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摘要:
There are plentiful asteroids moving periodically around their central primaries,such as the Sun.Due to the perturbation of the central primary,the gravitational force of the perturbed asteroid system varies periodically.In this paper,based on the idea of integrating the solar gravitational force as a part of the system instead of treating it as perturbation,the parametric resonance response is investigated.A novel type of stable parametric resonance orbits has been detected.It is found that the steady-state motion amplitude of parametric resonance orbit is determined by the frequency-response equation.The stability of the novel orbits has also been demonstrated.The new type of orbits may contribute to possible asteroid exploration missions.
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篇名 Parametric resonance orbit analysis for irregular shaped asteroids based on the perturbed particle-linkage model
来源期刊 天文和天体物理学研究 学科
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年,卷(期) 2020,(12) 所属期刊栏目 Research Papers
研究方向 页码范围 15-30
页数 16页 分类号
字数 语种 英文
DOI 10.1088/1674-4527/20/12/193
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天文和天体物理学研究
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1674-4527
11-5721/P
北京朝阳区大屯路甲20号国家天文台 RAA编辑部
eng
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