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This image is a derivative work of the following images: File:Auriga_constellation_map.png licensed with Cc-by-sa-3.0-migrated, GFDL 2004-12-12T17:53:02Z Alfio 2559x2559 (280768 Bytes) Auriga constellation map (bigger image) 2004-12-12T12:12:04Z Alfio 427x427 (28366 Bytes) Auriga constellation map; Uploaded with derivativeFX
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 open clusters M36 and M37, also discovered by Hodierna, are often grouped together with M38. [5]
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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]
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.
LY Aurigae is a multiple star system in the constellation Auriga. It is an eclipsing binary variable star , dropping in brightness by 0.7 magnitudes every 4 days. The system is around a thousand light years away in the Auriga OB1 stellar association .
Messier 37 (also known as M37, NGC 2099, or the Salt and Pepper Cluster) is the brightest and richest open cluster in the constellation Auriga. It was discovered by the Italian astronomer Giovanni Battista Hodierna before 1654. M37 was missed by French astronomer Guillaume Le Gentil when he rediscovered M36 and M38 in 1749.
65 Aurigae is a binary star [7] system located 252 light years away from the Sun in the northern constellation of Auriga. It is visible to the naked eye as a faint, orange hued star with an apparent visual magnitude of 5.12. [2] The primary, designated component A, is an aging giant star with a stellar classification of K0 III. [3]
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