Circular Features Located on Lineated Terrain, Ismenius Lacus Region, Mars: Implications for Post-Impact Crater Modification Attributed to Sub-Surface Ice Deflation

Details Circular Features Located on Lineated Terrain, Ismenius Lacus Region, Mars: Implications for Post-Impact Crater Modification Attributed to Sub-Surface Ice Deflation Circular Features Located on Lineated Terrain, Ismenius Lacus Region, Mars: Implications for Post-Impact Crater Modification Attributed to Sub-Surface Ice Deflation

Mar 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006lpi....37.1498m&link_type=abstract

37th Annual Lunar and Planetary Science Conference, March 13-17, 2006, League City, Texas, abstract no.1498

Physics

Scientific paper

Modified impact craters on lineated terrains formed by impact into
ice-bearing material followed by infill and subsequent sublimation of
the ice, resulting in collapsed crater rims, single and multiple inner
rings and central layered deposits.

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