A New Approach to Evaluate Planetary Perturbations on a Cloud of Dust in Low Eccentricity Heliocentric Orbits
1985 ◽
Vol 85
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pp. 381-384
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AbstractDynamical perturbations on ensembles of particles in heliocentric orbits of low eccentricity are integrated over time. The dust is perturbed by radiation pressure, Poynting-Robertson drag, their corpuscular counterparts, and by gravitation due to any number of planets. A dust cloud is represented by a set of centroids and orbital dispersions (about the centroids). Gravitational perturbations on the centroid are derived from a single matrix, valid for any planet, in the appropriate frame of reference. After transformation of the time derivatives to a common coordinate system, the perturbation rates are summed up and integrated. The time dependence of the planets’ orbital elements are evaluated inside the time integral.
2008 ◽
Vol 37
(4)
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pp. 597-620
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2019 ◽
Vol 18
(02)
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pp. 1950010
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Keyword(s):
2020 ◽
Vol 117
(18)
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pp. 9712-9722
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Keyword(s):
Keyword(s):