Numerous chondritic impactors and oxidized magma ocean set Earth's volatile depletion
Haruka Sakuraba, Hiroyuki Kurokawa, Hidenori Genda, and Kenji Ohta

TL;DR
This study models Earth's volatile element depletion through accretion, showing that chondritic impactors combined with specific oxidation and impact conditions can explain the observed C, N, and H distribution in Earth's interior.
Contribution
It demonstrates that Earth's volatile depletion pattern can be explained by continuous accretion of chondritic bodies with specific oxidation states and impact conditions, without requiring non-chondritic sources.
Findings
Depletion pattern reproduced by impact partitioning and erosion.
Oxidized magma ocean essential for volatile distribution.
Small impactors dominate late-stage accretion.
Abstract
Earth's surface environment is largely influenced by its budget of major volatile elements: carbon (C), nitrogen (N), and hydrogen (H). Although the volatiles on Earth are thought to have been delivered by chondritic materials, the elemental composition of the bulk silicate Earth (BSE) shows depletion in the order of N, C, and H. Previous studies have concluded that non-chondritic materials are needed for this depletion pattern. Here, we model the evolution of the volatile abundances in the atmosphere, oceans, crust, mantle, and core through the accretion history by considering elemental partitioning and impact erosion. We show that the BSE depletion pattern can be reproduced from continuous accretion of chondritic bodies by the partitioning of C into the core and H storage in the magma ocean in the main accretion stage and atmospheric erosion of N in the late accretion stage. This…
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