Trapping of Interplanetary Dust Particles in Earth's Quasi-Satellite Resonance: Dependance on Particle Size

Details Trapping of Interplanetary Dust Particles in Earth's Quasi-Satellite Resonance: Dependance on Particle Size Trapping of Interplanetary Dust Particles in Earth's Quasi-Satellite Resonance: Dependance on Particle Size

Mar 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012lpi....43.2779k&link_type=abstract

43rd Lunar and Planetary Science Conference, held March 19–23, 2012 at The Woodlands, Texas. LPI Contribution No. 1659, id.2779

Physics

Scientific paper

Numerical simulations are used to model the orbital evolution of
interplanetary dust particles decaying into the inner solar system under
PR drag. Trapping in Earth's 1:1 quasi-satellite resonance is studied as
a function of dust particle diameter.

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