Method for calculating stable orbit of non-synchronous binary star system
An orbital calculation and asynchronous technology, applied in the aerospace field, can solve the problems of inapplicability of asynchronous systems, and achieve the effects of many orbital families, high computational efficiency and good convergence.
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[0055] A kind of stable orbit calculation method of non-synchronous binary star system of the present embodiment, comprises the following steps:
[0056] Step 1. According to the determined parameters of the target binary star system, ignoring the difference in spin angular velocity, the binary star system is considered as a synchronous binary star system, an ellipsoid-ellipsoid binary star system model is established, and a dynamic model is established in the center-of-mass rotating coordinate system. The parameters of the binary system include the shape, mass ratio and relative distance of the binary.
[0057]
[0058] Where ρ represents the position vector from the detector to the center of mass, ω is the rotational angular velocity of the system, and ρ 1 and ρ 2 is the position vector from the detector to the primary and secondary stars of the binary star. u 1 , U 2 Denotes the gravitational potential energy of a binary star:
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