Analysis of the potential field and equilibrium points of irregular-shaped minor celestial bodies
Analysis of the potential field and equilibrium points of irregular-shaped minor celestial bodies
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不规则形状小天体的势场和平衡点分析
DOI:
10.1007/s10509-014-2022-8
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发表时间:
2014-03
影响因子:
1.9
通讯作者:
Gong Shengping
中科院分区:
文献类型:
--
作者:
Wang Xianyu;Jiang Yu;Gong Shengping
The equilibrium points of the gravitational potential field of minor celestial bodies, including asteroids, comets, and irregular satellites of planets, are studied. In order to understand better the orbital dynamics of massless particles moving near celestial minor bodies and their internal structure, both internal and external equilibrium points of the potential field of the body are analyzed. In this paper, the location and stability of the equilibrium points of 23 minor celestial bodies are presented. In addition, the contour plots of the gravitational effective potential of these minor bodies are used to point out the differences between them. Furthermore, stability and topological classifications of equilibrium points are discussed, which clearly illustrate the topological structure near the equilibrium points and help to have an insight into the orbital dynamics around the irregular-shaped minor celestial bodies. The results obtained here show that there is at least one equilibrium point in the potential field of a minor celestial body, and the number of equilibrium points could be one, five, seven, and nine, which are all odd integers. It is found that for some irregular-shaped celestial bodies, there are more than four equilibrium points outside the bodies while for some others there are no external equilibrium points. If a celestial body has one equilibrium point inside the body, this one is more likely linearly stable.
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影响因子:
3.2
作者:
S. Ostro;R. Jurgens;K. Rosema;R. Hudson;J. Giorgini;R. Winkler;D. Yeomans;D. Choate;R. Rose;M. Slade;S. Howard;D. Scheeres;D. Mitchell
通讯作者:
S. Ostro;R. Jurgens;K. Rosema;R. Hudson;J. Giorgini;R. Winkler;D. Yeomans;D. Choate;R. Rose;M. Slade;S. Howard;D. Scheeres;D. Mitchell
影响因子:
3.2
作者:
P. Thomas;J. Burns;L. Rossier;D. Simonelli;J. Veverka;C. Chapman;K. Klaasen;T. Johnson;M. Belton
通讯作者:
P. Thomas;J. Burns;L. Rossier;D. Simonelli;J. Veverka;C. Chapman;K. Klaasen;T. Johnson;M. Belton
DOI:
10.2514/6.2010-8373
发表时间:
2010-08
期刊:
--
影响因子:
--
作者:
J. Mondelo;S. Broschart;B. Villac
通讯作者:
J. Mondelo;S. Broschart;B. Villac
影响因子:
3.2
作者:
D. Scheeres;S. Ostro;R. Hudson;R. A. Werner
通讯作者:
D. Scheeres;S. Ostro;R. Hudson;R. A. Werner
影响因子:
56.9
作者:
M. A’Hearn;M. Belton;W. Delamere;J. Kissel;K. Klaasen;Lucy A. McFadden;K. Meech;H. Melosh;
通讯作者:
M. A’Hearn;M. Belton;W. Delamere;J. Kissel;K. Klaasen;Lucy A. McFadden;K. Meech;H. Melosh;