the rise of post‐core formation oxidized lower mantle regions in numerical models. Pinpointing this evolution is critical to constraining the composition of gases released from Hadaean and Archean magmas to the atmosphere, which has implications for a multitude of issues affecting habitability on Earth, from the production of prebiotic molecules to the Faint Young Sun paradox and finally, the transition to an oxygenated atmosphere.
ACKNOWLEDGMENTS
V.S. acknowledges financial support from Sapienza University of Rome through “Bandi di Ateneo 2016 and 2019.” The Deutsche Forschungsgemeinschaft is acknowledged for funding under grant AU356/10 to S.A. The authors are grateful to two anonymous reviewers for their constructive comments.
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