Erosional Shadow Remnants as Terrestrial Analogs for Teardrop-Shaped Islands on Mars: Implications for Outflow Channel Formation

Details Erosional Shadow Remnants as Terrestrial Analogs for Teardrop-Shaped Islands on Mars: Implications for Outflow Channel Formation Erosional Shadow Remnants as Terrestrial Analogs for Teardrop-Shaped Islands on Mars: Implications for Outflow Channel Formation

Mar 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011lpi....42.1005m&link_type=abstract

42nd Lunar and Planetary Science Conference, held March 7–11, 2011 at The Woodlands, Texas. LPI Contribution No. 1608, p.1005

Astronomy and Astrophysics

Astrophysics

Scientific paper

This work proposes that teardrop-shaped islands located on the outflow
channels of Mars might have been formed as the result of catastrophic
submarine mass movements similar to those documented within continental
margins on Earth.

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