Percolative sulfide core formation in oxidized planetary bodies

Percolative sulfide core formation in oxidized planetary bodies

Abstract Models of planetary core formation traditionally involve the fractionation of Fe,Ni-metal melts from silicate mantles after extensive silicate melting. However, in planetary bodies that form farther from their central star, where moderately volatile elements are more abundant, high concentr...

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Bibliographic Details
Main Authors: Samuel D. Crossley, Jacob B. Setera, Brendan A. Anzures, Kayla Iacovino, Wayne P. Buckley, Scott A. Eckley, Evan W. O’Neal, Jessica A. Maisano, Justin I. Simon, Kevin Righter
Format: Article
Language:English
Published: Nature Portfolio 2025-04-01
Series:Nature Communications
Online Access:https://doi.org/10.1038/s41467-025-58517-8
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