Deposition, exhumation, and paleoclimate of an ancient lake deposit, Gale crater, Mars

Science
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Abstract

The landforms of northern Gale crater on Mars expose thick sequences of sedimentary rocks. Based on images obtained by the Curiosity rover, we interpret these outcrops as evidence for past fluvial, deltaic, and lacustrine environments. Degradation of the crater wall and rim probably supplied these sediments, which advanced inward from the wall, infilling both the crater and an internal lake basin to a thickness of at least 75 meters. This intracrater lake system probably existed intermittently for thousands to millions of years, implying a relatively wet climate that supplied moisture to the crater rim and transported sediment via streams into the lake basin. The deposits in Gale crater were then exhumed, probably by wind-driven erosion, creating Aeolis Mons (Mount Sharp).

Publication type Article
Publication Subtype Journal Article
Title Deposition, exhumation, and paleoclimate of an ancient lake deposit, Gale crater, Mars
Series title Science
DOI 10.1126/science.aac7575
Volume 350
Issue 6257
Year Published 2015
Language English
Publisher American Association for the Advancement of Science
Publisher location New York, NY
Contributing office(s) Astrogeology Science Center
Larger Work Type Article
Larger Work Subtype Journal Article
Larger Work Title Science
Other Geospatial Gale crater, Mars
Online Only (Y/N) N
Additional Online Files (Y/N) N
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