Modeling the Formation of Large Desiccation Polygons on Earth: Possible Relation to Intermediate-Sized Polygons on Mars and Implications to Mars Hydrology

Details Modeling the Formation of Large Desiccation Polygons on Earth: Possible Relation to Intermediate-Sized Polygons on Mars and Implications to Mars Hydrology Modeling the Formation of Large Desiccation Polygons on Earth: Possible Relation to Intermediate-Sized Polygons on Mars and Implications to Mars Hydrology

Mar 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012lpi....43.1063e&link_type=abstract

43rd Lunar and Planetary Science Conference, held March 19–23, 2012 at The Woodlands, Texas. LPI Contribution No. 1659, id.1063

Physics

Scientific paper

We present a pre-fracture model to constrain the models of formation of
giant desiccation cracks on Earth as a possible analog to
intermediate-sized (70-350 m large) polygons located in many
impact craters on Mars.

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