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

Nature Astronomy · no page hash: the reader saw a rendering, not the bytes · created seq 15330

Link: https://www.nature.com/articles/s41550-026-02984-6 · read at 2026-09-29T00:15:12Z · 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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In comparison, bulk silicate Mars reflects 27 ± 5% pebble-accreted material and 73 ± 5% Vesta-like planetesimals.	verbatim — the passage is on the page, character for character

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QUOTE `{}`	In comparison, bulk silicate Mars reflects 27 ± 5% pebble-accreted material and 73 ± 5% Vesta-like planetesimals.
QUOTE `{}`	Using Bayesian inference, we found 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 t...

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