Crater Floor Polygons (CFPs): Signs of Desiccated Paleolakes on Mars?

Details Crater Floor Polygons (CFPs): Signs of Desiccated Paleolakes on Mars? Crater Floor Polygons (CFPs): Signs of Desiccated Paleolakes on Mars?

Mar 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010lpi....41.1650e&link_type=abstract

41st Lunar and Planetary Science Conference, held March 1-5, 2010 in The Woodlands, Texas. LPI Contribution No. 1533, p.1650

Physics

1

Scientific paper

Crater floor polygons on Mars are globally mapped. Physical modeling
suggests that thermal stresses are not responsible for formation of
these polygons, and as such, we propose desiccation to be the main
driving mechanism for formation.

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