Islands of ice on Mars and Pluto

Ice sheets, such as the polar layered deposits (PLDs) of Mars, are of great interest as records of past climate. Smaller outlier ice deposits near the north and south PLDs are likely more sensitive to climate changes and thus may hold information about more recent climate history. However, the south...

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Published in:Journal of Geophysical Research: Planets
Main Authors: Sori, Michael M., Bapst, Jonathan, Becerra, Patricio, Byrne, Shane
Other Authors: Univ Arizona, Lunar & Planetary Lab
Format: Article in Journal/Newspaper
Language:English
Published: AMER GEOPHYSICAL UNION 2019
Subjects:
Online Access:http://hdl.handle.net/10150/636169
https://doi.org/10.1029/2018je005861
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record_format openpolar
spelling ftunivarizona:oai:repository.arizona.edu:10150/636169 2023-05-15T16:41:24+02:00 Islands of ice on Mars and Pluto Sori, Michael M. Bapst, Jonathan Becerra, Patricio Byrne, Shane Univ Arizona, Lunar & Planetary Lab 2019 http://hdl.handle.net/10150/636169 https://doi.org/10.1029/2018je005861 en eng AMER GEOPHYSICAL UNION Sori, M. M., Bapst, J., Becerra, P., & Byrne, S. (2019). Islands of ice on Mars and Pluto. Journal of Geophysical Research: Planets, 124, 2522–2542. https://doi.org/10.1029/2018JE005861 2169-9097 doi:10.1029/2018je005861 http://hdl.handle.net/10150/636169 2169-9100 JOURNAL OF GEOPHYSICAL RESEARCH-PLANETS © 2019. American Geophysical Union. All Rights Reserved. 124 10 2522-2542 ice mounds volatiles craters south polar layered deposits Sputnik Planitia Article 2019 ftunivarizona https://doi.org/10.1029/2018je005861 https://doi.org/10.1029/2018JE005861 2020-06-14T08:18:02Z Ice sheets, such as the polar layered deposits (PLDs) of Mars, are of great interest as records of past climate. Smaller outlier ice deposits near the north and south PLDs are likely more sensitive to climate changes and thus may hold information about more recent climate history. However, the southern outlier deposits have largely remained unmapped and unanalyzed. Here, we identify 31 deposits near, but separated from, Mars's south PLDs, all of which are located within impact craters >15 km in diameter. On the basis of morphology, radar analysis, physical similarity to portions of the PLD margin, and overall similarity to previously described deposits in Mars's north polar region, we conclude that these deposits are primarily composed of water ice. An additional 66 craters contain smaller depositional features, some of which may be remnant ice deposits. The 31 outlier ice deposits represent a previously unquantified inventory of water on Mars, with a total volume between 15,000 and 38,000 km(3). In addition, we identify five analogous outlier nitrogen ice deposits located within impact craters near Sputnik Planitia, the large nitrogen ice sheet on Pluto. Although important differences exist between Mars and Pluto, broad physical similarities between the two cases suggest that the topography and microclimates of impact craters cause them to be favorable locations for volatile accumulation and/or retention throughout the Solar System. NASA's Mars Data Analysis Program National Aeronautics & Space Administration (NASA) [80NSSC17K0510] 6 month embargo; published online 15 Oct 2019 This item from the UA Faculty Publications collection is made available by the University of Arizona with support from the University of Arizona Libraries. If you have questions, please contact us at repository@u.library.arizona.edu. Article in Journal/Newspaper Ice Sheet The University of Arizona: UA Campus Repository Sputnik ENVELOPE(66.167,66.167,-70.833,-70.833) Journal of Geophysical Research: Planets 124 10 2522 2542
institution Open Polar
collection The University of Arizona: UA Campus Repository
op_collection_id ftunivarizona
language English
topic ice mounds
volatiles
craters
south polar layered deposits
Sputnik Planitia
spellingShingle ice mounds
volatiles
craters
south polar layered deposits
Sputnik Planitia
Sori, Michael M.
Bapst, Jonathan
Becerra, Patricio
Byrne, Shane
Islands of ice on Mars and Pluto
topic_facet ice mounds
volatiles
craters
south polar layered deposits
Sputnik Planitia
description Ice sheets, such as the polar layered deposits (PLDs) of Mars, are of great interest as records of past climate. Smaller outlier ice deposits near the north and south PLDs are likely more sensitive to climate changes and thus may hold information about more recent climate history. However, the southern outlier deposits have largely remained unmapped and unanalyzed. Here, we identify 31 deposits near, but separated from, Mars's south PLDs, all of which are located within impact craters >15 km in diameter. On the basis of morphology, radar analysis, physical similarity to portions of the PLD margin, and overall similarity to previously described deposits in Mars's north polar region, we conclude that these deposits are primarily composed of water ice. An additional 66 craters contain smaller depositional features, some of which may be remnant ice deposits. The 31 outlier ice deposits represent a previously unquantified inventory of water on Mars, with a total volume between 15,000 and 38,000 km(3). In addition, we identify five analogous outlier nitrogen ice deposits located within impact craters near Sputnik Planitia, the large nitrogen ice sheet on Pluto. Although important differences exist between Mars and Pluto, broad physical similarities between the two cases suggest that the topography and microclimates of impact craters cause them to be favorable locations for volatile accumulation and/or retention throughout the Solar System. NASA's Mars Data Analysis Program National Aeronautics & Space Administration (NASA) [80NSSC17K0510] 6 month embargo; published online 15 Oct 2019 This item from the UA Faculty Publications collection is made available by the University of Arizona with support from the University of Arizona Libraries. If you have questions, please contact us at repository@u.library.arizona.edu.
author2 Univ Arizona, Lunar & Planetary Lab
format Article in Journal/Newspaper
author Sori, Michael M.
Bapst, Jonathan
Becerra, Patricio
Byrne, Shane
author_facet Sori, Michael M.
Bapst, Jonathan
Becerra, Patricio
Byrne, Shane
author_sort Sori, Michael M.
title Islands of ice on Mars and Pluto
title_short Islands of ice on Mars and Pluto
title_full Islands of ice on Mars and Pluto
title_fullStr Islands of ice on Mars and Pluto
title_full_unstemmed Islands of ice on Mars and Pluto
title_sort islands of ice on mars and pluto
publisher AMER GEOPHYSICAL UNION
publishDate 2019
url http://hdl.handle.net/10150/636169
https://doi.org/10.1029/2018je005861
long_lat ENVELOPE(66.167,66.167,-70.833,-70.833)
geographic Sputnik
geographic_facet Sputnik
genre Ice Sheet
genre_facet Ice Sheet
op_source 124
10
2522-2542
op_relation Sori, M. M., Bapst, J., Becerra, P., & Byrne, S. (2019). Islands of ice on Mars and Pluto. Journal of Geophysical Research: Planets, 124, 2522–2542. https://doi.org/10.1029/2018JE005861
2169-9097
doi:10.1029/2018je005861
http://hdl.handle.net/10150/636169
2169-9100
JOURNAL OF GEOPHYSICAL RESEARCH-PLANETS
op_rights © 2019. American Geophysical Union. All Rights Reserved.
op_doi https://doi.org/10.1029/2018je005861
https://doi.org/10.1029/2018JE005861
container_title Journal of Geophysical Research: Planets
container_volume 124
container_issue 10
container_start_page 2522
op_container_end_page 2542
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