Two-pulse planet capture orbit method based on weak stability boundary
A weakly stable, planetary technology, used in the aerospace field, which can solve problems such as infeasibility
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[0041] Such as figure 2 As shown, the present invention discloses a two-pulse planet capture orbit method based on weak stability boundary, comprising the following steps:
[0042] Step 1: Establish the motion equation of the probe under the sun-planet barycenter rotation system.
[0043] The origin of the coordinate system is the center of mass of the system, the X axis coincides with the sun and the line connecting the planets, and the sun points to Mars, the Z axis coincides with the angular velocity direction of the system rotation, and the Y axis is perpendicular to the X and Z axes to form a right-handed coordinate system.
[0044] The motion equation of the detector under this system can be expressed as
[0045] x ·· - 2 y · ...
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