New insight into lunar impact melt mobility from the LRO camera

V. J. Bray; L. L. Tornabene; L. P. Keszthelyi; A. S. McEwen; B. R. Hawke; T. A. Giguere; S. A. Kattenhorn; W. B. Garry; B. Rizk; C. M. Caudill; L. R. Gaddis; C. H. Van Der Bogert

doi:10.1029/2010GL044666

New insight into lunar impact melt mobility from the LRO camera

V. J. Bray, L. L. Tornabene, L. P. Keszthelyi, A. S. McEwen, B. R. Hawke, T. A. Giguere, S. A. Kattenhorn, W. B. Garry, B. Rizk, C. M. Caudill, L. R. Gaddis, C. H. Van Der Bogert

Research output: Contribution to journal › Article › peer-review

84 Scopus citations

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.

Original language	English (US)
Article number	L21202
Journal	Geophysical Research Letters
Volume	37
Issue number	21
DOIs	https://doi.org/10.1029/2010GL044666
State	Published - Nov 1 2010

ASJC Scopus subject areas

Geophysics
General Earth and Planetary Sciences

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10.1029/2010GL044666

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title = "New insight into lunar impact melt mobility from the LRO camera",

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.",

author = "Bray, {V. J.} and Tornabene, {L. L.} and Keszthelyi, {L. P.} and McEwen, {A. S.} and Hawke, {B. R.} and Giguere, {T. A.} and Kattenhorn, {S. A.} and Garry, {W. B.} and B. Rizk and Caudill, {C. M.} and Gaddis, {L. R.} and {Van Der Bogert}, {C. H.}",

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T1 - New insight into lunar impact melt mobility from the LRO camera

AU - Bray, V. J.

AU - Tornabene, L. L.

AU - Keszthelyi, L. P.

AU - McEwen, A. S.

AU - Hawke, B. R.

AU - Giguere, T. A.

AU - Kattenhorn, S. A.

AU - Garry, W. B.

AU - Rizk, B.

AU - Caudill, C. M.

AU - Gaddis, L. R.

AU - Van Der Bogert, C. H.

PY - 2010/11/1

Y1 - 2010/11/1

N2 - 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.

AB - 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.

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New insight into lunar impact melt mobility from the LRO camera

Abstract

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