Martian Orbital Change and Its Effect on the Formation of Permafrost Polygons

Details Martian Orbital Change and Its Effect on the Formation of Permafrost Polygons Martian Orbital Change and Its Effect on the Formation of Permafrost Polygons

Mar 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999lpi....30.1118m&link_type=abstract

30th Annual Lunar and Planetary Science Conference, March 15-29, 1999, Houston, TX, abstract no. 1118

Physics

1

Scientific paper

Small-scale polygonal patterns have been observed on Mars and may have
been formed by thermal contraction in ice-cemented permafrost. The
seasonal tensile stress in martian permafrost is calculated at various
climatic conditions to evaluate polygon formation.

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