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Capella Aa has a projected rotational velocity of 4.1 ± 0.4 km per second, taking 104 ± 3 days to complete one rotation, while Capella Ab spins much more rapidly at 35.0 ± 0.5 km per second, completing a full rotation in only 8.5 ± 0.2 days.
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 .
Zeta Aurigae, or ζ Aurigae, is a binary star system in the northern constellation of Auriga.Based upon parallax measurements, this system is approximately 860 light-years (260 parsecs) distant from the Sun. [6]
Messier 38 or M38, also known as NGC 1912 or Starfish Cluster, [4] is an open cluster of stars in the constellation of Auriga.It was discovered by Giovanni Batista Hodierna before 1654 and independently found by Le Gentil in 1749.
The Perseus Family includes several constellations associated with the Perseus myth: Cassiopeia, Cepheus, Andromeda, Perseus, Pegasus, and Cetus (representing the monster sent to devour Andromeda). Menzel also included a few neighboring constellations: Auriga, Lacerta, and Triangulum. Except for Cetus, these constellations all lie north of the ...
This is the list of notable stars in the constellation Auriga, sorted by decreasing brightness. Name B F Var HD HIP ... +37° 18′ 20.5″ 4.72: −1.10: 475: M1III ...
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