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Capella Aa is the cooler and more luminous of the two with spectral class K0III; it is 78.7 ± 4.2 times the Sun's luminosity and 11.98 ± 0.57 times its radius. An aging red clump star, it is fusing helium to carbon and oxygen in its core.
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 ...
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.
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 ...
Eta Aurigae is larger than the Sun, with more than five times the Sun's mass and over three times its radius. [6] The spectrum of this star matches a stellar classification of B3 V, [ 3 ] which is a B-type main-sequence star that is generating its energy through the nuclear fusion of hydrogen at its core.
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 .
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 ...
R Aurigae has an apparent visual magnitude which varies between 6.7 and 13.9 with a period of 450 days. [3] The light curve varies strongly from cycle to cycle, sometimes having a pronounced hump on the ascending branch and usually having rise and fall times approximately equal. The cycle period has oscillated slowly between about 450 and 465 days.