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- W287714188 abstract "Midlatitude ground ice on Mars is of significant scientific interest for understanding the history and evolution of ice stability on Mars and is relevant for human exploration as a possible in situ resource. For both science and exploration, assessing the astrobiological potential of the ice is important in terms of (1) understanding the potential for life on Mars and (2) evaluating the presence of possible biohazards in advance of human exploration. In the present study, we review the evidence for midlatitude ground ice on Mars, discuss the possible explanations for its occurrence, and assess its potential habitability. During the course of study, we systematically analyzed remote-sensing data sets to determine whether a viable landing site exists in the northern midlatitudes to enable a robotic mission that conducts in situ characterization and searches for evidence of life in the ice. We classified each site according to (1) presence of polygons as a proxy for subsurface ice, (2) presence and abundance of rough topographic obstacles (e.g., large cracks, cliffs, uneven topography), (3) rock density, (4) presence and abundance of large boulders, and (5) presence of craters. We found that a suitable landing site exists within Amazonis Planitia near ground ice that was recently excavated by a meteorite impact. Key Words: Mars—Missions—Habitability—Landing sites—Ice. Astrobiology 14, 102–118." @default.
- W287714188 created "2016-06-24" @default.
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- W287714188 date "2014-02-01" @default.
- W287714188 modified "2023-09-30" @default.
- W287714188 title "Midlatitude Ice-Rich Ground on Mars as a Target in the Search for Evidence of Life and for <i>in situ</i> Resource Utilization on Human Missions" @default.
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- W287714188 doi "https://doi.org/10.1089/ast.2013.1103" @default.
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