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The Orbital Distributions of Particles Resulting from Multiple Close Encounters with Planet in a Steady-State Approximation

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Dikarev,  Valeri
Ralf Srama - Heidelberg Dust Group, Research Groups, MPI for Nuclear Physics, Max Planck Society;

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Grün,  Eberhard
Ralf Srama - Heidelberg Dust Group, Research Groups, MPI for Nuclear Physics, Max Planck Society;

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Citation

Dikarev, V., & Grün, E. (2004). The Orbital Distributions of Particles Resulting from Multiple Close Encounters with Planet in a Steady-State Approximation. In Order and Chaos in Stellar and Planetary Systems (pp. 122-128).


Cite as: http://hdl.handle.net/11858/00-001M-0000-0011-8D41-2
Abstract
Dynamics of meteoroids and dust grains of cometary origin are investigated both analytically and numerically. The gravity of the Sun and one planet is taken into account. A simple analytical formula for the orbital distribution of particles in the regime of close encounters with Jupiter is suggested supposing ergodicity on a limited region of phase space.