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Composition of Earth's initial atmosphere and fate of accreted volatiles set by core formation and magma ocean redox evolution

  • Published:2024-03 Issue: Volume:629 Page:118618
  • ISSN:0012-821X
  • Container-title:Earth and Planetary Science Letters
  • language:en
  • Short-container-title:Earth and Planetary Science Letters

Author:

Gu Jesse T.ORCID,Peng BoORCID,Ji XuanORCID,Zhang JishengORCID,Yang Hong,Hoyos SusanaORCID,Hirschmann Marc M.,Kite Edwin S.,Fischer Rebecca A.

Funder

National Science Foundation

National Aeronautics and Space Administration

Publisher

Elsevier BV

Reference94 articles.

1. Early evolution of the Earth: accretion, atmosphere formation, and thermal history;Abe;J. Geophys. Res.,1986

2. Differential melt scaling for oblique impacts on terrestrial planets;Abramov;Icarus,2012

3. Volatile accretion history of the terrestrial planets and dynamic implications;Albarède;Nature,2009

4. Solidus and liquidus profiles of chondritic mantle: implication for melting of the Earth across its history;Andrault;Earth. Planet. Sci. Lett.,2011

5. Deep magma ocean formation set the oxidation state of Earth's mantle;Armstrong;Science (1979),2019

Cited by 3 articles. 订阅此论文施引文献 订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献

1. Contribution of the Moon-forming Impactor to the Volatile Inventory in the Bulk Silicate Earth;The Planetary Science Journal;2024-08-01

2. The origin and evolution of Earth's nitrogen;National Science Review;2024-05-03

3. Earth's core composition and core formation;Reference Module in Earth Systems and Environmental Sciences;2024
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