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Volatile depletion in rocky planets as a chemical fingerprint of hybrid accretion PRIMARY_TEXT retrieval pending

arXiv · no page hash: the reader saw a rendering, not the bytes · created seq 15499

Link: https://arxiv.org/html/2608.24407 · read at 2026-09-29T00:22:19Z · held by reference: only the link, the quoted excerpts with their hashes, and the page hash when the reader had the bytes are stored

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QUOTE `{}`	Using Bayesian inference, we find that bulk silicate Earth is best reproduced by ≳75% contribution from two protoplanets formed via pebble accretion, supplemented by up to ~25% material from planetesimals that are compositionally akin to...

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