Pit-Floor Craters on Mercury: Characteristics and Modes of Formation

Details Pit-Floor Craters on Mercury: Characteristics and Modes of Formation Pit-Floor Craters on Mercury: Characteristics and Modes of Formation

Mar 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009lpi....40.2234g&link_type=abstract

40th Lunar and Planetary Science Conference, (Lunar and Planetary Science XL), held March 23-27, 2009 in The Woodlands, Texas, i

Physics

Scientific paper

We classify pit craters on Mercury into two categories on the basis of
morphology and size: small irregular-sized pit craters and larger-sized,
steep-sided pit craters. We conclude that differences in pit morphology
relates to the mode of formation.

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