semi-major axis iteration space transfer orbit calculation method for Lambert orbital transfer problem based on Newton iteration
A technology for transferring orbits and calculation methods, which is applied in complex mathematical operations and other directions, and can solve problems such as poor timeliness and complex calculations
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Embodiment 1
[0049] A semi-major axis iterative solution method for the Lambert orbit problem based on Newton's iterative thought, the semi-major axis iterative solution method comprises the following steps:
[0050] Step 1: Know the initial time t 1 The position vector of the mission vehicle on the initial orbit is r 1 , rendezvous time t 2 The position vector of the target aircraft in the target orbit is r 2 , calculate the transfer angle θ, auxiliary variable c and auxiliary variable s;
[0051] Step 2: According to the transfer angle θ, auxiliary variable c and auxiliary variable s calculated in step 1, determine the shape of the space transfer orbit of the aircraft;
[0052] Step 3: When the transfer time Δt is greater than the parabolic orbit transfer time Δt p , the transfer orbit is an elliptical orbit, and the elliptical orbit is solved;
[0053] Introducing the semi-major axis of the minimum energy ellipse When am , there is no elliptical transfer orbit between the two poi...
Embodiment 2
[0093] Next, select the orbit change position in the geocentric inertial system as r 1 =[-0.6058 0.3742 0.4001]×10 7 m, the intersection position is r 2 =[-1.5981 -2.1344 0.1212]×10 7 m as an example, the technical solution of the present invention will be further described in conjunction with the accompanying drawings.
[0094] Step 1: Calculate transfer angle θ=1.4707rad, auxiliary variable c=2.7121×10 7 m and auxiliary variable s=3.0990×10 7 m;
[0095] Using the orbital elements to solve the mission vehicle's orbit change position r at the initial moment 1 Velocity vector at
[0096] Calculate the distance r between the initial position and the intersection position 1 =||r 1 ||=8.168×10 6 m,r 2 =||r 2 ||=2.6691×10 7 m.
[0097] Step 2: Determine the track shape according to the transfer angle θ calculated in step 1, the auxiliary variable c and the auxiliary variable s;
[0098]
[0099] Where μ is the gravitational constant of the earth, and the parabol...
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