Premium
Mars Climate History: Insights From Impact Crater Wall Slope Statistics
Author(s) -
Kreslavsky Mikhail A.,
Head James W.
Publication year - 2018
Publication title -
geophysical research letters
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.007
H-Index - 273
eISSN - 1944-8007
pISSN - 0094-8276
DOI - 10.1002/2017gl075663
Subject(s) - noachian , hesperian , impact crater , amazonian , mars exploration program , geology , orbiter , mass wasting , latitude , altimeter , astrobiology , geomorphology , geodesy , martian , ecology , landslide , amazon rainforest , physics , engineering , biology , aerospace engineering
Abstract We use the global distribution of the steepest slopes on crater walls derived from Mars Orbiter Laser Altimeter profile data to assess the magnitudes of degradational processes with latitude, altitude, and time. We independently confirm that Amazonian polar/high‐latitude crater slope modification is substantial, but that craters in the low latitudes have essentially escaped significant slope modification since the Early Hesperian. We find that the total amount of crater wall degradation in the Late Noachian is very small in comparison to the circumpolar regions in the Late Amazonian, an observation that we interpret to mean that the Late Noachian climate was not characterized by persistent and continuous warm and wet conditions. A confirmed elevational zonality in degradation in the Early Hesperian is interpreted to mean that the atmosphere was denser than today.