sanduleak
QZ_Aurigae
the Constellations. Cambridge University Press. p. 170. ISBN 0-521-44921-9. Kaler, James B. "Saiph (Kappa Orionis)". Stars. University of Illinois. Archived
List_of_proper_names_of_stars
Star in the constellation Auriga
Omicron Aurigae is an astrometric binary star system in the northern constellation of Auriga. Its name is a Bayer designation that is Latinized from ο
Omicron_Aurigae
Star in the constellation Auriga
18 Aurigae is a star located 235 light years away from the Sun in the northern constellation of Auriga. The brightness of this object is near the limit
18_Aurigae
Large planetary embryo
formation for a gas giant. It is located in the gas disk of the star AB Aurigae. AB Aur b is among the largest exoplanets identified, and has a distant
Protoplanet
Variable star in the constellation Auriga
Nu Aurigae is a star in the northern constellation of Auriga. Its name is a Bayer designation that is Latinised from ν Aurigae, and abbreviated Nu Aur
Nu_Aurigae
Nova seen in 1891
T Aurigae (or Nova Aurigae 1891) was a nova, which lit up in the constellation Auriga in 1891. Thomas David Anderson, an amateur astronomer in Edinburgh
T_Aurigae
Binary star system in the constellation Auriga
65 Aurigae is a binary star system located 252 light years away from the Sun in the northern constellation of Auriga. It is visible to the naked eye as
65_Aurigae
Star in the constellation Auriga
64 Aurigae is a single star located 312 light years away from the Sun in the northern constellation of Auriga. It is visible to the naked eye as a dim
64_Aurigae
Star in the constellation Auriga
Pi Aurigae is a single, red-hued star in the northern constellation of Auriga. Its name is a Bayer designation that is Latinized from π Aurigae, and abbreviated
Pi_Aurigae
Classification of stars based on spectral properties
Upsilon Orionis B0Ia – Alnilam B2Ia – Chi2 Orionis B2Ib – 9 Cephei B3V – Alkaid B3V – Eta Aurigae B3Ia – Omicron2 Canis Majoris B5Ia – Eta Canis Majoris
Stellar_classification
Stellar classification distinguished by bright blue luminosity
remain unchanged since at least the 1940s, are Upsilon Orionis (B0 V), Eta Aurigae (B3 V), and Alkaid (B3 V). Besides these anchor standards, the seminal
B-type_main-sequence_star
Star in the constellation Auriga
R Aurigae (R Aur) is a Mira variable, a pulsating red giant star in the constellation of Auriga, at a distance of 930 light-years. In 1862 R Aurigae was
R_Aurigae
Zodiac constellation straddling the celestial equator
constellation of Auriga. As a result, it also bears the designation Gamma Aurigae. Zeta Tauri (the proper name is Tianguan) is an eclipsing binary star that
Taurus_(constellation)
Small number of stars that orbit each other
star groups or a multiple system. This event is credited with ejecting AE Aurigae, Mu Columbae and 53 Arietis at above 200 km·s−1 and has been traced to
Star_system
Triple star system in the constellation Auriga
AR Aurigae (AR Aur), also known by its Flamsteed designation 17 Aurigae, is a triple star in the constellation Auriga. Based on parallax measurements made
AR_Aurigae
Type of large cool star
Bootis) μ Leonis Gacrux (γ Crucis) Pollux (β Geminorum) Capella Aa (α Aurigae) Schedar (α Cassiopeiae) δ Andromedae ρ Persei Mira (ο Ceti) χ Cygni Rasalgethi
Red_giant
Star in the constellation Gemini
to its apparent magnitude of +9.89 it cannot be observed with the naked eye. The closest star to Gliese 251 is QY Aurigae, which is located 3.5 light years
Gliese_251
Brightest star in the constellation Lyra
FIRST: First on-sky demonstration on Keho'oea (α Lyrae) and Hokulei (α Aurigae)". Astronomy & Astrophysics. 677: A84. arXiv:2307.09746. Bibcode:2023A&A
Vega
Star in the constellation Auriga
Xi Aurigae is a single, white-hued star in the northern constellation of Auriga. Its name is a Bayer designation that is Latinized from ξ Aurigae, and
Xi_Aurigae
supernovae Variable star A higher magnitude means a lower brightness. i.e. T Aurigae (+3.8) was a brighter nova than HR Lyrae (+6.5) Prialnik, Dina. "Novae"
List of novae in the Milky Way galaxy
List_of_novae_in_the_Milky_Way_galaxy
Star in the constellation Auriga
47 Aurigae is a star located around 680 light years away from the Sun in the northern constellation of Auriga. It is visible to the naked eye as a dim
47_Aurigae
Aurigae 0043 K0 III, G1 III Northern 7 0.13 (0.05–0.18var) Rigel β Orionis 0860 B8 Ia Southern 8 0.34 Procyon α Canis Minoris 0011 F5 IV-V Northern 9
List_of_brightest_stars
T Tauri star; Chamaeleon
absolute magnitude of +6.55. The object was first suspected to be a RW Aurigae-type star in 1949. It was categorized as a T-Tauri star in 1975. In the
T_Chamaeleontis
Type of star, larger and brighter than the Sun
(σ Octantis), an F-type giant and a Delta Scuti variable; Capella Aa (α Aurigae Aa), a G-type giant. Beta Corvi (β Corvi), a G-type bright giant. The hottest
Giant_star
List of largest planets by size
"Images of embedded Jovian planet formation at a wide separation around AB Aurigae". Nature Astronomy. 6 (6): 751–759. arXiv:2204.00633. Bibcode:2022NatAs
List_of_largest_exoplanets
Constellation in the northern celestial hemisphere
"Properties of main-sequence eclipsing binaries - Into the G stars with HS Aurigae, FL Lyrae, and EW Orionis". The Astronomical Journal. 91: 383. Bibcode:1986AJ
Lyra
astronomer Williamina Fleming in 1888. Beta Aurigae binary star system The second spectroscopic binary, Beta Aurigae, was discovered in 1888 by Antonia Maury
List of inventions and discoveries by women
List_of_inventions_and_discoveries_by_women
Binary star system in the constellation Auriga
41 Aurigae is a binary star system located around 310–316 light years away from the Sun in the northern constellation of Auriga. It is visible to the
41_Aurigae
Star in the constellation Auriga
V394 Aurigae is a semi-regular variable star in the constellation Auriga. Its brightness varies between magnitudes 6.01 and 6.11, so it is faintly visible
V394_Aurigae
Show within 9 ly Show within 12 ly Show within 12 ly and directions This list covers all known stars, white dwarfs, brown dwarfs, and sub-brown dwarfs/rogue
List_of_nearest_stars
Mystery religion in the Roman Empire
relatively rapidly late in the reign of Antoninus Pius and under Marcus Aurelius (9). By that date, it is clear, the mysteries were fully institutionalised and
Mithraism
Type of star larger than main-sequence but smaller than a giant
Pegasi, ζ Cassiopeiae, η Lyrae B3: ι Herculis, η Aurigae B5: τ Herculis, δ Persei, CH Crucis A2: β Aurigae, λ Ursae Majoris, β Serpentis, α Ophiuchi A3:
Subgiant
Exoplanets confirmed or discovered from direct imaging
"Images of embedded Jovian planet formation at a wide separation around AB Aurigae". Nature Astronomy. 6 (6). Springer Science and Business Media LLC: 751–759
List of directly imaged exoplanets
List_of_directly_imaged_exoplanets
Unique identifier given to variable stars
to 45,678 variable stars. Among the newly designated objects were V0654 Aurigae, V1367 Centauri, and BU Coronae Borealis. Most of this system was invented
Variable-star_designation
Ohnaka, Keiichi; Griffin, Elizabeth (2022). "HST STIS Observations of ζ Aurigae A's Irradiated Atmosphere". The Astronomical Journal. 164 (1): 16. Bibcode:2022AJ
List_of_nearest_supergiants
Binary star in the constellation Dorado
features. Antares, formerly considered the largest known star Epsilon Aurigae, another eclipsing binary star containing a yellow supergiant primary and
WOH_G64
Stars with a supergiant luminosity class with a spectral type of K or M
Epsilon Pegasi Zeta Cephei Lambda Velorum Eta Persei 31 and 32 Cygni Psi1 Aurigae 119 Tauri Mira was historically thought to be a red supergiant star, but
Red_supergiant
Star in the constellation Ursa Major
(2019). "Magnetic field topologies of the bright, weak-field Ap stars θ Aurigae and ∊ Ursae Majoris". Astronomy and Astrophysics. 621: A47. arXiv:1811
Alioth
at zspec = 14.44 Confirmed with JWST". The Open Journal of Astrophysics. 9. arXiv:2505.11263v2. Bibcode:2026OJAp....956033N. doi:10.33232/001c.156033
List of the most distant astronomical objects
List_of_the_most_distant_astronomical_objects
Star in the constellation Columba
proper motion and radial velocity, astronomers know that this star and AE Aurigae are moving away from each other at a relative velocity of over 200 km/s
Mu_Columbae
members include Alpha Coronae Borealis (α CrB or Alphecca or Gemma), Beta Aurigae (β Aur), Delta Aquarii (δ Aqr), Gamma Leporis (γ Lep) and Beta Serpentis
Ursa_Major_moving_group
Polish writer and artist (1885–1939)
Arts, Szépművészeti, Budapest Bronisława Wieniawa-Długoszowska 1918 Nova Aurigae 1918, Adam Mickiewicz Museum of Literature, Warsaw Composition 1922, National
Stanisław_Ignacy_Witkiewicz
German astronomer
scientific papers. In 1931–32, he and Heribert Schneller discovered that Zeta Aurigae is an eclipsing binary. The minor planet 1985 Hopmann is named after him
Josef_Hopmann
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9 AURIGAE
9 AURIGAE
9 AURIGAE
9 AURIGAE
9 AURIGAE
9 AURIGAE
9 AURIGAE
9 AURIGAE
9 AURIGAE
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