Evidence for recent climate change on Mars from the identification of youthful near-surface ground ice
Ground ice in the crust and soil may be one of the largest reservoirs of water on Mars. Near-surface ground ice is predicted to be stable at latitudes higher than 40° (ref. 4), where a number of geomorphologic features indicative of viscous creep and hence ground ice have been observed. Mid-latitude...
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| Published in: | Nature (London) Vol. 412; no. 6845; pp. 411 - 414 |
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| Main Authors: | , , |
| Format: | Journal Article |
| Language: | English |
| Published: |
London
Nature Publishing
26-07-2001
Nature Publishing Group |
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| Abstract | Ground ice in the crust and soil may be one of the largest reservoirs of water on Mars. Near-surface ground ice is predicted to be stable at latitudes higher than 40° (ref. 4), where a number of geomorphologic features indicative of viscous creep and hence ground ice have been observed. Mid-latitude soils have also been implicated as a water-ice reservoir, the capacity of which is predicted to vary on a 100,000-year timescale owing to orbitally driven variations in climate. It is uncertain, however, whether near-surface ground ice currently exists at these latitudes, and how it is changing with time. Here we report observational evidence for a mid-latitude reservoir of near-surface water ice occupying the pore space of soils. The thickness of the ice-occupied soil reservoir (1-10 m) and its distribution in the 30° to 60° latitude bands indicate a reservoir of (1.5-6.0) × 104 km3, equivalent to a global layer of water 10-40 cm thick. We infer that the reservoir was created during the last phase of high orbital obliquity less than 100,000 years ago, and is now being diminished. |
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| AbstractList | We report observational evidence for a midlatitude Martian reservoir of near-surface water ice occupying the pore space of soils. The thickness of the ice-occupied soil reservoir (1-10 m) and its distribution in the 30 to 60 deg latitude bands indicate a reservoir of (1.5-6.0) x 10 exp 4 cu km, equivalent to a global layer of water 10-40 cm thick. We infer that the reservoir was created during the last phase of high orbital obliquity less than 100,000 years ago, and is now being diminished. (Author) Ground ice in the crust and soil may be one of the largest reservoirs of water on Mars. Mustard et al discuss observational evidence for a mid-latitude reservoir of near-surface water ice occupying the pore space of soils on the planet. Ground ice in the crust and soil may be one of the largest reservoirs of water on Mars. Near-surface ground ice is predicted to be stable at latitudes higher than 40° (ref. 4), where a number of geomorphologic features indicative of viscous creep and hence ground ice have been observed. Mid-latitude soils have also been implicated as a water-ice reservoir, the capacity of which is predicted to vary on a 100,000-year timescale owing to orbitally driven variations in climate. It is uncertain, however, whether near-surface ground ice currently exists at these latitudes, and how it is changing with time. Here we report observational evidence for a mid-latitude reservoir of near-surface water ice occupying the pore space of soils. The thickness of the ice-occupied soil reservoir (1-10 m) and its distribution in the 30° to 60° latitude bands indicate a reservoir of (1.5-6.0) × 104 km3, equivalent to a global layer of water 10-40 cm thick. We infer that the reservoir was created during the last phase of high orbital obliquity less than 100,000 years ago, and is now being diminished. Ground ice in the crust and soil may be one of the largest reservoirs of water on Mars. Near-surface ground ice is predicted to be stable at latitudes higher than 40 degrees (ref. 4), where a number of geomorphologic features indicative of viscous creep and hence ground ice have been observed. Mid-latitude soils have also been implicated as a water-ice reservoir, the capacity of which is predicted to vary on a 100,000-year timescale owing to orbitally driven variations in climate. It is uncertain, however, whether near-surface ground ice currently exists at these latitudes, and how it is changing with time. Here we report observational evidence for a mid-latitude reservoir of near-surface water ice occupying the pore space of soils. The thickness of the ice-occupied soil reservoir (1-10 m) and its distribution in the 30 degrees to 60 degrees latitude bands indicate a reservoir of (1.5-6.0) x 104 km3, equivalent to a global layer of water 10-40 cm thick. We infer that the reservoir was created during the last phase of high orbital obliquity less than 100,000 years ago, and is now being diminished. Ground ice in the crust and soil may be one of the largest reservoirs of water on Mars. Near-surface ground ice is predicted to be stable at latitudes higher than 40 degree , where a number of geomorphologic features indicative of viscous creep and hence ground ice have been observed. Mid-latitude soils have also been implicated as a water-ice reservoir, the capacity of which is predicted to vary on a 100,000-year timescale owing to orbitally driven variations in climate. It is uncertain, however, whether near-surface ground ice currently exists at these latitudes, and how it is changing with time. Here we report observational evidence for a mid-latitude reservoir of near-surface water ice occupying the pore space of soils. The thickness of the ice-occupied soil reservoir (1--10 m) and its distribution in the 30 degree to 60 degree latitude bands indicate a reservoir of (1.5-6.0) x 10 super(4) km super(3), equivalent to a global layer of water 10--40 cm thick. We infer that the reservoir was created during the last phase of high orbital obliquity less than 100,000 years ago, and is now being diminished. |
| Audience | Academic |
| Author | Mustard, John F Cooper, Christopher D Rifkin, Moses K |
| Author_xml | – sequence: 1 givenname: John F surname: Mustard fullname: Mustard, John F – sequence: 2 givenname: Christopher D surname: Cooper fullname: Cooper, Christopher D – sequence: 3 givenname: Moses K surname: Rifkin fullname: Rifkin, Moses K |
| BackLink | http://pascal-francis.inist.fr/vibad/index.php?action=getRecordDetail&idt=1088611$$DView record in Pascal Francis https://www.ncbi.nlm.nih.gov/pubmed/11473309$$D View this record in MEDLINE/PubMed |
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| CODEN | NATUAS |
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| Snippet | Ground ice in the crust and soil may be one of the largest reservoirs of water on Mars. Near-surface ground ice is predicted to be stable at latitudes higher... Ground ice in the crust and soil may be one of the largest reservoirs of water on Mars. Mustard et al discuss observational evidence for a mid-latitude... We report observational evidence for a midlatitude Martian reservoir of near-surface water ice occupying the pore space of soils. The thickness of the... |
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| SubjectTerms | Climate Climate change Cosmochemistry. Extraterrestrial geology Earth sciences Earth, ocean, space Exact sciences and technology Extraterrestrial Environment Extraterrestrial geology Geology Ground ice Ice Latitude Mars Reservoirs Soils Surface water Water |
| Title | Evidence for recent climate change on Mars from the identification of youthful near-surface ground ice |
| URI | http://dx.doi.org/10.1038/35086515 https://www.ncbi.nlm.nih.gov/pubmed/11473309 https://www.proquest.com/docview/204485663 https://search.proquest.com/docview/18427172 https://search.proquest.com/docview/27023872 https://search.proquest.com/docview/71045742 |
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