dc.contributor
TRR170-DB, Freie Universität Berlin, Germany
dc.contributor
Becker, Harry
dc.date.accessioned
2023-05-23T15:19:56Z
dc.date.available
2023-05-23T15:19:56Z
dc.identifier
https://doi.org/10.35003/BMFSHW
dc.identifier.uri
https://refubium.fu-berlin.de/handle/fub188/39445
dc.identifier.uri
http://dx.doi.org/10.17169/refubium-39162
dc.description
• Ratios of Cu, S, Se, Te, Re, Pt and Pd in Martian meteorites are relatively constant.
• Martian meteorites show very limited eruptive losses of volatile Re, S, Se and Te.
• The parent magmas of most Martian meteorites were sulfide-undersaturated.
• Martian mantle and core have a low sulfur content.
• Low Te/PGE ratios in Martian meteorites reflect a strongly volatile element-depleted Martian late veneer.
dc.subject
chalcophile elements
dc.subject
Martian mantle
dc.title
Replication Data for: Chalcophile elements in Martian meteorites indicate low sulfur content in the Martian interior and a volatile element-depleted late veneer.
dcterms.accessRights.openaire
metadata only access
