Burial and Exhumation of Sedimentary Rocks Revealed by the Base Stimson Erosional Unconformity, Gale Crater, Mars
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Burial and Exhumation of Sedimentary Rocks Revealed by the Base Stimson Erosional Unconformity, Gale Crater, Mars. / Watkins, Jessica A.; Grotzinger, John P.; Stein, Nathan T.; Banham, Steven G.; Gupta, Sanjeev; Rubin, David M.; Morgan, Kathryn Stack; Edgett, Kenneth S.; Frydenvang, Jens; Siebach, Kirsten L.; Lamb, Michael P.; Sumner, Dawn Y.; Lewis, Kevin W.
In: Journal of Geophysical Research - Planets, Vol. 127, No. 7, e2022JE007293, 2022.Research output: Contribution to journal › Journal article › Research › peer-review
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TY - JOUR
T1 - Burial and Exhumation of Sedimentary Rocks Revealed by the Base Stimson Erosional Unconformity, Gale Crater, Mars
AU - Watkins, Jessica A.
AU - Grotzinger, John P.
AU - Stein, Nathan T.
AU - Banham, Steven G.
AU - Gupta, Sanjeev
AU - Rubin, David M.
AU - Morgan, Kathryn Stack
AU - Edgett, Kenneth S.
AU - Frydenvang, Jens
AU - Siebach, Kirsten L.
AU - Lamb, Michael P.
AU - Sumner, Dawn Y.
AU - Lewis, Kevin W.
PY - 2022
Y1 - 2022
N2 - Sedimentary rocks record the ancient climate of Mars through changes between subaqueous and eolian depositional environments, recognized by their stratal geometries and suites of sedimentary structures. Orbiter- and rover-image-based geologic mapping show a dynamic evolution of the 5-km-thick sedimentary sequence exposed along the flanks of Aeolis Mons (informally, Mt. Sharp) in Gale crater, Mars, by deposition of subaqueous strata followed by exhumation via eolian erosion and then deposition of overlying, onlapping strata of inferred eolian origin. This interpretation suggests that a significant unconformity should occur at the base of the onlapping strata, thus predicting lateral variations in elevation along the contact between the underlying Mt. Sharp group and overlying Stimson formation. Curiosity rover and high-resolution orbital image data quantify paleotopographic variability associated with the contact; similar to 140 m of net elevation change and a slope closely aligned with the modern topography is expressed along the regional contact. These results support the interpretation of an erosional unconformity between these strata and that it was likely formed as a result of eolian erosion within the crater, indicative of a transition from wet to dry climate and providing insight into the stratigraphic context, geologic history, and habitability within Gale crater.
AB - Sedimentary rocks record the ancient climate of Mars through changes between subaqueous and eolian depositional environments, recognized by their stratal geometries and suites of sedimentary structures. Orbiter- and rover-image-based geologic mapping show a dynamic evolution of the 5-km-thick sedimentary sequence exposed along the flanks of Aeolis Mons (informally, Mt. Sharp) in Gale crater, Mars, by deposition of subaqueous strata followed by exhumation via eolian erosion and then deposition of overlying, onlapping strata of inferred eolian origin. This interpretation suggests that a significant unconformity should occur at the base of the onlapping strata, thus predicting lateral variations in elevation along the contact between the underlying Mt. Sharp group and overlying Stimson formation. Curiosity rover and high-resolution orbital image data quantify paleotopographic variability associated with the contact; similar to 140 m of net elevation change and a slope closely aligned with the modern topography is expressed along the regional contact. These results support the interpretation of an erosional unconformity between these strata and that it was likely formed as a result of eolian erosion within the crater, indicative of a transition from wet to dry climate and providing insight into the stratigraphic context, geologic history, and habitability within Gale crater.
KW - Mars
KW - sedimentary
KW - unconformity
KW - erosion
KW - gale
KW - STRATIGRAPHY
KW - EVOLUTION
KW - MUDSTONE
KW - ANCIENT
KW - RECORD
U2 - 10.1029/2022JE007293
DO - 10.1029/2022JE007293
M3 - Journal article
VL - 127
JO - Journal of Geophysical Research: Solid Earth
JF - Journal of Geophysical Research: Solid Earth
SN - 0148-0227
IS - 7
M1 - e2022JE007293
ER -
ID: 312706780