Morphologic Observations of Chasma Boreale, Mars Using MOC, THEMIS, and MOLA: Origins Revisted

Details Morphologic Observations of Chasma Boreale, Mars Using MOC, THEMIS, and MOLA: Origins Revisted Morphologic Observations of Chasma Boreale, Mars Using MOC, THEMIS, and MOLA: Origins Revisted

Mar 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006lpi....37.1363w&link_type=abstract

37th Annual Lunar and Planetary Science Conference, March 13-17, 2006, League City, Texas, abstract no.1363

Astronomy and Astrophysics

Astrophysics

Scientific paper

The current models of formation for Chasma Boreale involve wind or
catastrophic fluvial erosion. We provide new evidence from THEMIS and
MOC data suggesting basal north polar ice melting, possibly induced by
youthful volcanic activity.

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