A Two-Pulse Planet Capture Orbit Method Based on Weak Stability Boundary
A weakly stable, planetary technology, applied in the aerospace field, can solve problems such as infeasibility, and achieve the effect of large application range, small speed increment, and fuel saving.
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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]
[0046] where μ=m 2 / (m 1 +m 2 ) represents the mass coefficient of the system, m 1 is the mass of the sun, m 2 is the mass of the planet, . is the distance between the detector and the sun, is the distance between the probe and the planet.
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