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Later, Bedouin astronomers created constellations that were groups of animals, where each star represented one animal. The stars of Auriga comprised a herd of goats, an association also present in Greek mythology. [37] It is sometimes called the Shepherd's Star in English literature. [38] Capella was seen as a portent of rain in classical times ...
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.
Constellation: Auriga: Right ascension: 6 h 4 m -0 s: Declination +39° 00′ 00″ Properties; Occurs during: August 26 to September 5: Date of peak: September 1 [1] Velocity: 65 [1] km/s: Zenithal hourly rate: 6: See also: List of meteor showers
In Indian astronomy, it is known by the name Prajapati / p r ə ˈ dʒ ɑː p ə t i /, from the Sanskrit प्रजापति prajāpati "the Lord of Created Beings". [15] [16]In Chinese, 八穀 (Bā Gǔ), meaning Eight Kinds of Crops, refers to an asterism consisting of δ Aurigae, ξ Aurigae, 26 Camelopardalis, 14 Camelopardalis, 7 Camelopardalis, 9 Aurigae, 11 Camelopardalis and 31 ...
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]
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.
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 ...
The 25–26 January 1938 geomagnetic storm (also titled the Fátima Storm) was a massive solar storm which occurred 16–26 January with peak activity on 22, 25, and 26 January and was part of the 17th solar cycle. As the electrification of Europe and North America was still in its infancy, the light storm could be seen brilliantly.