How the Shape and Volume of Impact Tracks in Stardust Aerogel Reflect Cometary Dust Properties: Experimental Evidence

Details How the Shape and Volume of Impact Tracks in Stardust Aerogel Reflect Cometary Dust Properties: Experimental Evidence How the Shape and Volume of Impact Tracks in Stardust Aerogel Reflect Cometary Dust Properties: Experimental Evidence

Mar 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012lpi....43.1398k&link_type=abstract

43rd Lunar and Planetary Science Conference, held March 19–23, 2012 at The Woodlands, Texas. LPI Contribution No. 1659, id.1398

Physics

Scientific paper

Stardust aerogel track shape was controlled by impactor internal
structure, subgrain size and overall strength, rather than bulk grain
density. Carbonaceous chondrite powders make Type B tracks; organics can
make distinctive, squat "carrot" tracks.

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