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Hollows on Mercury: MESSENGER Evidence for Geologically Recent Volatile-Related Activity

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dc.contributor.author Blewett, David T. en
dc.contributor.author Chabot, Nancy L. en
dc.contributor.author Denevi, Brett W. en
dc.contributor.author Ernst, Carolyn M. en
dc.contributor.author Head, James W. en
dc.contributor.author Izenberg, Noam R. en
dc.contributor.author Murchie, Scott L. en
dc.contributor.author Solomon, Sean C. en
dc.contributor.author Nittler, Larry R. en
dc.contributor.author McCoy, Timothy J. en
dc.contributor.author Xiao, Zhiyong en
dc.contributor.author Baker, David M. H. en
dc.contributor.author Fassett, Caleb I. en
dc.contributor.author Braden, Sarah E. en
dc.contributor.author Oberst, Juergen en
dc.contributor.author Scholten, Frank en
dc.contributor.author Preusker, Frank en
dc.contributor.author Hurwitz, Debra M. en
dc.date.accessioned 2013-04-09T19:33:16Z
dc.date.available 2013-04-09T19:33:16Z
dc.date.issued 2011
dc.identifier.citation Blewett, David T., Chabot, Nancy L., Denevi, Brett W., Ernst, Carolyn M., Head, James W., Izenberg, Noam R., Murchie, Scott L., Solomon, Sean C., Nittler, Larry R., McCoy, Timothy J., Xiao, Zhiyong, Baker, David M. H., Fassett, Caleb I., Braden, Sarah E., Oberst, Juergen, Scholten, Frank, Preusker, Frank, and Hurwitz, Debra M. 2011. "<a href="https%3A%2F%2Frepository.si.edu%2Fhandle%2F10088%2F20452">Hollows on Mercury: MESSENGER Evidence for Geologically Recent Volatile-Related Activity</a>." <em>Science</em>. 333 (6051):1856&ndash;1859. <a href="https://doi.org/10.1126/science.1211681">https://doi.org/10.1126/science.1211681</a> en
dc.identifier.issn 0036-8075
dc.identifier.uri http://hdl.handle.net/10088/20452
dc.description.abstract High-resolution images of Mercury&#39;s surface from orbit reveal that many bright deposits within impact craters exhibit fresh-appearing, irregular, shallow, rimless depressions. The depressions, or hollows, range from tens of meters to a few kilometers across, and many have high-reflectance interiors and halos. The host rocks, which are associated with crater central peaks, peak rings, floors, and walls, are interpreted to have been excavated from depth by the crater-forming process. The most likely formation mechanisms for the hollows involve recent loss of volatiles through some combination of sublimation, space weathering, outgassing, or pyroclastic volcanism. These features support the inference that Mercury&#39;s interior contains higher abundances of volatile materials than predicted by most scenarios for the formation of the solar system&#39;s innermost planet. en
dc.relation.ispartof Science en
dc.title Hollows on Mercury: MESSENGER Evidence for Geologically Recent Volatile-Related Activity en
dc.type Journal Article en
dc.identifier.srbnumber 103108
dc.identifier.doi 10.1126/science.1211681
rft.jtitle Science
rft.volume 333
rft.issue 6051
rft.spage 1856
rft.epage 1859
dc.description.SIUnit NH-Mineral Sciences en
dc.description.SIUnit NMNH en
dc.description.SIUnit Peer-Reviewed en
dc.citation.spage 1856
dc.citation.epage 1859

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