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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
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
Constellation in the northern celestial hemisphere
Aurigae. SIMBAD Kappa Aurigae. SIMBAD Pi Aurigae. SIMBAD Tau Aurigae. SIMBAD Upsilon Aurigae. SIMBAD Chi Aurigae. SIMBAD 2 Aurigae. SIMBAD Mu Aurigae
Auriga
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
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
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
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
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
NO Aurigae is a pulsating variable star in the constellation Auriga. It is an unusually luminous asymptotic giant branch star about 3,500 light-years
NO_Aurigae
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 Auriga
Psi5 Aurigae is a star in the northern constellation of Auriga. Its name is a Bayer designation that is Latinized from ψ5 Aurigae, and abbreviated Psi5
Psi5_Aurigae
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
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
Emission and reflection nebula in the constellation Auriga
celestial equator, surrounding the bluish, irregular variable star AE Aurigae. It shines at magnitude +6.0. Its celestial coordinates are RA 05h 16.2m
IC_405
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
Principal meridians of the celestial sphere
HarperCollins. p. 98. ISBN 978-006095368-3. OCLC 50409366. Kaler, Jim. "Pi Aurigae." Pi Aurigae. N.p. 22 Feb. 2008. Web. Portals: Astronomy Stars Spaceflight Outer
Colure
Star in the constellation Lynx
constellation border with Auriga, and is also known as Psi10 Aurigae, which is Latinized from ψ10 Aurigae. The star has a white hue and is visible to the naked
16_Lyncis
Star in the constellation Auriga
PU Aurigae is an irregular variable star located in the constellation Auriga. A red giant, it varies by 0.1 magnitude around magnitude 5.64, so it is
PU_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
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
RT Aurigae (RT Aur, 48 Aurigae) is a yellow supergiant variable star in the constellation Auriga, about 1,500 light years from Earth. Although its brightness
RT_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
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
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
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
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
Arabic: الكاس alkās or Arabic: الكأس alka's ('the cup') /ˈælkɛs/ Almaaz ε Aurigae Aa Auriga Arabic /ˈælmeɪ.əz/ Almach γ Andromedae A Andromeda Arabic Derived
List_of_proper_names_of_stars
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
Star in the constellation Auriga
6 Aurigae is a star in the constellation Auriga. Its apparent magnitude is 6.48, making it just visible to the naked eye in optimal conditions (HR 1602)
6_Aurigae
Former constellation
the planet Uranus. It fell out of use by the end of the 19th century. ψ2 Aurigae at apparent magnitude 4.79 was the constellation's brightest star. It was
Telescopium_Herschelii
Star in the constellation Auriga
42 Aurigae is a star in the northern constellation of Auriga. The designation is from the star catalogue of English astronomer John Flamsteed, first published
42_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
Stellar classification distinguished by bright blue luminosity
Omega Scorpii (B1 V), 42 Orionis (B1 V), 22 Scorpii (B3 V), Rho Aurigae (B5 V), and 18 Tauri (B8 V). The Revised MK Spectra Atlas of Morgan, Abt, & Tapscott
B-type_main-sequence_star
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
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
Star in the constellation Auriga
Upsilon Aurigae is a single star in the northern constellation of Auriga. Its name is a Bayer designation that is Latinised from υ Aurigae, and abbreviated
Upsilon_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
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
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
07var) Vega α Lyrae 0025 A0Va Northern 6 0.08 (0.03–0.16var) Capella α Aurigae 0043 K0 III, G1 III Northern 7 0.13 (0.05–0.18var) Rigel β Orionis 0860
List_of_brightest_stars
Star in the constellation Gemini
cannot be observed with the naked eye. The closest star to Gliese 251 is QY Aurigae, which is located 3.5 light years away. Gliese 251 is a red dwarf with
Gliese_251
Star naming system
both constellations: Alpha Andromedae = Delta Pegasi, Beta Tauri = Gamma Aurigae, and Nu Boötis = Psi Herculis. (He catalogued Fomalhaut only once, as Alpha
Bayer_designation
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
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
Star in the constellation Auriga
12 Aurigae is a Be star in the northern constellation Auriga. It lies below the normal limit for visibility to the naked eye, having an apparent visual
12_Aurigae
Red supergiant star in the constellation Orion
supernovae, and there is strong evidence that OB stars μ Columbae, AE Aurigae, and 53 Arietis all originated from such explosions in Ori OB1 2.2, 2.7
Betelgeuse
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
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
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
Part of Latin grammar
poēta, poētae m. ('poet'), agricola, agricolae m. ('farmer'), auriga, aurigae m. ('auriga, charioteer'), pīrāta, pīrātae m. ('pirate') and nauta, nautae
Latin_declension
Binary star system in the constellation Auriga
Gliese 268 (QY Aurigae) is a binary star system in the constellation of Auriga, and is one of the one hundred closest star systems to the Earth, at a
Gliese_268
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
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
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
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
J.; Turner, N.; Pedretti, E.; Thureau, N. (2015). "Interferometry of ɛ Aurigae: Characterization of the Asymmetric Eclipsing Disk". The Astrophysical
List of stars with resolved images
List_of_stars_with_resolved_images
Mystery religion in the Roman Empire
from the Papyri. Nova Roma. 11 March 2009. Archived from the original on 18 May 2013. Retrieved 7 September 2013. Janson, Horst Woldemar; Janson, Anthony
Mithraism
Star in the constellation Auriga
Omega Aurigae is a double star in the northern constellation of Auriga. Its name is a Bayer designation that is Latinized from ω Aurigae, and abbreviated
Omega_Aurigae
applications". The Astronomy & Astrophysics Review. 18 (1–2): 67–126. arXiv:0908.2624. Bibcode:2010A&ARv..18...67T. doi:10.1007/s00159-009-0025-1. S2CID 14006009
List_of_nearest_stars
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)
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
Star in the constellation Auriga
59 Aurigae, often abbreviated as 59 Aur, is a star in the constellation Auriga. Its baseline apparent magnitude is 6.1, meaning it can just barely be
59_Aurigae
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
G-type giant star in the constellation Auriga
Kappa Aurigae is a star in the northern constellation of Auriga. Its name is a Bayer designation that is Latinised from κ Aurigae, and is abbreviated
Kappa_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
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
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
Study of the movement of stars
process. An example of a related set of runaway stars is the case of AE Aurigae, 53 Arietis and Mu Columbae, all of which are moving away from each other
Stellar_kinematics
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
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
universe came into existence about 13.66 billion years ago Cooper, Keith (18 April 2023). "JWST spectrometer refines redshifts of distant galaxies". Physics
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
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
Accumulation of matter around a star
Beta Pictoris or AU Microscopii) and face-on disks (e.g. IM Lupi or AB Aurigae) require a coronagraph, adaptive optics or differential images to take
Circumstellar_disc
star system 3.18 Eta Aurigae (Haedus) Star 3.18 Epsilon Leporis (Ping) Star 3.18 Theta Ursae Majoris Star Suspected variable star 3.18 Pi Herculis (Nüchuang)
List of brightest natural objects in the sky
List_of_brightest_natural_objects_in_the_sky
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
Organization of amateur and professional astronomers
collaboration project examining the 2009-2011 eclipse of the star epsilon Aurigae. The AAVSO headquarters was originally located at the residence of its
American Association of Variable Star Observers
American_Association_of_Variable_Star_Observers
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
"SIMBAD Astronomical Database". Strasbourg astronomical Data Center. Retrieved 18 August 2015. "HD 55". SIMBAD. Retrieved 1 March 2025. "HD 38A". SIMBAD. Retrieved
List of Gliese and GJ objects (1-1000)
List_of_Gliese_and_GJ_objects_(1-1000)
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
Binary star in the constellation Cepheus
the exact onset is difficult to measure because it is gradual. Only ε Aurigae (period = 27.08 years), and AS Leonis Minoris (period = 69.1 years) have
VV_Cephei
American astronomer (1882–1967)
published as “The Orbits of the Cepheid Variables Y Sagittarii and RT Aurigae; with a Discussion of the Possible Causes of This Type of Stellar Variation
John_Charles_Duncan
Stellar classification
Main-sequence 9 Sagittarii 10 Lacertae AE Aurigae BI 253 Delta Circini HD 93205 (V560 Carinae) Mu Columbae Sigma Orionis Theta1 Orionis C VFTS 102 Zeta
O-type_star
K-type giant star in the constellation Auriga
38 Aurigae is a star located 236 light years away from the Sun in the northern constellation of Auriga. It is visible to the naked eye as a dim, orange-hued
38_Aurigae
previously been recorded of having a parallax of 127 mas. Capella (Alpha Aurigae) Solitary star 1849− 72 ly (46 mas) Polaris (Alpha Ursae Minoris) Variable
List_of_most_distant_stars
American astronomer, writer, and skeptic (born 1964)
presentation of high-resolution images of isolated stellar objects (including AB Aurigae and HD 163296) from the Hubble Space Telescope, among the first of those
Phil_Plait
Star in the constellation Perseus
Schroder, K. P.; Misch, A.; Griffin, R. F. (1992). "Optical Spectra of Zeta-Aurigae Binary Systems - Part Three - the 1989 Eclipse of Tau-Persei". Astronomy
Tau_Persei
Daniel J.; Shappee, Benjamin J. (May 2016). "An extreme analogue of ε Aurigae: an M-giant eclipsed every 69 years by a large opaque disk surrounding
List_of_nearest_hypergiants
3 2 O9.5V 4.07 Meissa A (Lambda Orionis) 1260±200 1 O8 III((f)) 3.7 AE Aurigae 1,320 ± 40 1 O9.5V 5.96 Xi Persei (Menkib) 1,340±65 1 O7.5III(n)((f)) 4
List_of_O-type_stars
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
Star that is particularly similar to the Sun
1051/0004-6361:200809698. S2CID 18173201. See VizieR catalogue J/A+A/487/373. V538 Aurigae at SIMBAD - Ids - Bibliography - Image. HD 14412 at SIMBAD - Ids - Bibliography
Solar_analog
Quasar in the constellation Auriga
constellation Auriga not far in the sky from the 5th magnitude star Omicron Aurigae. The "distance" of a far away galaxy depends on the distance measurement
3C_147
Benjamin J.; Kochanek, Christopher S. (April 2016). "AN EXTREME ANALOGUE OF ϵ AURIGAE: AN M-GIANT ECLIPSED EVERY 69 YEARS BY A LARGE OPAQUE DISK SURROUNDING
List_of_smallest_known_stars
Constellation in the northern celestial hemisphere
light-years distant from Earth. Likewise 16 Lyncis was originally known as Psi10 Aurigae and conversely, 37, 39, 41 and 44 Lyncis became part of Ursa Major. Y Lyncis
Lynx_(constellation)
starting at 0° at the left of the chart, and increasing counter-clockwise. The 18 southern stars are those with a declination between 30° south and 90° south
List_of_stars_for_navigation
Star whose brightness fluctuates, as seen from Earth
Herbig Ae/Be stars, are the more massive form. The fourth are the RW Aurigae irregular variables that have similar properties but lack nearby nebulosity
Variable_star
System of two stars orbiting each other
mass that is 98% of the Sun. An example of an eclipsing binary is Epsilon Aurigae in the constellation Auriga. The visible component belongs to the spectral
Binary_star
source of the Flaming Star Nebula IC 405 (aka Cederblad 42) in Auriga, AE Aurigae. Named after John Martin Schaeberle. Scheiner's Star is BD +15°2083 (HD
Stars_named_after_people
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
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18 AURIGAE
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