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Accretion, differentiation of early planetary bodies as recorded in the composition of the silicate Earth · 2021 · arXiv 2021.114497

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Oxidation Constraints on Terrestrial Planet Formation from a Ring

astro-ph.EP · 2026-05-29 · unverdicted · novelty 6.0

Narrow-ring accretion models for terrestrial planets cannot reproduce bulk silicate Earth composition because embryos mix reduced and oxidized planetesimals early, requiring segregated reservoirs and late oxidized delivery.

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  • Oxidation Constraints on Terrestrial Planet Formation from a Ring astro-ph.EP · 2026-05-29 · unverdicted · none · ref 27

    Narrow-ring accretion models for terrestrial planets cannot reproduce bulk silicate Earth composition because embryos mix reduced and oxidized planetesimals early, requiring segregated reservoirs and late oxidized delivery.