Thermally Induced Graben in Peak-Ring Basins and Ghost Craters on Mercury

Details Thermally Induced Graben in Peak-Ring Basins and Ghost Craters on Mercury Thermally Induced Graben in Peak-Ring Basins and Ghost Craters on Mercury

Mar 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012lpi....43.2501b&link_type=abstract

43rd Lunar and Planetary Science Conference, held March 19–23, 2012 at The Woodlands, Texas. LPI Contribution No. 1659, id.2501

Physics

Scientific paper

The graben patterns seen in the interiors of mercurian peak-ring basins
Rachmaninoff, Raditladi, and Mozart, and in the ghost craters of the
northern plains of Mercury, can be attributed to thermal stresses in the
cooling volcanic fill.

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