Chasma Boreale, Mars: A Product of Non-Uniform Polar Accumulation Influenced by Basal Topography

Details Chasma Boreale, Mars: A Product of Non-Uniform Polar Accumulation Influenced by Basal Topography Chasma Boreale, Mars: A Product of Non-Uniform Polar Accumulation Influenced by Basal Topography

Mar 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010lpi....41.2547h&link_type=abstract

41st Lunar and Planetary Science Conference, held March 1-5, 2010 in The Woodlands, Texas. LPI Contribution No. 1533, p.2547

Physics

Scientific paper

The mapping of radar unconformities within Planum Boreum, Mars reveals
episodes of deposition and erosion leading to non-uniform accumulation
of the NPLD and the early creation of Chasma Boreale, Gemina Lingula,
and a now-buried, major chasma.

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