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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 15501

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 `{}`	In comparison, bulk silicate Mars reflects 27 ± 5% pebble-accreted material and 73 ± 5% Vesta-like planetesimals.

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