1,721,064 research outputs found
Replication Data for: Origin of lunar fragmental matrix breccias—Highly siderophile element constraints
No full textThe dataset contains concentration data for highly siderophile elements (Ru, Rh, Pd, Re, Os, Ir, Pt, and Au) analyzed by isotope dilution inductively coupled plasma mass spectrometry. We analyzed 5 different impact breccias sampled from the rim of the North Ray Crater, during the Apollo 16 mission to the lunar highlands. All samples we allocated by NASA/JSC and analyzed in the Geochemistry Laboratories at Freie Universität Berlin, Germany. (2019-08-06), TRR 170 paper no. 7
Replication Data for: Origin of lunar fragmental matrix breccias—Highly siderophile element constraints
No full textThe dataset contains concentration data for highly siderophile elements (Ru, Rh, Pd, Re, Os, Ir, Pt, and Au) analyzed by isotope dilution inductively coupled plasma mass spectrometry. We analyzed 5 different impact breccias sampled from the rim of the North Ray Crater, during the Apollo 16 mission to the lunar highlands. All samples we allocated by NASA/JSC and analyzed in the Geochemistry Laboratories at Freie Universität Berlin, Germany. (2019-08-06), TRR 170 paper no. 7
Replication Data for: New constraints on the formation of lunar mafic impact melt breccias from S-Se-Te and highly siderophile elements.
No full textThe data set contains concentration data for chalcogens (S, Se, and Te) and highly siderophile elements (Ru, Rh, Pd, Re, Os, Ir, Pt, and Au) analyzed by isotope dilution inductively coupled plasma mass spectrometry. We analyzed 5 different impact breccias sampled from the Fra Mauro formation of the Apollo 14, the Apennine Front of the Apollo 15, and the Cayley formation of the Apollo 16 landing sites
Replication Data for: New constraints on the formation of lunar mafic impact melt breccias from S-Se-Te and highly siderophile elements.
No full textThe data set contains concentration data for chalcogens (S, Se, and Te) and highly siderophile elements (Ru, Rh, Pd, Re, Os, Ir, Pt, and Au) analyzed by isotope dilution inductively coupled plasma mass spectrometry. We analyzed 5 different impact breccias sampled from the Fra Mauro formation of the Apollo 14, the Apennine Front of the Apollo 15, and the Cayley formation of the Apollo 16 landing sites
Replication Data for: Formation of Apollo 16 impactites and the composition of late accreted material: Constraints from Os isotopes, highly siderophile elements and sulfur abundances.
No full textThe data set contains concentration data for highly siderophile elements (Ru, Rh, Pd, Re, Os, Ir, Pt, and Au) analyzed by isotope dilution inductively coupled plasma mass spectrometry. We analyzed 5 impact melt breccias sampled from the Cayley formation, during the Apollo 16 mission to the lunar highlands. All samples we allocated by NASA/JSC and analyzed in the Geochemistry Laboratories at Freie Universität Berlin, Germany
Replication Data for: Origin of lunar fragmental matrix breccias—Highly siderophile element constraints
No full textThe dataset contains concentration data for highly siderophile elements (Ru, Rh, Pd, Re, Os, Ir, Pt, and Au) analyzed by isotope dilution inductively coupled plasma mass spectrometry. We analyzed 5 different impact breccias sampled from the rim of the North Ray Crater, during the Apollo 16 mission to the lunar highlands. All samples we allocated by NASA/JSC and analyzed in the Geochemistry Laboratories at Freie Universität Berlin, Germany. (2019-08-06), TRR 170 paper no. 7
Replication Data for: Formation of Apollo 16 impactites and the composition of late accreted material: Constraints from Os isotopes, highly siderophile elements and sulfur abundances.
No full textThe data set contains concentration data for highly siderophile elements (Ru, Rh, Pd, Re, Os, Ir, Pt, and Au) analyzed by isotope dilution inductively coupled plasma mass spectrometry. We analyzed 5 impact melt breccias sampled from the Cayley formation, during the Apollo 16 mission to the lunar highlands. All samples we allocated by NASA/JSC and analyzed in the Geochemistry Laboratories at Freie Universität Berlin, Germany
Replication Data for: New constraints on the formation of lunar mafic impact melt breccias from S-Se-Te and highly siderophile elements.
No full textThe data set contains concentration data for chalcogens (S, Se, and Te) and highly siderophile elements (Ru, Rh, Pd, Re, Os, Ir, Pt, and Au) analyzed by isotope dilution inductively coupled plasma mass spectrometry. We analyzed 5 different impact breccias sampled from the Fra Mauro formation of the Apollo 14, the Apennine Front of the Apollo 15, and the Cayley formation of the Apollo 16 landing sites
Replication Data for: Formation of Apollo 16 impactites and the composition of late accreted material: Constraints from Os isotopes, highly siderophile elements and sulfur abundances.
No full textThe data set contains concentration data for highly siderophile elements (Ru, Rh, Pd, Re, Os, Ir, Pt, and Au) analyzed by isotope dilution inductively coupled plasma mass spectrometry. We analyzed 5 impact melt breccias sampled from the Cayley formation, during the Apollo 16 mission to the lunar highlands. All samples we allocated by NASA/JSC and analyzed in the Geochemistry Laboratories at Freie Universität Berlin, Germany
Replication Data for: Chalcophile elements in Martian meteorites indicate low sulfur content in the Martian interior and a volatile element-depleted late veneer.
No full text• 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
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