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Epsilon Aurigae (ε Aurigae, abbreviated Epsilon Aur, ε Aur) is a multiple star system in the northern constellation of Auriga, the charioteer.It is an unusual eclipsing binary system comprising an F0 supergiant (officially named Almaaz / æ l ˈ m ɑː z /, the traditional name for the system) and a companion which is generally accepted to be a huge dark disk orbiting an unknown object ...
Capella is the brightest star in the northern 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 star in the night sky , and the third-brightest in the northern celestial hemisphere after Arcturus and Vega .
3 Aur Other objects; Common name ... M 36: NGC 1960 M 37: NGC 2099 M 38: NGC 1912 Constellation map: Pages in category "Auriga" The following 155 pages are in this ...
This is the list of notable stars in the constellation Auriga, sorted by decreasing brightness. Name B F Var HD HIP RA Dec vis. mag. abs. ... V min = 1.98 m, P = 3. ...
9 Aurigae (9 Aur) is a star system in Auriga (constellation).It has an apparent magnitude of about 5, making it visible to the naked eye in many suburban skies. [15] Parallax estimates made by the Hipparcos spacecraft put it at about 86 light-years (26 parsecs) from the solar system, [1] although individual Gaia Data Release 3 parallaxes place all three components at 88 light years.
In Indian astronomy, it is known by the name Prajapati / p r ə ˈ dʒ ɑː p ə t i /, from the Sanskrit प्रजापति prajāpati "the Lord of Created Beings". [15] [16]In Chinese, 八穀 (Bā Gǔ), meaning Eight Kinds of Crops, refers to an asterism consisting of δ Aurigae, ξ Aurigae, 26 Camelopardalis, 14 Camelopardalis, 7 Camelopardalis, 9 Aurigae, 11 Camelopardalis and 31 ...
AB Aurigae is a young Herbig Ae star [3] in the Auriga constellation. It is located at a distance of approximately 509 light years from the Sun based on stellar parallax. [1] This pre-main-sequence star has a stellar classification of A0Ve, [4] matching an A-type main-sequence star with emission lines in the spectrum.
The secondary, Theta Aurigae B, is a +7.2 magnitude companion, 4.5 [3] magnitudes fainter than the primary, located at an angular separation of 3.91 arcseconds along a position angle of 304.9° as of 2002. [18] This is an F-type main sequence star with a stellar classification in the range F2-5 V. [3]