The Mars Northern Residual Ice Cap: New Geomorphologic Facts About Its Formation and Evolution

Details The Mars Northern Residual Ice Cap: New Geomorphologic Facts About Its Formation and Evolution The Mars Northern Residual Ice Cap: New Geomorphologic Facts About Its Formation and Evolution

Mar 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008lpi....39.1283d&link_type=abstract

39th Lunar and Planetary Science Conference, (Lunar and Planetary Science XXXIX), held March 10-14, 2008 in League City, Texas.

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The NPLD form a dome on the pole and it is connected to a lobe. These
two entities are separated by Chasma Boreale. They are, however, joined
by a transition zone having unique geomorphologic characteristics that
can be explained by ice flow mechanism.

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