TOUGH+/GasH20 study of the effects of a heat source buried in theMartian permafrost
We use TOUGH+/GasH2O to study the effects of a heat sourceburied in the Martian permafrost to evaluate the possibility ofestablishing a wet zone of liquid water, in which terrestrialmicroorganisms could survive and multiply. Analysis of the problemindicates that (1) only a limited permafrost volume...
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ftosti:oai:osti.gov:923641 2023-07-30T04:04:04+02:00 TOUGH+/GasH20 study of the effects of a heat source buried in theMartian permafrost Moridis, George J. Pruess, Karsten 2008-03-13 application/pdf http://www.osti.gov/servlets/purl/923641 https://www.osti.gov/biblio/923641 unknown http://www.osti.gov/servlets/purl/923641 https://www.osti.gov/biblio/923641 54 HEAT SOURCES MICROORGANISMS PERMAFROST SOLS THICKNESS WATER 2008 ftosti 2023-07-11T08:45:48Z We use TOUGH+/GasH2O to study the effects of a heat sourceburied in the Martian permafrost to evaluate the possibility ofestablishing a wet zone of liquid water, in which terrestrialmicroorganisms could survive and multiply. Analysis of the problemindicates that (1) only a limited permafrost volume (not exceeding 0.35 min radius) is affected, (2) a "wet" zone with limited amounts of liquidwater de-velops (not exceeding 8 and 0.7 kg for a 250 W and a 62.5 Wsource, respectively), (3) the wet zone per-sists for a long time,becomes practically stationary after t = 20 sols because of venting intothe Martian atmosphere, and its thickness is limited and decreases slowlyover time, (4) a "dry" zone (where SG>0.9) evolves, continues toexpand (albeit slowly) with time, but its extent remains limited, and (5)the ice front surrounding the wet zone is self-sharpening. For a range ofinitial conditions investigated, evolution of the liquid water massoccurs at approximately the same rate, reaches roughly the same maximum,and occurs at about the same time (10 to 20 sols; 1 sol = 24.39hours). Other/Unknown Material Ice permafrost SciTec Connect (Office of Scientific and Technical Information - OSTI, U.S. Department of Energy) |
institution |
Open Polar |
collection |
SciTec Connect (Office of Scientific and Technical Information - OSTI, U.S. Department of Energy) |
op_collection_id |
ftosti |
language |
unknown |
topic |
54 HEAT SOURCES MICROORGANISMS PERMAFROST SOLS THICKNESS WATER |
spellingShingle |
54 HEAT SOURCES MICROORGANISMS PERMAFROST SOLS THICKNESS WATER Moridis, George J. Pruess, Karsten TOUGH+/GasH20 study of the effects of a heat source buried in theMartian permafrost |
topic_facet |
54 HEAT SOURCES MICROORGANISMS PERMAFROST SOLS THICKNESS WATER |
description |
We use TOUGH+/GasH2O to study the effects of a heat sourceburied in the Martian permafrost to evaluate the possibility ofestablishing a wet zone of liquid water, in which terrestrialmicroorganisms could survive and multiply. Analysis of the problemindicates that (1) only a limited permafrost volume (not exceeding 0.35 min radius) is affected, (2) a "wet" zone with limited amounts of liquidwater de-velops (not exceeding 8 and 0.7 kg for a 250 W and a 62.5 Wsource, respectively), (3) the wet zone per-sists for a long time,becomes practically stationary after t = 20 sols because of venting intothe Martian atmosphere, and its thickness is limited and decreases slowlyover time, (4) a "dry" zone (where SG>0.9) evolves, continues toexpand (albeit slowly) with time, but its extent remains limited, and (5)the ice front surrounding the wet zone is self-sharpening. For a range ofinitial conditions investigated, evolution of the liquid water massoccurs at approximately the same rate, reaches roughly the same maximum,and occurs at about the same time (10 to 20 sols; 1 sol = 24.39hours). |
author |
Moridis, George J. Pruess, Karsten |
author_facet |
Moridis, George J. Pruess, Karsten |
author_sort |
Moridis, George J. |
title |
TOUGH+/GasH20 study of the effects of a heat source buried in theMartian permafrost |
title_short |
TOUGH+/GasH20 study of the effects of a heat source buried in theMartian permafrost |
title_full |
TOUGH+/GasH20 study of the effects of a heat source buried in theMartian permafrost |
title_fullStr |
TOUGH+/GasH20 study of the effects of a heat source buried in theMartian permafrost |
title_full_unstemmed |
TOUGH+/GasH20 study of the effects of a heat source buried in theMartian permafrost |
title_sort |
tough+/gash20 study of the effects of a heat source buried in themartian permafrost |
publishDate |
2008 |
url |
http://www.osti.gov/servlets/purl/923641 https://www.osti.gov/biblio/923641 |
genre |
Ice permafrost |
genre_facet |
Ice permafrost |
op_relation |
http://www.osti.gov/servlets/purl/923641 https://www.osti.gov/biblio/923641 |
_version_ |
1772815245471907840 |