Stable and unstable orbits around Mercury

Stable and unstable orbits around Mercury
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DOI:
10.1007/s10569-010-9309-z
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发表时间:
2010-10
影响因子:
1.6
通讯作者:
Z. Makó;Ferenc Szenkovits;J. Salamon;Róbert Oláh-Gál
Z. Makó;Ferenc Szenkovits;J. Salamon;Róbert Oláh-Gál
中科院分区:
物理与天体物理3区
文献类型:
--
作者:
Z. Makó;Ferenc Szenkovits;J. Salamon;Róbert Oláh-Gál

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本文在空间椭圆型限制性三体问题的框架下,研究了小质点周围的稳定和不稳定区域。用于确定稳定和不稳定区域的定义和方法被扩展到三维。在太阳-水星系统中获得了有关水星周围稳定区和不稳定区的新结果。
This paper provides a study of the stable and unstable regions around the smaller primary in the framework of the spatial elliptic restricted three-body problem. The definitions and methods used to determine stable and unstable regions are extended to three dimensions. New results concerning the stable and unstable regions around Mercury are obtained in the Sun–Mercury system.