Interplanetary dust particles - Disintegration and orbital motion

Details Interplanetary dust particles - Disintegration and orbital motion Interplanetary dust particles - Disintegration and orbital motion

Jan 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993em%26p...60...17k&link_type=abstract

Earth, Moon, and Planets (ISSN 0167-9295), vol. 60, no. 1, p. 17-21.

Physics

5

Interplanetary Dust, Orbital Mechanics, Solar Wind, Disintegration, Eccentricity, Poynting-Robertson Effect, Radiation Pressure

Scientific paper

Abrupt or gradual disintegration of the interplanetary dust particle causes increase of its distance from the sun due to the solar radiation pressure. The problem of the orbital evolution of the interplanetary dust particles under such disintegration processes is discussed. The process of gradual disintegration due to the solar wind particles is calculated in detail. Obtained results represent corrections to the changes of orbital elements for the Poynting-Robertson effect and effect of the solar wind.

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