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3065 Sarahill: Asteroid Family, Solar System, Trojan (Astronomy), Near-Earth Object - Couverture souple
Synopsis
Please note that the content of this book primarily consists of articles available from Wikipedia or other free sources online. 3065 Sarahill (1984 CV) is a main-belt asteroid discovered on February 8, 1984 by E. Bowell at Flagstaff (AM). Asteroids (from Greek ¿¿¿¿¿ 'star' and ¿¿¿¿¿ 'like, in form') are a class of Small Solar System Bodies in orbit around the Sun. They have also been called planetoids, especially the larger ones. These terms have historically been applied to any astronomical object orbiting the Sun that did not show the disk of a planet and was not observed to have the characteristics of an active comet, but as small objects in the outer Solar System were discovered, their volatile-based surfaces were found to more closely resemble comets, and so were often distinguished from traditional asteroids.
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3065 SARAHILL
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3065 Sarahill
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Taschenbuch. Etat : Neu. This item is printed on demand - Print on Demand Titel. Neuware OmniScriptum SRL, Str. Armeneasca 28/1, office 1, 2012 Chisinau 108 pp. Englisch. N° de réf. du vendeur 9786138519980
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3065 Sarahill : Asteroid Family, Solar System, Trojan (Astronomy), Near-Earth Object
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Taschenbuch. Etat : Neu. nach der Bestellung gedruckt Neuware - Printed after ordering - Please note that the content of this book primarily consists of articles available from Wikipedia or other free sources online. 3065 Sarahill (1984 CV) is a main-belt asteroid discovered on February 8, 1984 by E. Bowell at Flagstaff (AM). Asteroids (from Greek ¿¿¿¿¿ 'star' and ¿¿¿¿¿ 'like, in form') are a class of Small Solar System Bodies in orbit around the Sun. They have also been called planetoids, especially the larger ones. These terms have historically been applied to any astronomical object orbiting the Sun that did not show the disk of a planet and was not observed to have the characteristics of an active comet, but as small objects in the outer Solar System were discovered, their volatile-based surfaces were found to more closely resemble comets, and so were often distinguished from traditional asteroids. N° de réf. du vendeur 9786138519980
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