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  2. Capella - Wikipedia

    en.wikipedia.org/wiki/Capella

    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. Category:Auriga - Wikipedia

    en.wikipedia.org/wiki/Category:Auriga

    Constellation map: Pages in category "Auriga" The following 155 pages are in this category, out of 155 total. This list may not reflect recent changes. ...

  4. Theta Aurigae - Wikipedia

    en.wikipedia.org/wiki/Theta_Aurigae

    Theta Aurigae (Latinized from θ Aurigae, abbreviated Theta Aur, θ Aur) is a binary star in the constellation of Auriga. Based upon parallax measurements, the distance to this system is about 166 light-years (51 parsecs). [1] The two components are designated Theta Aurigae A (also named Mahasim [10]) and B.

  5. 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 ...

  6. Omega Aurigae - Wikipedia

    en.wikipedia.org/wiki/Omega_Aurigae

    Omega Aurigae, Latinized from ω Aurigae, is the Bayer designation for a double star [11] in the northern constellation of Auriga. Its apparent magnitude is 4.95, [2] which is bright enough to be seen with the naked eye. The distance to this system, as determined using parallax measurements, is approximately 162 light-years (50 parsecs). [1]

  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. AE Aurigae - Wikipedia

    en.wikipedia.org/wiki/AE_Aurigae

    Hipparcos light curves for AE Aurigae. The main plot shows the long-term variation, and the inset plot shows the variation folded over a period of 213.7 days. Adapted from Marchenko et al. (1998) [8]

  9. 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.