Resonant Orbital Dynamics in LEO Region: Space Debris in Focus

被引:12
作者
Sampaio, J. C. [1 ]
Wnuk, E. [2 ]
Vilhena de Moraes, R. [1 ]
Fernandes, S. S. [3 ]
机构
[1] Univ Fed Sao Paulo UNIFESP, BR-12231280 Sao Jose Dos Campos, SP, Brazil
[2] Astron Observ, AMU, PL-60286 Poznan, Poland
[3] ITA, BR-12228900 Sao Jose Dos Campos, SP, Brazil
基金
巴西圣保罗研究基金会;
关键词
2; PLANETS; MOTION; SYSTEM;
D O I
10.1155/2014/929810
中图分类号
T [工业技术];
学科分类号
08 ;
摘要
The increasing number of objects orbiting the earth justifies the great attention and interest in the observation, spacecraft protection, and collision avoidance. These studies involve different disturbances and resonances in the orbital motions of these objects distributed by the distinct altitudes. In this work, objects in resonant orbital motions are studied in low earth orbits. Using the two-line elements (TLE) of the NORAD, resonant angles and resonant periods associated with real motions are described, providing more accurate information to develop an analytical model that describes a certain resonance. The time behaviors of the semimajor axis, eccentricity, and inclination of some space debris are studied. Possible irregular motions are observed by the frequency analysis and by the presence of different resonant angles describing the orbital dynamics of these objects.
引用
收藏
页数:12
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