Microanalyses of interplanetary dust particles and micrometeorites: implications for sample return missions to undifferentiated protoplanets

Details Microanalyses of interplanetary dust particles and micrometeorites: implications for sample return missions to undifferentiated protoplanets Microanalyses of interplanetary dust particles and micrometeorites: implications for sample return missions to undifferentiated protoplanets

Jan 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004adspr..34.2286r&link_type=abstract

Advances in Space Research, Volume 34, Issue 11, p. 2286-2291.

Physics

Interplanetary Dust Particles, Micrometeorites, Sample Return Missions, Comets, Asteroids, Microanalyses

Scientific paper

A few grams of sample from an asteroid or a comet nucleus contain a cornucopia of information on accretion and evolution, including space weathering, of small, undifferentiated protoplanets. The information can be extracted by already available state-of-the-art microanalytical tools together with testable hypotheses of solar nebula dust accretion and parent body modification based on the laboratory analyses of undifferentiated meteoritic materials.

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