Loading…
Impact-induced overland fluid flow and channelized erosion at Lyot Crater, Mars
Lyot Crater is one of the youngest impact basins > 200 km in diameter on Mars. Although published hydrological models suggest that impact‐related groundwater release might have occurred at Lyot, no geomorphic evidence for such activity has been previously identified. Here, we use images acquired...
Saved in:
| Published in: | Geophysical research letters 2010-11, Vol.37 (21), p.np-n/a |
|---|---|
| Main Authors: | , , , , , , , |
| Format: | Article |
| Language: | English |
| Subjects: | |
| Citations: | Items that this one cites Items that cite this one |
| Online Access: | Get full text |
| Tags: |
Add Tag
No Tags, Be the first to tag this record!
|
| cited_by | cdi_FETCH-LOGICAL-c4126-d5664c10b8240ff5c19424cdf1f6a7381dfba59e14ca03cf52b10b7566ba2d583 |
|---|---|
| cites | cdi_FETCH-LOGICAL-c4126-d5664c10b8240ff5c19424cdf1f6a7381dfba59e14ca03cf52b10b7566ba2d583 |
| container_end_page | n/a |
| container_issue | 21 |
| container_start_page | np |
| container_title | Geophysical research letters |
| container_volume | 37 |
| creator | Harrison, Tanya N. Malin, Michael C. Edgett, Kenneth S. Shean, David E. Kennedy, Megan R. Lipkaman, Leslie J. Cantor, Bruce A. Posiolova, Liliya V. |
| description | Lyot Crater is one of the youngest impact basins > 200 km in diameter on Mars. Although published hydrological models suggest that impact‐related groundwater release might have occurred at Lyot, no geomorphic evidence for such activity has been previously identified. Here, we use images acquired predominantly by the Mars Reconnaissance Orbiter (MRO) Context Camera (CTX) and Mars Odyssey Thermal Emission Imaging Spectrometer (THEMIS) visible and infrared subsystems to document an extensive channeled scabland extending to the north, west, and east of Lyot, covering an area of ∼300,000 km2. The configuration and morphology suggests that the channel‐forming fluid was water derived from the target substrate and/or the surrounding terrain. Possible formation mechanisms are groundwater mobilization by seismic energy from the impact event and dewatering of the ejecta blanket. |
| doi_str_mv | 10.1029/2010GL045074 |
| format | article |
| fullrecord | <record><control><sourceid>proquest_cross</sourceid><recordid>TN_cdi_proquest_miscellaneous_1671580696</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>1671580696</sourcerecordid><originalsourceid>FETCH-LOGICAL-c4126-d5664c10b8240ff5c19424cdf1f6a7381dfba59e14ca03cf52b10b7566ba2d583</originalsourceid><addsrcrecordid>eNqFkMtKxDAUhoMoOF52PkA3ggurJ_d2KUVHoSqI4jJk0gSjnXZMOur49KaMiCvd5ALf9_Ofg9ABhhMMpDwlgGFaA-Mg2Qaa4JKxvACQm2gCUKY3kWIb7cT4DAAUKJ6g26v5Qpsh912zNLbJ-jcbWt01mWuXfjz792z8mifddbb1n4mxoY--7zI9ZPWqH7Iq6MGG4-xah7iHtpxuo93_vnfRw8X5fXWZ17fTq-qszg3DROQNF4IZDLOCMHCOm9SVMNM47ISWtMCNm2leWsyMBmocJ7MEy2TNNGl4QXfR0Tp3EfrXpY2DmvtobJu6234ZFRYS8wJEKf5HOSlLVoKgCT1eoyaNGIN1ahH8XIeVwqDGFavfK0744Xeyjka3LujO-PjjECpEAcXYgKy5d9_a1Z-ZanpXE8lhlPK15ONgP34kHV6UkFRy9XgzVdUFFNfA71RFvwAb1ZcJ</addsrcrecordid><sourcetype>Aggregation Database</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>1529949063</pqid></control><display><type>article</type><title>Impact-induced overland fluid flow and channelized erosion at Lyot Crater, Mars</title><source>Wiley-Blackwell AGU Digital Archive</source><creator>Harrison, Tanya N. ; Malin, Michael C. ; Edgett, Kenneth S. ; Shean, David E. ; Kennedy, Megan R. ; Lipkaman, Leslie J. ; Cantor, Bruce A. ; Posiolova, Liliya V.</creator><creatorcontrib>Harrison, Tanya N. ; Malin, Michael C. ; Edgett, Kenneth S. ; Shean, David E. ; Kennedy, Megan R. ; Lipkaman, Leslie J. ; Cantor, Bruce A. ; Posiolova, Liliya V.</creatorcontrib><description>Lyot Crater is one of the youngest impact basins > 200 km in diameter on Mars. Although published hydrological models suggest that impact‐related groundwater release might have occurred at Lyot, no geomorphic evidence for such activity has been previously identified. Here, we use images acquired predominantly by the Mars Reconnaissance Orbiter (MRO) Context Camera (CTX) and Mars Odyssey Thermal Emission Imaging Spectrometer (THEMIS) visible and infrared subsystems to document an extensive channeled scabland extending to the north, west, and east of Lyot, covering an area of ∼300,000 km2. The configuration and morphology suggests that the channel‐forming fluid was water derived from the target substrate and/or the surrounding terrain. Possible formation mechanisms are groundwater mobilization by seismic energy from the impact event and dewatering of the ejecta blanket.</description><identifier>ISSN: 0094-8276</identifier><identifier>EISSN: 1944-8007</identifier><identifier>DOI: 10.1029/2010GL045074</identifier><identifier>CODEN: GPRLAJ</identifier><language>eng</language><publisher>Washington, DC: Blackwell Publishing Ltd</publisher><subject>Computational fluid dynamics ; crater ; Craters ; Earth sciences ; Earth, ocean, space ; Exact sciences and technology ; Fluid flow ; Fluids ; fluvial processes ; Groundwater ; Hydrology ; Imaging spectrometers ; impact ; Lyot ; Mars</subject><ispartof>Geophysical research letters, 2010-11, Vol.37 (21), p.np-n/a</ispartof><rights>Copyright 2010 by the American Geophysical Union.</rights><rights>2015 INIST-CNRS</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c4126-d5664c10b8240ff5c19424cdf1f6a7381dfba59e14ca03cf52b10b7566ba2d583</citedby><cites>FETCH-LOGICAL-c4126-d5664c10b8240ff5c19424cdf1f6a7381dfba59e14ca03cf52b10b7566ba2d583</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktopdf>$$Uhttps://onlinelibrary.wiley.com/doi/pdf/10.1029%2F2010GL045074$$EPDF$$P50$$Gwiley$$H</linktopdf><linktohtml>$$Uhttps://onlinelibrary.wiley.com/doi/full/10.1029%2F2010GL045074$$EHTML$$P50$$Gwiley$$H</linktohtml><link.rule.ids>314,780,784,11514,27924,27925,46468,46892</link.rule.ids><backlink>$$Uhttp://pascal-francis.inist.fr/vibad/index.php?action=getRecordDetail&idt=23668086$$DView record in Pascal Francis$$Hfree_for_read</backlink></links><search><creatorcontrib>Harrison, Tanya N.</creatorcontrib><creatorcontrib>Malin, Michael C.</creatorcontrib><creatorcontrib>Edgett, Kenneth S.</creatorcontrib><creatorcontrib>Shean, David E.</creatorcontrib><creatorcontrib>Kennedy, Megan R.</creatorcontrib><creatorcontrib>Lipkaman, Leslie J.</creatorcontrib><creatorcontrib>Cantor, Bruce A.</creatorcontrib><creatorcontrib>Posiolova, Liliya V.</creatorcontrib><title>Impact-induced overland fluid flow and channelized erosion at Lyot Crater, Mars</title><title>Geophysical research letters</title><addtitle>Geophys. Res. Lett</addtitle><description>Lyot Crater is one of the youngest impact basins > 200 km in diameter on Mars. Although published hydrological models suggest that impact‐related groundwater release might have occurred at Lyot, no geomorphic evidence for such activity has been previously identified. Here, we use images acquired predominantly by the Mars Reconnaissance Orbiter (MRO) Context Camera (CTX) and Mars Odyssey Thermal Emission Imaging Spectrometer (THEMIS) visible and infrared subsystems to document an extensive channeled scabland extending to the north, west, and east of Lyot, covering an area of ∼300,000 km2. The configuration and morphology suggests that the channel‐forming fluid was water derived from the target substrate and/or the surrounding terrain. Possible formation mechanisms are groundwater mobilization by seismic energy from the impact event and dewatering of the ejecta blanket.</description><subject>Computational fluid dynamics</subject><subject>crater</subject><subject>Craters</subject><subject>Earth sciences</subject><subject>Earth, ocean, space</subject><subject>Exact sciences and technology</subject><subject>Fluid flow</subject><subject>Fluids</subject><subject>fluvial processes</subject><subject>Groundwater</subject><subject>Hydrology</subject><subject>Imaging spectrometers</subject><subject>impact</subject><subject>Lyot</subject><subject>Mars</subject><issn>0094-8276</issn><issn>1944-8007</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2010</creationdate><recordtype>article</recordtype><recordid>eNqFkMtKxDAUhoMoOF52PkA3ggurJ_d2KUVHoSqI4jJk0gSjnXZMOur49KaMiCvd5ALf9_Ofg9ABhhMMpDwlgGFaA-Mg2Qaa4JKxvACQm2gCUKY3kWIb7cT4DAAUKJ6g26v5Qpsh912zNLbJ-jcbWt01mWuXfjz792z8mifddbb1n4mxoY--7zI9ZPWqH7Iq6MGG4-xah7iHtpxuo93_vnfRw8X5fXWZ17fTq-qszg3DROQNF4IZDLOCMHCOm9SVMNM47ISWtMCNm2leWsyMBmocJ7MEy2TNNGl4QXfR0Tp3EfrXpY2DmvtobJu6234ZFRYS8wJEKf5HOSlLVoKgCT1eoyaNGIN1ahH8XIeVwqDGFavfK0744Xeyjka3LujO-PjjECpEAcXYgKy5d9_a1Z-ZanpXE8lhlPK15ONgP34kHV6UkFRy9XgzVdUFFNfA71RFvwAb1ZcJ</recordid><startdate>201011</startdate><enddate>201011</enddate><creator>Harrison, Tanya N.</creator><creator>Malin, Michael C.</creator><creator>Edgett, Kenneth S.</creator><creator>Shean, David E.</creator><creator>Kennedy, Megan R.</creator><creator>Lipkaman, Leslie J.</creator><creator>Cantor, Bruce A.</creator><creator>Posiolova, Liliya V.</creator><general>Blackwell Publishing Ltd</general><general>American Geophysical Union</general><scope>BSCLL</scope><scope>IQODW</scope><scope>AAYXX</scope><scope>CITATION</scope><scope>7QH</scope><scope>7TG</scope><scope>7UA</scope><scope>C1K</scope><scope>F1W</scope><scope>H96</scope><scope>KL.</scope><scope>L.G</scope><scope>8FD</scope><scope>H8D</scope><scope>L7M</scope></search><sort><creationdate>201011</creationdate><title>Impact-induced overland fluid flow and channelized erosion at Lyot Crater, Mars</title><author>Harrison, Tanya N. ; Malin, Michael C. ; Edgett, Kenneth S. ; Shean, David E. ; Kennedy, Megan R. ; Lipkaman, Leslie J. ; Cantor, Bruce A. ; Posiolova, Liliya V.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c4126-d5664c10b8240ff5c19424cdf1f6a7381dfba59e14ca03cf52b10b7566ba2d583</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2010</creationdate><topic>Computational fluid dynamics</topic><topic>crater</topic><topic>Craters</topic><topic>Earth sciences</topic><topic>Earth, ocean, space</topic><topic>Exact sciences and technology</topic><topic>Fluid flow</topic><topic>Fluids</topic><topic>fluvial processes</topic><topic>Groundwater</topic><topic>Hydrology</topic><topic>Imaging spectrometers</topic><topic>impact</topic><topic>Lyot</topic><topic>Mars</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Harrison, Tanya N.</creatorcontrib><creatorcontrib>Malin, Michael C.</creatorcontrib><creatorcontrib>Edgett, Kenneth S.</creatorcontrib><creatorcontrib>Shean, David E.</creatorcontrib><creatorcontrib>Kennedy, Megan R.</creatorcontrib><creatorcontrib>Lipkaman, Leslie J.</creatorcontrib><creatorcontrib>Cantor, Bruce A.</creatorcontrib><creatorcontrib>Posiolova, Liliya V.</creatorcontrib><collection>Istex</collection><collection>Pascal-Francis</collection><collection>CrossRef</collection><collection>Aqualine</collection><collection>Meteorological & Geoastrophysical Abstracts</collection><collection>Water Resources Abstracts</collection><collection>Environmental Sciences and Pollution Management</collection><collection>ASFA: Aquatic Sciences and Fisheries Abstracts</collection><collection>Aquatic Science & Fisheries Abstracts (ASFA) 2: Ocean Technology, Policy & Non-Living Resources</collection><collection>Meteorological & Geoastrophysical Abstracts - Academic</collection><collection>Aquatic Science & Fisheries Abstracts (ASFA) Professional</collection><collection>Technology Research Database</collection><collection>Aerospace Database</collection><collection>Advanced Technologies Database with Aerospace</collection><jtitle>Geophysical research letters</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Harrison, Tanya N.</au><au>Malin, Michael C.</au><au>Edgett, Kenneth S.</au><au>Shean, David E.</au><au>Kennedy, Megan R.</au><au>Lipkaman, Leslie J.</au><au>Cantor, Bruce A.</au><au>Posiolova, Liliya V.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Impact-induced overland fluid flow and channelized erosion at Lyot Crater, Mars</atitle><jtitle>Geophysical research letters</jtitle><addtitle>Geophys. Res. Lett</addtitle><date>2010-11</date><risdate>2010</risdate><volume>37</volume><issue>21</issue><spage>np</spage><epage>n/a</epage><pages>np-n/a</pages><issn>0094-8276</issn><eissn>1944-8007</eissn><coden>GPRLAJ</coden><abstract>Lyot Crater is one of the youngest impact basins > 200 km in diameter on Mars. Although published hydrological models suggest that impact‐related groundwater release might have occurred at Lyot, no geomorphic evidence for such activity has been previously identified. Here, we use images acquired predominantly by the Mars Reconnaissance Orbiter (MRO) Context Camera (CTX) and Mars Odyssey Thermal Emission Imaging Spectrometer (THEMIS) visible and infrared subsystems to document an extensive channeled scabland extending to the north, west, and east of Lyot, covering an area of ∼300,000 km2. The configuration and morphology suggests that the channel‐forming fluid was water derived from the target substrate and/or the surrounding terrain. Possible formation mechanisms are groundwater mobilization by seismic energy from the impact event and dewatering of the ejecta blanket.</abstract><cop>Washington, DC</cop><pub>Blackwell Publishing Ltd</pub><doi>10.1029/2010GL045074</doi><tpages>6</tpages></addata></record> |
| fulltext | fulltext |
| identifier | ISSN: 0094-8276 |
| ispartof | Geophysical research letters, 2010-11, Vol.37 (21), p.np-n/a |
| issn | 0094-8276 1944-8007 |
| language | eng |
| recordid | cdi_proquest_miscellaneous_1671580696 |
| source | Wiley-Blackwell AGU Digital Archive |
| subjects | Computational fluid dynamics crater Craters Earth sciences Earth, ocean, space Exact sciences and technology Fluid flow Fluids fluvial processes Groundwater Hydrology Imaging spectrometers impact Lyot Mars |
| title | Impact-induced overland fluid flow and channelized erosion at Lyot Crater, Mars |
| url | http://sfxeu10.hosted.exlibrisgroup.com/loughborough?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-01-02T18%3A12%3A29IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-proquest_cross&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=Impact-induced%20overland%20fluid%20flow%20and%20channelized%20erosion%20at%20Lyot%20Crater,%20Mars&rft.jtitle=Geophysical%20research%20letters&rft.au=Harrison,%20Tanya%20N.&rft.date=2010-11&rft.volume=37&rft.issue=21&rft.spage=np&rft.epage=n/a&rft.pages=np-n/a&rft.issn=0094-8276&rft.eissn=1944-8007&rft.coden=GPRLAJ&rft_id=info:doi/10.1029/2010GL045074&rft_dat=%3Cproquest_cross%3E1671580696%3C/proquest_cross%3E%3Cgrp_id%3Ecdi_FETCH-LOGICAL-c4126-d5664c10b8240ff5c19424cdf1f6a7381dfba59e14ca03cf52b10b7566ba2d583%3C/grp_id%3E%3Coa%3E%3C/oa%3E%3Curl%3E%3C/url%3E&rft_id=info:oai/&rft_pqid=1529949063&rft_id=info:pmid/&rfr_iscdi=true |