The origin and rotation of binary asteroids

Binary asteroids were detected in a variety of dynamical populations, including Near-Earth Asteroids (NEAs), the main belt (MB), Trojans, and transneptunian objects (TNO). We discuss a new “multi-impact” model for origin of all classes of binary objects, including binary asteroids, Pluto–Charon, and...

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Veröffentlicht in:Кинематика и физика небесных тел
Datum:2005
Hauptverfasser: Gaftonyuk, N., Gorkavyi, N.
Format: Artikel
Sprache:English
Veröffentlicht: Головна астрономічна обсерваторія НАН України 2005
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Online Zugang:https://nasplib.isofts.kiev.ua/handle/123456789/79704
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Назва журналу:Digital Library of Periodicals of National Academy of Sciences of Ukraine
Zitieren:The origin and rotation of binary asteroids / N. Gaftonyuk, N. Gorkavyi // Кинематика и физика небесных тел. — 2005. — Т. 21, № 5-додаток. — С. 483-486. — Бібліогр.: 15 назв. — англ.

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