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Weidenschilling, S · 1993 · arXiv 1993.1099

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astro-ph.EP 1

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2026 1

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Resonance and Stochastic Dynamics of Interplanetary Dust

astro-ph.EP · 2026-06-22 · unverdicted · novelty 5.0

Dust particles inspiraling under PR drag are temporarily trapped in MMRs, escape due to overstability of librations, then undergo stochastic scattering with predicted fractions for planetary collision, sublimation, or ejection via an analytic epicycle model and Monte Carlo method.

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  • Resonance and Stochastic Dynamics of Interplanetary Dust astro-ph.EP · 2026-06-22 · unverdicted · none · ref 35

    Dust particles inspiraling under PR drag are temporarily trapped in MMRs, escape due to overstability of librations, then undergo stochastic scattering with predicted fractions for planetary collision, sublimation, or ejection via an analytic epicycle model and Monte Carlo method.