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  2. Capella - Wikipedia

    en.wikipedia.org/wiki/Capella

    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.

  3. Epsilon Aurigae - Wikipedia

    en.wikipedia.org/wiki/Epsilon_Aurigae

    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 ...

  4. 9 Aurigae - Wikipedia

    en.wikipedia.org/wiki/9_Aurigae

    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.

  5. Category:Auriga - Wikipedia

    en.wikipedia.org/wiki/Category:Auriga

    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 ...

  6. Eta Aurigae - Wikipedia

    en.wikipedia.org/wiki/Eta_Aurigae

    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.

  7. AB Aurigae - Wikipedia

    en.wikipedia.org/wiki/AB_Aurigae

    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 .

  8. Delta Aurigae - Wikipedia

    en.wikipedia.org/wiki/Delta_Aurigae

    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 ...

  9. R Aurigae - Wikipedia

    en.wikipedia.org/wiki/R_Aurigae

    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.