Sulfide and Layer Silicate Grain Size Distributions Constrain the Unique Petrogenesis of a Type CM Interplanetary Dust Particle

Details Sulfide and Layer Silicate Grain Size Distributions Constrain the Unique Petrogenesis of a Type CM Interplanetary Dust Particle Sulfide and Layer Silicate Grain Size Distributions Constrain the Unique Petrogenesis of a Type CM Interplanetary Dust Particle

Mar 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994lpi....25.1131r&link_type=gif

Abstracts of the 25th Lunar and Planetary Science Conference, held in Houston, TX, 14-18 March 1994., p.1131

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