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://hdl.handle.net/10261/234109 https://doi.org/10.1016/j.icarus.2020.113897 |
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ftcsic:oai:digital.csic.es:10261/234109 2024-02-11T10:09:27+01:00 Origin and composition of three heterolithic boulder- and cobble-bearing deposits overlying the Murray and Stimson formations, Gale Crater, Mars Wiens, Roger C. Edgett, Kenneth S. Stack, K. Dietrich, William E. Bryk, Alexander B. Mangold, Nicolas Bedford, Candice Gasda, Patrick Fairén, Alberto G. Thompson, L. Johnson, Jeff Gasnault, Olivier Clegg, Sam Cousin, Agnes Forni, Olivier Frydenvang, J. Lanza, Nina Maurice, Sylvestre Newsom, H. Payré, Valerie Rivera-Hernandez, Frances Vasavada, Ashwin R. 2020 http://hdl.handle.net/10261/234109 https://doi.org/10.1016/j.icarus.2020.113897 unknown Academic Press http://dx.doi.org/10.1016/j.icarus.2020.113897 Sí doi:10.1016/j.icarus.2020.113897 issn: 1090-2643 Icarus 350 (2020) http://hdl.handle.net/10261/234109 open artículo http://purl.org/coar/resource_type/c_6501 2020 ftcsic https://doi.org/10.1016/j.icarus.2020.113897 2024-01-16T11:04:41Z 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 × 26 m), while Brandberg is nearly circular (50 × 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 sky-facing 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. Dark, massive sandstone blocks at Bimbe are chemically distinct from blocks of similar ... Article in Journal/Newspaper Yellowknife Digital.CSIC (Spanish National Research Council) Bathurst Inlet ENVELOPE(-108.051,-108.051,66.840,66.840) Hidden Valley ENVELOPE(78.451,78.451,-68.615,-68.615) Pyramid ENVELOPE(157.300,157.300,-81.333,-81.333) The Landing ENVELOPE(-45.689,-45.689,-60.733,-60.733) Yellowknife Yellowknife Bay ENVELOPE(-114.336,-114.336,62.367,62.367) Icarus 350 113897 |
institution |
Open Polar |
collection |
Digital.CSIC (Spanish National Research Council) |
op_collection_id |
ftcsic |
language |
unknown |
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 × 26 m), while Brandberg is nearly circular (50 × 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 sky-facing 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. Dark, massive sandstone blocks at Bimbe are chemically distinct from blocks of similar ... |
format |
Article in Journal/Newspaper |
author |
Wiens, Roger C. Edgett, Kenneth S. Stack, K. Dietrich, William E. Bryk, Alexander B. Mangold, Nicolas Bedford, Candice Gasda, Patrick Fairén, Alberto G. Thompson, L. Johnson, Jeff Gasnault, Olivier Clegg, Sam Cousin, Agnes Forni, Olivier Frydenvang, J. Lanza, Nina Maurice, Sylvestre Newsom, H. Payré, Valerie Rivera-Hernandez, Frances Vasavada, Ashwin R. |
spellingShingle |
Wiens, Roger C. Edgett, Kenneth S. Stack, K. Dietrich, William E. Bryk, Alexander B. Mangold, Nicolas Bedford, Candice Gasda, Patrick Fairén, Alberto G. Thompson, L. Johnson, Jeff Gasnault, Olivier Clegg, Sam Cousin, Agnes Forni, Olivier Frydenvang, J. Lanza, Nina Maurice, Sylvestre Newsom, H. 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 |
author_facet |
Wiens, Roger C. Edgett, Kenneth S. Stack, K. Dietrich, William E. Bryk, Alexander B. Mangold, Nicolas Bedford, Candice Gasda, Patrick Fairén, Alberto G. Thompson, L. Johnson, Jeff Gasnault, Olivier Clegg, Sam Cousin, Agnes Forni, Olivier Frydenvang, J. Lanza, Nina Maurice, Sylvestre Newsom, H. Payré, Valerie Rivera-Hernandez, Frances Vasavada, Ashwin R. |
author_sort |
Wiens, Roger C. |
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 |
publisher |
Academic Press |
publishDate |
2020 |
url |
http://hdl.handle.net/10261/234109 https://doi.org/10.1016/j.icarus.2020.113897 |
long_lat |
ENVELOPE(-108.051,-108.051,66.840,66.840) ENVELOPE(78.451,78.451,-68.615,-68.615) ENVELOPE(157.300,157.300,-81.333,-81.333) ENVELOPE(-45.689,-45.689,-60.733,-60.733) ENVELOPE(-114.336,-114.336,62.367,62.367) |
geographic |
Bathurst Inlet Hidden Valley Pyramid The Landing Yellowknife Yellowknife Bay |
geographic_facet |
Bathurst Inlet Hidden Valley Pyramid The Landing Yellowknife Yellowknife Bay |
genre |
Yellowknife |
genre_facet |
Yellowknife |
op_relation |
http://dx.doi.org/10.1016/j.icarus.2020.113897 Sí doi:10.1016/j.icarus.2020.113897 issn: 1090-2643 Icarus 350 (2020) http://hdl.handle.net/10261/234109 |
op_rights |
open |
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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1790609338677592064 |