Enstatite chondrites have often been considered to be closely related to the material from which Earth accreted. However, tungsten isotopic data reveal clear differences. Moreover, the silicate and metal fractions define distinct initial 182Hf/180Hf corresponding to a 13.8 ± 5.3 million year apparent age difference, Internal reequilibration does not provide a ready explanation for this result. Larger scale redistribution of tungsten is more likely, such as may have occurred during collisions between planetesimals
The processes of planet formation in our Solar System resulted in a final product of a small number ...
International audienceHeterogeneity in isotopic compositions within the protoplanetary disc has been...
The abundances of highly siderophile elements (HSE: Re, Os, Ir, Ru, Pt, Pd), as well as 187Re-187Os ...
[[sponsorship]]地球科學研究所[[note]]已出版;[SCI];有審查制度;不具代表性[[note]]http://gateway.isiknowledge.com/gateway/G...
The short-lived Hf-182-W-182-isotope system is an ideal clock to trace core formation and accretion ...
Three ordinary chondrites, Forest Vale (H4), Ste. Marguerite (H4) and Richardton (H5) have been stud...
Tafassasset is a primitive meteorite, the origin of which is still debated. Its possible relationshi...
Abstract—The rates of accretion and core formation of the Earth and other inner solar system objects...
We examine 141 N-body simulations of terrestrial planet late-stage accretion that use the Grand Tack...
THE accretion of the Earth and Moon within the solar nebula is thought(1-3) to have taken 50 to 100 ...
We couple the results of N-body simulations of late-stage accretion (O’Brien et al. 2006) to a hafni...
International audienceThe revelation of a small 182W terrestrial excess relatively to the 182Hf–182W...
Core formation in planetesimals can, in principle, be dated using the short-lived 182Hf-182W chronom...
High-precision W isotopic compositions are presented for 35 iron meteorites from 7 magmatic groups (...
We have measured182W/184W for Eoarchean rocks from the Itsaq Gneiss Complex (3.8-3.7 Ga pillow meta-...
The processes of planet formation in our Solar System resulted in a final product of a small number ...
International audienceHeterogeneity in isotopic compositions within the protoplanetary disc has been...
The abundances of highly siderophile elements (HSE: Re, Os, Ir, Ru, Pt, Pd), as well as 187Re-187Os ...
[[sponsorship]]地球科學研究所[[note]]已出版;[SCI];有審查制度;不具代表性[[note]]http://gateway.isiknowledge.com/gateway/G...
The short-lived Hf-182-W-182-isotope system is an ideal clock to trace core formation and accretion ...
Three ordinary chondrites, Forest Vale (H4), Ste. Marguerite (H4) and Richardton (H5) have been stud...
Tafassasset is a primitive meteorite, the origin of which is still debated. Its possible relationshi...
Abstract—The rates of accretion and core formation of the Earth and other inner solar system objects...
We examine 141 N-body simulations of terrestrial planet late-stage accretion that use the Grand Tack...
THE accretion of the Earth and Moon within the solar nebula is thought(1-3) to have taken 50 to 100 ...
We couple the results of N-body simulations of late-stage accretion (O’Brien et al. 2006) to a hafni...
International audienceThe revelation of a small 182W terrestrial excess relatively to the 182Hf–182W...
Core formation in planetesimals can, in principle, be dated using the short-lived 182Hf-182W chronom...
High-precision W isotopic compositions are presented for 35 iron meteorites from 7 magmatic groups (...
We have measured182W/184W for Eoarchean rocks from the Itsaq Gneiss Complex (3.8-3.7 Ga pillow meta-...
The processes of planet formation in our Solar System resulted in a final product of a small number ...
International audienceHeterogeneity in isotopic compositions within the protoplanetary disc has been...
The abundances of highly siderophile elements (HSE: Re, Os, Ir, Ru, Pt, Pd), as well as 187Re-187Os ...