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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 .
The story takes the form of a one-sided correspondence between Skander, an alien, to an unnamed human (whose replies are not presented.) In his initial letter, Skander spends some time describing himself and his home planet in the constellation Auriga, whose intelligent lifeforms are long-lived, highly radioactive, and chromium-based, thriving at a temperature of around 900 degrees Kelvin.
Download as PDF; Printable version; ... Constellation map ... Pages in category "Auriga" The following 155 pages are in this category, out of 155 total. ...
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.
Nu Aurigae, Latinised from ν Aurigae, is the Bayer designation for a star in the northern constellation of Auriga. It is visible to the naked eye with an apparent visual magnitude of 3.96 [2] and is approximately 200 light-years (61 parsecs) distant from the Earth. [1] This is an evolved giant star with a stellar classification of G9.5 III. [9]
Download as PDF; Printable version; In other projects ... This is the list of notable stars in the constellation Auriga, sorted by decreasing brightness. Name B F Var ...
Download as PDF; Printable version; In other projects Wikimedia Commons; Wikidata item; Appearance. ... Constellation: Auriga: Right ascension: 05 h 16 m 18.15000 s ...
R Aurigae (R Aur) is a Mira variable, a pulsating red giant star in the constellation of Auriga, at a distance of 930 light years. In 1862 R Aurigae was found to be a variable star at Bonn Observatory. [9] It was widely observed in the late 19th century and its spectrum was described in 1890. [10]