Highly siderophile elements in Earth, Mars, the Moon, and asteroids
JMD Day, AD Brandon… - Reviews in Mineralogy …, 2016 - pubs.geoscienceworld.org
The highly siderophile elements (HSE: Os, Ir, Ru, Rh, Pt, Pd, Re, Au) are key tracers of
planetary accretion and differentiation processes due to their affinity for metal relative to …
planetary accretion and differentiation processes due to their affinity for metal relative to …
[HTML][HTML] Siderophile elements in tracing planetary formation and evolution
RJ Walker - Geochemical perspectives, 2016 - ncbi.nlm.nih.gov
The siderophile, or iron-loving elements have many applications in the Earth and planetary
sciences. In primitive meteorites, differences in the relative abundances of these elements …
sciences. In primitive meteorites, differences in the relative abundances of these elements …
Rhodium, gold and other highly siderophile element abundances in chondritic meteorites
M Fischer-Gödde, H Becker, F Wombacher - Geochimica et Cosmochimica …, 2010 - Elsevier
The abundances of the highly siderophile elements (HSE) Re, Os, Ir, Ru, Pt, Rh, Pd and Au,
and 187Os/188Os isotope ratios have been determined for a set of carbonaceous, ordinary …
and 187Os/188Os isotope ratios have been determined for a set of carbonaceous, ordinary …
Origin of felsic achondrites Graves Nunataks 06128 and 06129, and ultramafic brachinites and brachinite-like achondrites by partial melting of volatile-rich primitive …
New major-and trace-element abundances, highly siderophile element (HSE: Os, Ir, Ru, Pt,
Pd, Re) abundances, and oxygen and rhenium–osmium isotope data are reported for …
Pd, Re) abundances, and oxygen and rhenium–osmium isotope data are reported for …
Stable isotopes and the noncarbonaceous derivation of ureilites, in common with nearly all differentiated planetary materials
PH Warren - Geochimica et Cosmochimica Acta, 2011 - Elsevier
The abundant, diverse ureilite meteorites are peridotitic asteroidal mantle restites that have
remarkably high bulk carbon contents (average 3wt%) and have long been linked to the so …
remarkably high bulk carbon contents (average 3wt%) and have long been linked to the so …
Origin and provenance of spherules and magnetic grains at the Younger Dryas boundary
One or more bolide impacts are hypothesized to have triggered the Younger Dryas cooling
at∼ 12.9 ka. In support of this hypothesis, varying peak abundances of magnetic grains with …
at∼ 12.9 ka. In support of this hypothesis, varying peak abundances of magnetic grains with …
Osmium isotope evidence for a large Late Triassic impact event
Anomalously high platinum group element concentrations have previously been reported for
Upper Triassic deep-sea sediments, which are interpreted to be derived from an …
Upper Triassic deep-sea sediments, which are interpreted to be derived from an …
A 187Re-187Os, 87Rb-87Sr, highly siderophile and incompatible trace element study of some carbonaceous, ordinary and enstatite chondrite meteorites
Abstract New 187 Re-187 Os, 87 Rb-87 Sr, triple O-isotope isotope, bulk rock highly
siderophile-(HSE: Os, Ir, Ru, Pt, Pd, Re), major-and trace-element abundance data are …
siderophile-(HSE: Os, Ir, Ru, Pt, Pd, Re), major-and trace-element abundance data are …
Early metal-silicate differentiation during planetesimal formation revealed by acapulcoite and lodranite meteorites
In order to establish the role and expression of silicate-metal fractionation in early
planetesimal bodies, we have conducted a highly siderophile element (HSE: Os, Ir, Ru, Pt …
planetesimal bodies, we have conducted a highly siderophile element (HSE: Os, Ir, Ru, Pt …
Ferrous oxide-rich asteroid achondrites
JMD Day, CA Corder, N Assayag, P Cartigny - … et Cosmochimica Acta, 2019 - Elsevier
Ferrous oxide (FeO)-rich asteroid achondrites can be defined as asteroid-derived samples
that experienced incipient partial melting processes in the early Solar System (> 4.5 Ga) …
that experienced incipient partial melting processes in the early Solar System (> 4.5 Ga) …