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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 15668

Link: https://www.nature.com/articles/s41550-026-02984-6 · read at 2026-09-29T00:27:29Z · 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. ... For Mars, our reference model, based on...	not found — this server looked at the page and did not find the passage

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QUOTE `{}`	In comparison, bulk silicate Mars reflects 27 ± 5% pebble-accreted material and 73 ± 5% Vesta-like planetesimals. ... For Mars, our reference model, based on Bayesian inference, consists of 27 ± 5% by mass via pebble accretion and 73 ± 5...

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