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dc.contributor.authorTrulove, Susanen
dc.coverage.spatialBlacksburg, Va.en
dc.date.accessioned2015-10-29T21:30:19Zen
dc.date.available2015-10-29T21:30:19Zen
dc.date.issued2008-03-27en
dc.identifier.urihttp://hdl.handle.net/10919/60960en
dc.description.abstractPatterns of scalloped-edged cliffs or lobate scarps on Mercury's surface are thrust faults that are consistent with the planet shrinking and cooling with time. However, compression occurred in the planet's early history and Mariner 10 images revealed decades ago that lobate scarps are among the youngest features on Mercury. Why don't we find more evidence of older compressive features?en
dc.format.mimetypetext/htmlen
dc.publisherVirginia Tech. University Relationsen
dc.rightsIn Copyrighten
dc.rights.urihttp://rightsstatements.org/vocab/InC/1.0/en
dc.subjectResearchen
dc.titleMercury's shifting, rolling pasten
dc.typePress releaseen
dc.rights.holderVirginia Tech. University Relationsen
dc.type.dcmitypeTexten


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