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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 .
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.
AURIGA (Antenna Ultracriogenica Risonante per l'Indagine Gravitazionale Astronomica) is an ultracryogenic resonant bar gravitational wave detector in Italy. [1] It is at the Laboratori Nazionali di Legnaro of the Istituto Nazionale di Fisica Nucleare , near Padova . [ 2 ]
Constellation map: Pages in category "Auriga" The following 155 pages are in this category, out of 155 total. ... List of stars in Auriga; 0–9. 1 Aurigae; 2 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 ...
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.
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.
Lambda Aurigae, Latinized from λ Aurigae, is the Bayer designation for a solar analog [9] star in the northern constellation of Auriga. [13] It is visible to the naked eye with an apparent visual magnitude of 4.71. [2] Based upon parallax measurements, it is approximately 40.7 light-years (12.5 parsecs) distant from the Earth. [14]