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作 者:Valentina M.Chepurova Nelli V.Kulikova Elena N.Petrovskaya
机构地区:[1]Sternberg Astronomical Institute, Lomonosov Moscow State University [2]Department of Computer Systems, Networks and Technologies, National Research Nuclear University, Moscow Engineering Physics Institute, Institute for Nuclear Power Engineering
出 处:《Research in Astronomy and Astrophysics》2016年第4期1-6,共6页天文和天体物理学研究(英文版)
摘 要:We present simulation results on evolution development of orbital motion of short-period comets with the revolution period not exceeding 6-7 years, namely comets 21P/Giacobini-Zinner, 26P/Grigg- Skjellerup and 7P/Pons-Winnecke. The calculations cover the range from the date of the object's discovery to 2100. Variations in the objects' orbital elements under the action of gravity disturbances, taking Earth's gravitational potential into account when the small body approaches, are analyzed. Corrected dates of peri- helion passages can be used for scheduling observations.We present simulation results on evolution development of orbital motion of short-period comets with the revolution period not exceeding 6-7 years, namely comets 21P/Giacobini-Zinner, 26P/Grigg- Skjellerup and 7P/Pons-Winnecke. The calculations cover the range from the date of the object's discovery to 2100. Variations in the objects' orbital elements under the action of gravity disturbances, taking Earth's gravitational potential into account when the small body approaches, are analyzed. Corrected dates of peri- helion passages can be used for scheduling observations.
关 键 词:comets: individual (21P/Giacobini-Zinner 26P/Grigg-Skjellerup 7P/Pons-Winnecke)-- me-teorites METEORS METEOROIDS
分 类 号:P185.81[天文地球—天文学] V412.41[航空宇航科学与技术—航空宇航推进理论与工程]
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