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Capella was the brightest star in the night sky from 210,000 years ago to 160,000 years ago, at about −1.8 in apparent magnitude. At −1.1, Aldebaran was brightest before this period; it and Capella were situated rather close to each other in the sky and approximated boreal pole stars at the time. [35] Building J (foreground) at Monte Albán
AR Aurigae (AR Aur), also known by its Flamsteed designation 17 Aurigae, is a binary star in the constellation Auriga. Based on parallax measurements made by the Hipparcos spacecraft, it is approximately 461 light-years from Earth. [10] Both components are blue-white B-type main-sequence stars that do not fill their Roche lobes.
Category: Auriga. 50 languages. ... Constellation map Pages in category "Auriga" The following 155 pages are in this category, out of 155 total. ... 1 Aurigae; 2 ...
59 Aurigae, often abbreviated as 59 Aur, is a star in the constellation Auriga. Its baseline apparent magnitude is 6.1, [3] meaning it can just barely be seen with the naked eye as a dim, yellow-white hued star. Based on parallax measurements, it is located about 483 light-years (148 parsecs) away from the Sun. [2]
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 .
AE Aurigae (abbreviated as AE Aur) is a runaway star in the constellation Auriga; it lights the Flaming Star Nebula. Description. Hipparcos light curves for AE ...
Iota Aurigae (ι Aurigae, abbreviated Iota Aur, ι Aur), officially named Hassaleh / ˈ h æ s ə l eɪ /, [12] is a star in the northern constellation of Auriga.It has an apparent visual magnitude of 2.7, [2] which is bright enough to be readily visible to the naked eye.
64 Aurigae is a single [7] star located 312 [1] light years away from the Sun in the northern constellation of Auriga. [6] It is visible to the naked eye as a dim, white-hued star with an apparent magnitude of 5.87. [2]