New insight into lunar impact melt mobility from the LRO camera
The Lunar Reconnaissance Orbiter Camera (LROC) is systematically imaging impact melt deposits in and around lunar craters at meter and sub‐meter scales. These images reveal that lunar impact melts, although morphologically similar to terrestrial lava flows of similar size, exhibit distinctive featur...
Gespeichert in:
| Veröffentlicht in: | Geophysical research letters 2010-11, Vol.37 (21), p.np-n/a |
|---|---|
| Hauptverfasser: | , , , , , , , , , , , |
| Format: | Artikel |
| Sprache: | eng |
| Schlagworte: | |
| Online-Zugang: | Volltext |
| Tags: |
Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
|
| container_end_page | n/a |
|---|---|
| container_issue | 21 |
| container_start_page | np |
| container_title | Geophysical research letters |
| container_volume | 37 |
| creator | Bray, V. J. Tornabene, L. L. Keszthelyi, L. P. McEwen, A. S. Hawke, B. R. Giguere, T. A. Kattenhorn, S. A. Garry, W. B. Rizk, B. Caudill, C. M. Gaddis, L. R. van der Bogert, C. H. |
| description | The Lunar Reconnaissance Orbiter Camera (LROC) is systematically imaging impact melt deposits in and around lunar craters at meter and sub‐meter scales. These images reveal that lunar impact melts, although morphologically similar to terrestrial lava flows of similar size, exhibit distinctive features (e.g., erosional channels). Although generated in a single rapid event, the post‐impact mobility and morphology of lunar impact melts is surprisingly complex. We present evidence for multi‐stage influx of impact melt into flow lobes and crater floor ponds. Our volume and cooling time estimates for the post‐emplacement melt movements noted in LROC images suggest that new flows can emerge from melt ponds an extended time period after the impact event. |
| doi_str_mv | 10.1029/2010GL044666 |
| format | Article |
| fullrecord | <record><control><sourceid>proquest_cross</sourceid><recordid>TN_cdi_proquest_miscellaneous_1529950512</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>1529950512</sourcerecordid><originalsourceid>FETCH-LOGICAL-c4600-44c001493e1a285a2f95c726f3c07fe418aed4edbd592ee67f41520133f901f13</originalsourceid><addsrcrecordid>eNp9kE1PGzEQhq0KpIbAjR-wl0o9dGH8sfb6VLVREygrIkVU5WYZZ0zc7maDvRHNv8coKOqJy8wcnueV5iXknMIFBaYvGVCYNSCElPIDGVEtRFkDqCMyAtD5Zkp-JCcp_QEADpyOyNdbfC7COoXH1ZD30Bftdm1jEbqNdUPRYZtH_xDaMOwKH_uuGFZYNIt54WyH0Z6SY2_bhGdve0x-TX_cTa7KZj67nnxrSickQCmEA6BCc6SW1ZVlXldOMem5A-VR0NriUuDyYVlphiiVF7TK73DuNVBP-Zh83uduYv-0xTSYLiSHbWvX2G-TybTWFVSUZfTLHnWxTymiN5sYOht3hoJ57cn831PGP70l2-Rs66Ndu5AODuNS1lCrzLE99xxa3L2baWaLhilBIUvlXgppwH8Hyca_RiquKvP7dmbu5VRc0Z835jt_AUcWgs0</addsrcrecordid><sourcetype>Aggregation Database</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>1529950512</pqid></control><display><type>article</type><title>New insight into lunar impact melt mobility from the LRO camera</title><source>Wiley Free Content</source><source>Wiley-Blackwell AGU Digital Library</source><source>Wiley Online Library Journals Frontfile Complete</source><source>Elektronische Zeitschriftenbibliothek - Frei zugängliche E-Journals</source><creator>Bray, V. J. ; Tornabene, L. L. ; Keszthelyi, L. P. ; McEwen, A. S. ; Hawke, B. R. ; Giguere, T. A. ; Kattenhorn, S. A. ; Garry, W. B. ; Rizk, B. ; Caudill, C. M. ; Gaddis, L. R. ; van der Bogert, C. H.</creator><creatorcontrib>Bray, V. J. ; Tornabene, L. L. ; Keszthelyi, L. P. ; McEwen, A. S. ; Hawke, B. R. ; Giguere, T. A. ; Kattenhorn, S. A. ; Garry, W. B. ; Rizk, B. ; Caudill, C. M. ; Gaddis, L. R. ; van der Bogert, C. H.</creatorcontrib><description>The Lunar Reconnaissance Orbiter Camera (LROC) is systematically imaging impact melt deposits in and around lunar craters at meter and sub‐meter scales. These images reveal that lunar impact melts, although morphologically similar to terrestrial lava flows of similar size, exhibit distinctive features (e.g., erosional channels). Although generated in a single rapid event, the post‐impact mobility and morphology of lunar impact melts is surprisingly complex. We present evidence for multi‐stage influx of impact melt into flow lobes and crater floor ponds. Our volume and cooling time estimates for the post‐emplacement melt movements noted in LROC images suggest that new flows can emerge from melt ponds an extended time period after the impact event.</description><identifier>ISSN: 0094-8276</identifier><identifier>EISSN: 1944-8007</identifier><identifier>DOI: 10.1029/2010GL044666</identifier><identifier>CODEN: GPRLAJ</identifier><language>eng</language><publisher>Washington, DC: Blackwell Publishing Ltd</publisher><subject>Cameras ; Channels ; crater ; Craters ; Earth sciences ; Earth, ocean, space ; Exact sciences and technology ; flow ; impact ; Impact melts ; lava ; lunar ; Lunar spacecraft ; melt ; Melts ; Ponds</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><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c4600-44c001493e1a285a2f95c726f3c07fe418aed4edbd592ee67f41520133f901f13</citedby><cites>FETCH-LOGICAL-c4600-44c001493e1a285a2f95c726f3c07fe418aed4edbd592ee67f41520133f901f13</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%2F2010GL044666$$EPDF$$P50$$Gwiley$$H</linktopdf><linktohtml>$$Uhttps://onlinelibrary.wiley.com/doi/full/10.1029%2F2010GL044666$$EHTML$$P50$$Gwiley$$H</linktohtml><link.rule.ids>314,776,780,1411,1427,11493,27901,27902,45550,45551,46384,46443,46808,46867</link.rule.ids><backlink>$$Uhttp://pascal-francis.inist.fr/vibad/index.php?action=getRecordDetail&idt=23668087$$DView record in Pascal Francis$$Hfree_for_read</backlink></links><search><creatorcontrib>Bray, V. J.</creatorcontrib><creatorcontrib>Tornabene, L. L.</creatorcontrib><creatorcontrib>Keszthelyi, L. P.</creatorcontrib><creatorcontrib>McEwen, A. S.</creatorcontrib><creatorcontrib>Hawke, B. R.</creatorcontrib><creatorcontrib>Giguere, T. A.</creatorcontrib><creatorcontrib>Kattenhorn, S. A.</creatorcontrib><creatorcontrib>Garry, W. B.</creatorcontrib><creatorcontrib>Rizk, B.</creatorcontrib><creatorcontrib>Caudill, C. M.</creatorcontrib><creatorcontrib>Gaddis, L. R.</creatorcontrib><creatorcontrib>van der Bogert, C. H.</creatorcontrib><title>New insight into lunar impact melt mobility from the LRO camera</title><title>Geophysical research letters</title><addtitle>Geophys. Res. Lett</addtitle><description>The Lunar Reconnaissance Orbiter Camera (LROC) is systematically imaging impact melt deposits in and around lunar craters at meter and sub‐meter scales. These images reveal that lunar impact melts, although morphologically similar to terrestrial lava flows of similar size, exhibit distinctive features (e.g., erosional channels). Although generated in a single rapid event, the post‐impact mobility and morphology of lunar impact melts is surprisingly complex. We present evidence for multi‐stage influx of impact melt into flow lobes and crater floor ponds. Our volume and cooling time estimates for the post‐emplacement melt movements noted in LROC images suggest that new flows can emerge from melt ponds an extended time period after the impact event.</description><subject>Cameras</subject><subject>Channels</subject><subject>crater</subject><subject>Craters</subject><subject>Earth sciences</subject><subject>Earth, ocean, space</subject><subject>Exact sciences and technology</subject><subject>flow</subject><subject>impact</subject><subject>Impact melts</subject><subject>lava</subject><subject>lunar</subject><subject>Lunar spacecraft</subject><subject>melt</subject><subject>Melts</subject><subject>Ponds</subject><issn>0094-8276</issn><issn>1944-8007</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2010</creationdate><recordtype>article</recordtype><recordid>eNp9kE1PGzEQhq0KpIbAjR-wl0o9dGH8sfb6VLVREygrIkVU5WYZZ0zc7maDvRHNv8coKOqJy8wcnueV5iXknMIFBaYvGVCYNSCElPIDGVEtRFkDqCMyAtD5Zkp-JCcp_QEADpyOyNdbfC7COoXH1ZD30Bftdm1jEbqNdUPRYZtH_xDaMOwKH_uuGFZYNIt54WyH0Z6SY2_bhGdve0x-TX_cTa7KZj67nnxrSickQCmEA6BCc6SW1ZVlXldOMem5A-VR0NriUuDyYVlphiiVF7TK73DuNVBP-Zh83uduYv-0xTSYLiSHbWvX2G-TybTWFVSUZfTLHnWxTymiN5sYOht3hoJ57cn831PGP70l2-Rs66Ndu5AODuNS1lCrzLE99xxa3L2baWaLhilBIUvlXgppwH8Hyca_RiquKvP7dmbu5VRc0Z835jt_AUcWgs0</recordid><startdate>201011</startdate><enddate>201011</enddate><creator>Bray, V. J.</creator><creator>Tornabene, L. L.</creator><creator>Keszthelyi, L. P.</creator><creator>McEwen, A. S.</creator><creator>Hawke, B. R.</creator><creator>Giguere, T. A.</creator><creator>Kattenhorn, S. A.</creator><creator>Garry, W. B.</creator><creator>Rizk, B.</creator><creator>Caudill, C. M.</creator><creator>Gaddis, L. R.</creator><creator>van der Bogert, C. H.</creator><general>Blackwell Publishing Ltd</general><general>American Geophysical Union</general><scope>BSCLL</scope><scope>IQODW</scope><scope>AAYXX</scope><scope>CITATION</scope><scope>8FD</scope><scope>H8D</scope><scope>L7M</scope></search><sort><creationdate>201011</creationdate><title>New insight into lunar impact melt mobility from the LRO camera</title><author>Bray, V. J. ; Tornabene, L. L. ; Keszthelyi, L. P. ; McEwen, A. S. ; Hawke, B. R. ; Giguere, T. A. ; Kattenhorn, S. A. ; Garry, W. B. ; Rizk, B. ; Caudill, C. M. ; Gaddis, L. R. ; van der Bogert, C. H.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c4600-44c001493e1a285a2f95c726f3c07fe418aed4edbd592ee67f41520133f901f13</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2010</creationdate><topic>Cameras</topic><topic>Channels</topic><topic>crater</topic><topic>Craters</topic><topic>Earth sciences</topic><topic>Earth, ocean, space</topic><topic>Exact sciences and technology</topic><topic>flow</topic><topic>impact</topic><topic>Impact melts</topic><topic>lava</topic><topic>lunar</topic><topic>Lunar spacecraft</topic><topic>melt</topic><topic>Melts</topic><topic>Ponds</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Bray, V. J.</creatorcontrib><creatorcontrib>Tornabene, L. L.</creatorcontrib><creatorcontrib>Keszthelyi, L. P.</creatorcontrib><creatorcontrib>McEwen, A. S.</creatorcontrib><creatorcontrib>Hawke, B. R.</creatorcontrib><creatorcontrib>Giguere, T. A.</creatorcontrib><creatorcontrib>Kattenhorn, S. A.</creatorcontrib><creatorcontrib>Garry, W. B.</creatorcontrib><creatorcontrib>Rizk, B.</creatorcontrib><creatorcontrib>Caudill, C. M.</creatorcontrib><creatorcontrib>Gaddis, L. R.</creatorcontrib><creatorcontrib>van der Bogert, C. H.</creatorcontrib><collection>Istex</collection><collection>Pascal-Francis</collection><collection>CrossRef</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>Bray, V. J.</au><au>Tornabene, L. L.</au><au>Keszthelyi, L. P.</au><au>McEwen, A. S.</au><au>Hawke, B. R.</au><au>Giguere, T. A.</au><au>Kattenhorn, S. A.</au><au>Garry, W. B.</au><au>Rizk, B.</au><au>Caudill, C. M.</au><au>Gaddis, L. R.</au><au>van der Bogert, C. H.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>New insight into lunar impact melt mobility from the LRO camera</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>The Lunar Reconnaissance Orbiter Camera (LROC) is systematically imaging impact melt deposits in and around lunar craters at meter and sub‐meter scales. These images reveal that lunar impact melts, although morphologically similar to terrestrial lava flows of similar size, exhibit distinctive features (e.g., erosional channels). Although generated in a single rapid event, the post‐impact mobility and morphology of lunar impact melts is surprisingly complex. We present evidence for multi‐stage influx of impact melt into flow lobes and crater floor ponds. Our volume and cooling time estimates for the post‐emplacement melt movements noted in LROC images suggest that new flows can emerge from melt ponds an extended time period after the impact event.</abstract><cop>Washington, DC</cop><pub>Blackwell Publishing Ltd</pub><doi>10.1029/2010GL044666</doi><tpages>5</tpages><oa>free_for_read</oa></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_1529950512 |
| source | Wiley Free Content; Wiley-Blackwell AGU Digital Library; Wiley Online Library Journals Frontfile Complete; Elektronische Zeitschriftenbibliothek - Frei zugängliche E-Journals |
| subjects | Cameras Channels crater Craters Earth sciences Earth, ocean, space Exact sciences and technology flow impact Impact melts lava lunar Lunar spacecraft melt Melts Ponds |
| title | New insight into lunar impact melt mobility from the LRO camera |
| url | https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-02-02T09%3A01%3A14IST&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=New%20insight%20into%20lunar%20impact%20melt%20mobility%20from%20the%20LRO%20camera&rft.jtitle=Geophysical%20research%20letters&rft.au=Bray,%20V.%20J.&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/10.1029/2010GL044666&rft_dat=%3Cproquest_cross%3E1529950512%3C/proquest_cross%3E%3Curl%3E%3C/url%3E&disable_directlink=true&sfx.directlink=off&sfx.report_link=0&rft_id=info:oai/&rft_pqid=1529950512&rft_id=info:pmid/&rfr_iscdi=true |