Properties of Lunar Crater Ejecta from New 70-cm Radar Observations

Details Properties of Lunar Crater Ejecta from New 70-cm Radar Observations Properties of Lunar Crater Ejecta from New 70-cm Radar Observations

Mar 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004lpi....35.1679g&link_type=abstract

35th Lunar and Planetary Science Conference, March 15-19, 2004, League City, Texas, abstract no.1679

Mathematics

Logic

2

Scientific paper

Recent 70-cm radar observations are used to examine the properties of
lunar impact crater ejecta. Preliminary work suggests that block size
variations, not mineralogical differences, are likely responsible for
characteristic low-radar-return haloes.

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