Origins and Age Constraints of the Palos Crater Floor Deposits and Tinto Vallis, Mars

Details Origins and Age Constraints of the Palos Crater Floor Deposits and Tinto Vallis, Mars Origins and Age Constraints of the Palos Crater Floor Deposits and Tinto Vallis, Mars

Mar 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012lpi....43.2261r&link_type=abstract

43rd Lunar and Planetary Science Conference, held March 19–23, 2012 at The Woodlands, Texas. LPI Contribution No. 1659, id.2261

Physics

Scientific paper

Our observations indicate that the previously hypothesized volcanic
origin of Tinto Vallis is very unlikely. Palos crater records variety of
events and it likely served as a conduit for water and material transfer
from Hesperia to Amenthes Planum.

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