On the Evolution of Balloon Satellite Motions in a Plane Restricted Three-Body Problem with Light Pressure
Autor: | A. V. Dobroslavskiy, P. S. Krasilnikov |
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Rok vydání: | 2018 |
Předmět: |
Physics
Phase portrait Earth's shadow Astronomy and Astrophysics 02 engineering and technology Three-body problem 01 natural sciences Displacement (vector) 020303 mechanical engineering & transports Mean motion Classical mechanics 0203 mechanical engineering Radiation pressure Space and Planetary Science Physics::Space Physics 0103 physical sciences Trajectory Satellite Astrophysics::Earth and Planetary Astrophysics 010303 astronomy & astrophysics |
Zdroj: | Astronomy Letters. 44:567-578 |
ISSN: | 1562-6873 1063-7737 |
DOI: | 10.1134/s1063773718090025 |
Popis: | We investigate the evolution of high Earth satellite orbits under gravitational perturbations from the Sun and light pressure forces, without the Earth shadow effect. We present the disturbing function of the problem provided that the satellite is a sphere. The mean value of the disturbing function in the absence of resonances between the mean unperturbed motion of the satellite and the mean motion of the Sun has also been obtained. The semimajor axis of the satellite orbit and the mean value of the disturbing function are shown to be integrals of the averaged osculating equations. TheHill version of the problem, whereby the distance to the satellite is much smaller than the Earth–Sun distance, has been studied in detail: we have constructed the phase portraits of the oscillations at various parameters and described three types of quasiperiodic satellite trajectories—librational and rotational trajectories as well as Earth collision trajectories. Numerical simulations of trajectories have allowed the additional effects caused by light pressure to be described: the displacement of the bounded trajectory of the satellite as a whole relative to the trajectory of the classical three-body problem into a region more distant from the Sun. |
Databáze: | OpenAIRE |
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