Articolo in rivista, 2017, ENG, 10.1038/nature23899
Hin, Remco C.; Coath, Christopher D.; Carter, Philip J.; Nimmo, Francis; Lai, Yi Jen; Pogge von Strandmann, Philip A.E.; Willbold, Matthias; Leinhardt, Zoë M.; Walter, Michael J.; Elliott, Tim
Georg-August-Universität Göttingen; University of California, Santa Cruz; University College London; University of Bristol; Macquarie University; University of California, Davis; Birkbeck, University of London
It has long been recognized that Earth and other differentiated planetary bodies are chemically fractionated compared to primitive, chondritic meteorites and, by inference, the primordial disk from which they formed. However, it is not known whether the notable volatile depletions of planetary bodies are a consequence of accretion or inherited from prior nebular fractionation. The isotopic compositions of the main constituents of planetary bodies can contribute to this debate. Here we develop an analytical approach that corrects a major cause of measurement inaccuracy inherent in conventional methods, and show that all differentiated bodies have isotopically heavier magnesium compositions than chondritic meteorites. We argue that possible magnesium isotope fractionation during condensation of the solar nebula, core formation and silicate differentiation cannot explain these observations. However, isotopic fractionation between liquid and vapour, followed by vapour escape during accretionary growth of planetesimals, generates appropriate residual compositions. Our modelling implies that the isotopic compositions of magnesium, silicon and iron, and the relative abundances of the major elements of Earth and other planetary bodies, are a natural consequence of substantial (about 40 per cent by mass) vapour loss from growing planetesimals by this mechanism.
Nature (Lond.) 549 , pp. 511–527
magnesium isotopes, planet formation, vapour loss
ID: 490684
Year: 2017
Type: Articolo in rivista
Creation: 2023-12-27 10:36:25.000
Last update: 2024-01-26 15:20:51.000
CNR authors
CNR institutes
External links
OAI-PMH: Dublin Core
OAI-PMH: Mods
OAI-PMH: RDF
DOI: 10.1038/nature23899
URL: http://www.scopus.com/record/display.url?eid=2-s2.0-85040632682&origin=inward
External IDs
CNR OAI-PMH: oai:it.cnr:prodotti:490684
DOI: 10.1038/nature23899
Scopus: 2-s2.0-85040632682