Twin asteroid detection autonomous cooperation optical navigation method
A technology of optical navigation and double asteroids, which is applied in the direction of integrated navigators and navigation calculation tools, etc., which can solve the problems of inaccurate master star and slave star ephemeris, affecting navigation accuracy, and inaccurate slave stars, etc.
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[0065] The double asteroid system 65803 Didymos is selected as the target celestial body, and Table 1 lists various parameters of the double asteroid system 65803 Didymos. The orbits of the binary asteroid around the center of the double asteroid system are in the same plane as the orbit of the double asteroid system around the sun, the resolution of the navigation camera is 500×500 pixels, the field of view is 90°, and the focal length of the navigation camera is is 20mm, and the camera measurement error is 4×10 -3 rad, the inter-satellite ranging error is 0.1m, and the inter-satellite angle measurement error is 1×10 -3 rad. The mass of the detector is constant at 500kg and the maximum cross-sectional area is 20m 2 , and the reflection coefficient is assumed to be 1.
[0066] Table 1 Parameters of the binary asteroid 65803 Didymos
[0067]
[0068] Let the initial position of the detector 1 be the Lagrangian point L4 of the double asteroid system, and the normal vector...
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