Periodic orbit search method for double asteroid system based on velocity Poincaré section
A Poincaré cross-section, double asteroid technology, applied in the aerospace field, can solve problems such as periodic orbit search limitations, and achieve the effects of simple calculation, high efficiency, and improved search efficiency
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[0059] 1) The mass and size of the asteroid can be determined according to the astronomical observation data, and the system is normalized. The mass sum of the double stars is unit mass, and the distance between the double stars is unit length. The normalized asteroid mass sum can be obtained size;
[0060] Select the double asteroid system 1996FG3 as an example to carry out periodic orbit search. According to the observation, the distance between the two stars in the system is 3km, the diameter of the main star is 1.69km, the diameter of the satellite is 0.49km, and the mass of the main star is 3.5×10 12 kg, satellite mass 1.0×10 11 kg, after normalization, the distance between the two stars is 1, the diameter of the main star is 0.5633, the diameter of the satellite is 0.1633, the mass of the main star is 0.972, and the mass of the satellite is 0.0278.
[0061] 2) Select the periodic orbit search range, select the initial position of the detector along the X-axis direction,...
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