We conducted isotopic model calculations and high-pressure melting experiments in order to estimate the major element composition of the “missing reservoir”, which is a supposed component that should compensate the difference in ¹⁴²Nd/¹⁴⁴Nd ratio between the bulk silicate Earth and carbonaceous chondrite, from which the Earth is assumed to have formed. Our estimation demonstrated that the missing reservoir should have picritic to komatiitic composition, and that it was likely to have been lost from the Earth's surface by a giant impact event at the last stage of the Earth formation
The degree to which efficient mixing of new material or losses of earlier accreted material to space...
New high-precision samarium-neodymium isotopic data for chondritic meteorites show that their 142Nd/...
International audienceThe first 100 Myr of Earth’s history was marked by accretion and core...
The Accessible Silicate Earth (ASE) has a higher 142Nd/144Nd ratio than most chondrites. Thus, if th...
International audienceEarly in the Solar System's history, energetic collisions of differentiated bo...
Recent geochemical evidence based on the ^(146)Sm–^(142)Nd system and Hadean zircons shows that the ...
The Earth formed over tens of millions of years from an unknown number of stochastic collisions with...
Primitive meteorites preserve the chemical and isotopic composition of the first aggregates that for...
International audienceThe compositions of Earth materials are strikingly similar to those of enstati...
The fractionation of stable isotopes at high temperatures offers a unique insight into the sources a...
International audienceThe revelation of a small 182W terrestrial excess relatively to the 182Hf–182W...
The Earth formed in a swarm of Moon- to Mars-sized objects that collided together to build our plane...
A theoretical simulation on the process by which the hydrogen isotope differentiation took place in ...
International audienceKnowing the isotopic composition of Theia, the proto-planet which collided wit...
This study uses high precision chromium (Cr) isotope measurements to provide insights into the compo...
The degree to which efficient mixing of new material or losses of earlier accreted material to space...
New high-precision samarium-neodymium isotopic data for chondritic meteorites show that their 142Nd/...
International audienceThe first 100 Myr of Earth’s history was marked by accretion and core...
The Accessible Silicate Earth (ASE) has a higher 142Nd/144Nd ratio than most chondrites. Thus, if th...
International audienceEarly in the Solar System's history, energetic collisions of differentiated bo...
Recent geochemical evidence based on the ^(146)Sm–^(142)Nd system and Hadean zircons shows that the ...
The Earth formed over tens of millions of years from an unknown number of stochastic collisions with...
Primitive meteorites preserve the chemical and isotopic composition of the first aggregates that for...
International audienceThe compositions of Earth materials are strikingly similar to those of enstati...
The fractionation of stable isotopes at high temperatures offers a unique insight into the sources a...
International audienceThe revelation of a small 182W terrestrial excess relatively to the 182Hf–182W...
The Earth formed in a swarm of Moon- to Mars-sized objects that collided together to build our plane...
A theoretical simulation on the process by which the hydrogen isotope differentiation took place in ...
International audienceKnowing the isotopic composition of Theia, the proto-planet which collided wit...
This study uses high precision chromium (Cr) isotope measurements to provide insights into the compo...
The degree to which efficient mixing of new material or losses of earlier accreted material to space...
New high-precision samarium-neodymium isotopic data for chondritic meteorites show that their 142Nd/...
International audienceThe first 100 Myr of Earth’s history was marked by accretion and core...