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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Online Access: | http://www.osti.gov/servlets/purl/1634970 https://www.osti.gov/biblio/1634970 https://doi.org/10.1016/j.icarus.2020.113897 |
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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 |
container_volume |
350 |
container_start_page |
113897 |
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1772820770650587136 |