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1804 Chebotarev : ウィキペディア英語版 | 1804 Chebotarev
1804 Chebotarev, provisional designation 1967 GG, is a bright asteroid dwelling in the inner regions of the main-belt. It was discovered on 6 April 1967 by Russian female astronomer Tamara Smirnova at the Crimean Astrophysical Observatory in Nauchnyj.〔 The stony S-type asteroid measures about 10 kilometers in diameter. It orbits the Sun at a distance of 2.4–2.5 AU once every 3 years and 9 months (1,368 days). A preliminary analysis by the WISE/NEOWISE missions published an exceptionally high, yet very uncertain albedo of , while the LCDB project assumes a much lower value of 0.20.〔〔 The body rotates around its axis every 4.03 hours.〔 It was named in honor of G. A. Chebotarev (1913–1975), who was a professor and the director of the ''Institute of Theoretical Astronomy'' as well as president of IAU's Commission 20 ''(Positions & Motions of Minor Planets, Comets & Satellites)''. He is known for his work on celestial mechanics of asteroids, comets and satellites.〔 == References ==
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