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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Online Access: | http://hdl.handle.net/10150/636169 https://doi.org/10.1029/2018je005861 |
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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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1766031825480712192 |