1,720,973 research outputs found
The Earth-Moon late-accretion conundrum
No full textNature Geoscience, News & Views, Published: 19 August 2019 // The Earth–Moon late-accretion conundrum: The distribution of iron-loving elements between the mantles of the Moon and Earth may differ from established belief, suggest two studies that determine the hafnium–tungsten ratio and sulfide–silicate melt partitioning of elements in the lunar mantle.// Nature Geoscience volume 12, pages 683–684(2019) (2019)
The Earth-Moon late-accretion conundrum
No full textNature Geoscience, News & Views, Published: 19 August 2019 // The Earth–Moon late-accretion conundrum: The distribution of iron-loving elements between the mantles of the Moon and Earth may differ from established belief, suggest two studies that determine the hafnium–tungsten ratio and sulfide–silicate melt partitioning of elements in the lunar mantle.// Nature Geoscience volume 12, pages 683–684(2019) (2019)
The Earth-Moon late-accretion conundrum
No full textNature Geoscience, News & Views, Published: 19 August 2019 // The Earth–Moon late-accretion conundrum: The distribution of iron-loving elements between the mantles of the Moon and Earth may differ from established belief, suggest two studies that determine the hafnium–tungsten ratio and sulfide–silicate melt partitioning of elements in the lunar mantle.// Nature Geoscience volume 12, pages 683–684(2019) (2019)
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: 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: 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
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