Earth’s composition was modified by collisional erosion

29/09/2022 22:05 · by karmaka · in accretion, carbonaceous chondrite, CI, CV, Earth, EH, EL, enstatite chondrite, H, L, ordinary chondrite, ungrouped

Paul Frossard, Claudine Israel, Audrey Bouvier, Maud Boyet

Science
29 Sep 2022
Vol 377, Issue 6614
pp. 1529-1532

LINK

Supplementary Materials

“The samarium-146 (146Sm)–neodymium-142 (142Nd) short-lived decay system (half-life of 103 million years) is a powerful tracer of the early mantle-crust evolution of planetary bodies. However, an increased 142Nd/144Nd in modern terrestrial rocks relative to chondrite meteorites has been proposed to be caused by nucleosynthetic anomalies, obscuring early Earth’s differentiation history. We use stepwise dissolution of primitive chondrites to quantify nucleosynthetic contributions on the composition of chondrites. After correction for nucleosynthetic anomalies, Earth and the silicate parts of differentiated planetesimals contain resolved excesses of 142Nd relative to chondrites. We conclude that only collisional erosion of primordial crusts can explain such compositions. This process associated with planetary accretion must have produced substantial loss of incompatible elements, including long-term heat-producing elements such as uranium, thorium, and potassium.”