Impacts into non-polar ice-rich paleodeposits on Mars: Excess ejecta craters, perched craters and pedestal craters as clues to Amazonian climate history

Details Impacts into non-polar ice-rich paleodeposits on Mars: Excess ejecta craters, perched craters and pedestal craters as clues to Amazonian climate history Impacts into non-polar ice-rich paleodeposits on Mars: Excess ejecta craters, perched craters and pedestal craters as clues to Amazonian climate history

Sep 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011icar..215...34k&link_type=abstract

Icarus, Volume 215, Issue 1, p. 34-46.

Computer Science

3

Scientific paper

We compare excess ejecta craters, perched craters, and pedestal craters on Mars. Impacts into ice-rich paleodeposits yield the genetically-related morphologies. The crater types have very similar excess thicknesses and geographic distributions. The primary distinguishing traits are the crater diameters and ages. Amazonian climate change results in episodic ice-rich deposits at mid latitudes.

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