Origin and composition of three heterolithic boulder- and cobble-bearing deposits overlying the Murray and Stimson formations, Gale Crater, Mars

Heterolithic, boulder-containing, pebble-strewn surfaces occur along the lower slopes of Aeolis Mons (“Mt. Sharp”) in Gale crater, Mars. They were observed in HiRISE images acquired from orbit prior to the landing of the Curiosity rover. The rover was used to investigate three of these units named B...

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Published in:Icarus
Main Authors: Wiens, Roger Craig, Edgett, Kenneth S., Stack, Kathryn M., Dietrich, William E., Bryk, Alexander B., Mangold, Nicolas, Bedford, Candice, Gasda, Patrick L., Fairén, Alberto, Thompson, Lucy M., Johnson, Jeffrey R., Gasnault, Olivier, Clegg, Samuel M., Cousin, Agnes, Forni, Olivier, Frydenvang, Jens, Lanza, Nina Louise, Maurice, Sylvestre, Newsom, Horton, Ollila, Anna Martha, Payré, Valerie, Rivera-Hernandez, Frances, Vasavada, Ashwin R.
Language:unknown
Published: 2023
Subjects:
Online Access:http://www.osti.gov/servlets/purl/1634970
https://www.osti.gov/biblio/1634970
https://doi.org/10.1016/j.icarus.2020.113897
id ftosti:oai:osti.gov:1634970
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spelling ftosti:oai:osti.gov:1634970 2023-07-30T04:07:28+02:00 Origin and composition of three heterolithic boulder- and cobble-bearing deposits overlying the Murray and Stimson formations, Gale Crater, Mars Wiens, Roger Craig Edgett, Kenneth S. Stack, Kathryn M. Dietrich, William E. Bryk, Alexander B. Mangold, Nicolas Bedford, Candice Gasda, Patrick L. Fairén, Alberto Thompson, Lucy M. Johnson, Jeffrey R. Gasnault, Olivier Clegg, Samuel M. Cousin, Agnes Forni, Olivier Frydenvang, Jens Lanza, Nina Louise Maurice, Sylvestre Newsom, Horton Ollila, Anna Martha Payré, Valerie Rivera-Hernandez, Frances Vasavada, Ashwin R. 2023-07-03 application/pdf http://www.osti.gov/servlets/purl/1634970 https://www.osti.gov/biblio/1634970 https://doi.org/10.1016/j.icarus.2020.113897 unknown http://www.osti.gov/servlets/purl/1634970 https://www.osti.gov/biblio/1634970 https://doi.org/10.1016/j.icarus.2020.113897 doi:10.1016/j.icarus.2020.113897 58 GEOSCIENCES 2023 ftosti https://doi.org/10.1016/j.icarus.2020.113897 2023-07-11T09:43:36Z Heterolithic, boulder-containing, pebble-strewn surfaces occur along the lower slopes of Aeolis Mons (“Mt. Sharp”) in Gale crater, Mars. They were observed in HiRISE images acquired from orbit prior to the landing of the Curiosity rover. The rover was used to investigate three of these units named Blackfoot, Brandberg, and Bimbe between sols 1099 and 1410. These unconsolidated units overlie the lower Murray formation that forms the base of Mt. Sharp, and consist of pebbles, cobbles and boulders. Blackfoot also overlies portions of the Stimson formation, which consists of eolian sandstone that is understood to significantly postdate the dominantly lacustrine deposition of the Murray formation. Blackfoot is elliptical in shape (62 x 26 m), while Brandberg is nearly circular (50 x 55 m), and Bimbe is irregular in shape, covering about ten times the area of the other two. The largest boulders are 1.5–2.5 m in size and are interpreted to be sandstones. As seen from orbit, some boulders are light-toned and others are dark-toned. Rover-based observations show that both have the same gray appearance from the ground and their apparently different albedos in orbital observations result from relatively flat skyfacing surfaces. Chemical observations show that two clasts of fine sandstone at Bimbe have similar compositions and morphologies to nine ChemCam targets observed early in the mission, near Yellowknife Bay, including the Bathurst Inlet outcrop, and to at least one target (Pyramid Hills, Sol 692) and possibly a cap rock unit just north of Hidden Valley, locations that are several kilometers apart in distance and tens of meters in elevation. These findings may suggest the earlier existence of draping strata, like the Stimson formation, that would have overlain the current surface from Bimbe to Yellowknife Bay. Compositionally these extinct strata could be related to the Siccar Point group to which the Stimson formation belongs. Other/Unknown Material Yellowknife SciTec Connect (Office of Scientific and Technical Information - OSTI, U.S. Department of Energy) Yellowknife Yellowknife Bay ENVELOPE(-114.336,-114.336,62.367,62.367) The Landing ENVELOPE(-45.689,-45.689,-60.733,-60.733) Pyramid ENVELOPE(157.300,157.300,-81.333,-81.333) Bathurst Inlet ENVELOPE(-108.051,-108.051,66.840,66.840) Hidden Valley ENVELOPE(78.451,78.451,-68.615,-68.615) Icarus 350 113897
institution Open Polar
collection SciTec Connect (Office of Scientific and Technical Information - OSTI, U.S. Department of Energy)
op_collection_id ftosti
language unknown
topic 58 GEOSCIENCES
spellingShingle 58 GEOSCIENCES
Wiens, Roger Craig
Edgett, Kenneth S.
Stack, Kathryn M.
Dietrich, William E.
Bryk, Alexander B.
Mangold, Nicolas
Bedford, Candice
Gasda, Patrick L.
Fairén, Alberto
Thompson, Lucy M.
Johnson, Jeffrey R.
Gasnault, Olivier
Clegg, Samuel M.
Cousin, Agnes
Forni, Olivier
Frydenvang, Jens
Lanza, Nina Louise
Maurice, Sylvestre
Newsom, Horton
Ollila, Anna Martha
Payré, Valerie
Rivera-Hernandez, Frances
Vasavada, Ashwin R.
Origin and composition of three heterolithic boulder- and cobble-bearing deposits overlying the Murray and Stimson formations, Gale Crater, Mars
topic_facet 58 GEOSCIENCES
description Heterolithic, boulder-containing, pebble-strewn surfaces occur along the lower slopes of Aeolis Mons (“Mt. Sharp”) in Gale crater, Mars. They were observed in HiRISE images acquired from orbit prior to the landing of the Curiosity rover. The rover was used to investigate three of these units named Blackfoot, Brandberg, and Bimbe between sols 1099 and 1410. These unconsolidated units overlie the lower Murray formation that forms the base of Mt. Sharp, and consist of pebbles, cobbles and boulders. Blackfoot also overlies portions of the Stimson formation, which consists of eolian sandstone that is understood to significantly postdate the dominantly lacustrine deposition of the Murray formation. Blackfoot is elliptical in shape (62 x 26 m), while Brandberg is nearly circular (50 x 55 m), and Bimbe is irregular in shape, covering about ten times the area of the other two. The largest boulders are 1.5–2.5 m in size and are interpreted to be sandstones. As seen from orbit, some boulders are light-toned and others are dark-toned. Rover-based observations show that both have the same gray appearance from the ground and their apparently different albedos in orbital observations result from relatively flat skyfacing surfaces. Chemical observations show that two clasts of fine sandstone at Bimbe have similar compositions and morphologies to nine ChemCam targets observed early in the mission, near Yellowknife Bay, including the Bathurst Inlet outcrop, and to at least one target (Pyramid Hills, Sol 692) and possibly a cap rock unit just north of Hidden Valley, locations that are several kilometers apart in distance and tens of meters in elevation. These findings may suggest the earlier existence of draping strata, like the Stimson formation, that would have overlain the current surface from Bimbe to Yellowknife Bay. Compositionally these extinct strata could be related to the Siccar Point group to which the Stimson formation belongs.
author Wiens, Roger Craig
Edgett, Kenneth S.
Stack, Kathryn M.
Dietrich, William E.
Bryk, Alexander B.
Mangold, Nicolas
Bedford, Candice
Gasda, Patrick L.
Fairén, Alberto
Thompson, Lucy M.
Johnson, Jeffrey R.
Gasnault, Olivier
Clegg, Samuel M.
Cousin, Agnes
Forni, Olivier
Frydenvang, Jens
Lanza, Nina Louise
Maurice, Sylvestre
Newsom, Horton
Ollila, Anna Martha
Payré, Valerie
Rivera-Hernandez, Frances
Vasavada, Ashwin R.
author_facet Wiens, Roger Craig
Edgett, Kenneth S.
Stack, Kathryn M.
Dietrich, William E.
Bryk, Alexander B.
Mangold, Nicolas
Bedford, Candice
Gasda, Patrick L.
Fairén, Alberto
Thompson, Lucy M.
Johnson, Jeffrey R.
Gasnault, Olivier
Clegg, Samuel M.
Cousin, Agnes
Forni, Olivier
Frydenvang, Jens
Lanza, Nina Louise
Maurice, Sylvestre
Newsom, Horton
Ollila, Anna Martha
Payré, Valerie
Rivera-Hernandez, Frances
Vasavada, Ashwin R.
author_sort Wiens, Roger Craig
title Origin and composition of three heterolithic boulder- and cobble-bearing deposits overlying the Murray and Stimson formations, Gale Crater, Mars
title_short Origin and composition of three heterolithic boulder- and cobble-bearing deposits overlying the Murray and Stimson formations, Gale Crater, Mars
title_full Origin and composition of three heterolithic boulder- and cobble-bearing deposits overlying the Murray and Stimson formations, Gale Crater, Mars
title_fullStr Origin and composition of three heterolithic boulder- and cobble-bearing deposits overlying the Murray and Stimson formations, Gale Crater, Mars
title_full_unstemmed Origin and composition of three heterolithic boulder- and cobble-bearing deposits overlying the Murray and Stimson formations, Gale Crater, Mars
title_sort origin and composition of three heterolithic boulder- and cobble-bearing deposits overlying the murray and stimson formations, gale crater, mars
publishDate 2023
url http://www.osti.gov/servlets/purl/1634970
https://www.osti.gov/biblio/1634970
https://doi.org/10.1016/j.icarus.2020.113897
long_lat ENVELOPE(-114.336,-114.336,62.367,62.367)
ENVELOPE(-45.689,-45.689,-60.733,-60.733)
ENVELOPE(157.300,157.300,-81.333,-81.333)
ENVELOPE(-108.051,-108.051,66.840,66.840)
ENVELOPE(78.451,78.451,-68.615,-68.615)
geographic Yellowknife
Yellowknife Bay
The Landing
Pyramid
Bathurst Inlet
Hidden Valley
geographic_facet Yellowknife
Yellowknife Bay
The Landing
Pyramid
Bathurst Inlet
Hidden Valley
genre Yellowknife
genre_facet Yellowknife
op_relation http://www.osti.gov/servlets/purl/1634970
https://www.osti.gov/biblio/1634970
https://doi.org/10.1016/j.icarus.2020.113897
doi:10.1016/j.icarus.2020.113897
op_doi https://doi.org/10.1016/j.icarus.2020.113897
container_title Icarus
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