High-pressure metamorphic mineralogy of the Martian crust with implications for density and seismic profiles

dc.contributor.author Semprich, Julia
dc.contributor.author Filiberto, Justin
dc.contributor.author https://orcid.org/0000-0003-4398-0961
dc.contributor.author https://orcid.org/0000-0001-5058-1905
dc.coverage.spatial Mars (Planet)
dc.date.accessioned 2020-07-15T19:32:36Z
dc.date.available 2020-07-15T19:32:36Z
dc.date.issued 2020-06-22
dc.description.abstract Here, we calculate the mineralogy of the Martian lower crust and upper mantle as a function of pressure and temperature with depth using four bulk compositions (average crust, Gusev basalt, olivine-phyric shergottite, and primitive average mantle). We then use this mineralogy to extract rock properties such as density and seismic velocities, describe their changes with varying conditions and geotherms, and make predictions for the crust–mantle boundary. en
dc.format.extent 15 pages
dc.format.mimetype application/pdf
dc.identifier.citation Semprich, J. and Filiberto, J. (2020), High‐pressure metamorphic mineralogy of the Martian crust with implications for density and seismic profiles. Meteorit Planet Sci. doi:10.1111/maps.13535 en
dc.identifier.uri https://hdl.handle.net/20.500.11753/1640
dc.language.iso en en
dc.publisher The Meteoritical Society en
dc.relation.ispartofseries LPI contribution ; no. 2371
dc.rights.license This is an open access article under the terms of the Creative Commons Attribution License, which permits use, distribution and reproduction in any medium, provided the original work is properly cited.
dc.subject Mars (Planet)--Crust en
dc.title High-pressure metamorphic mineralogy of the Martian crust with implications for density and seismic profiles en
dc.type Article en
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Fig S1 : (a‐d) Calculated S‐wave velocities (km/s) overlain by mineral phase diagram for compositions as in Fig. 1 (bulk compositions in Table 1).