{
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"name": "New insight into lunar impact melt mobility from the LRO camera",
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"value": "70047291",
"url": "https://pubs.usgs.gov/publication/70047291"
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"value": "10.1029/2010GL044666",
"url": "https://doi.org/10.1029/2010GL044666"
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"name": "Geophysical Research Letters",
"volumeNumber": "37",
"issueNumber": "21"
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"datePublished": "2010",
"dateModified": "2018-11-07",
"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.",
"description": "L21202; 5 p.",
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