Formation Constraints on Martian North Polar Volcanic Edifices

Details Formation Constraints on Martian North Polar Volcanic Edifices Formation Constraints on Martian North Polar Volcanic Edifices

Mar 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009lpi....40.1976f&link_type=abstract

40th Lunar and Planetary Science Conference, (Lunar and Planetary Science XL), held March 23-27, 2009 in The Woodlands, Texas, i

Computer Science

Scientific paper

Comparisons of topographic characteristics between Icelandic volcanoes
and martian north polar edifices imply that many of the latter may be of
subglacial origin and thus suggest a potential former ice sheet with a
minimum thickness of 80-550m.

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