Interplanetary Dust and Carbonaceous Meteorites: Constraints on Porosity, Mineralogy and Chemistry of Meteors from Rubble-Pile Planetesimals

Details Interplanetary Dust and Carbonaceous Meteorites: Constraints on Porosity, Mineralogy and Chemistry of Meteors from Rubble-Pile Planetesimals Interplanetary Dust and Carbonaceous Meteorites: Constraints on Porosity, Mineralogy and Chemistry of Meteors from Rubble-Pile Planetesimals

Dec 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004em%26p...95..321r&link_type=abstract

Earth, Moon, and Planets, Volume 95, Issue 1-4, pp. 321-338

Physics

7

Asteroids, Carbonaceous Chondrites, Chemistry, Comets, Interplanetary Dust Particles, Meteors, Mineralogy, Porosity, Rubble-Pile Planetesimals, Structure

Scientific paper

This paper discusses measured textures, porosity, chemical compositions
and the minerals of interplanetary dust and meteorites from primitive
planetesimals and how this information can be used to explain some of
the observed physical and chemical properties of meteor phenomena.

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