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Physical state of an early magma ocean constrained by the thermodynamics and viscosity of iron silicate liquid

  • Published:2020-12 Issue: Volume:551 Page:116556
  • ISSN:0012-821X
  • Container-title:Earth and Planetary Science Letters
  • language:en
  • Short-container-title:Earth and Planetary Science Letters

Author:

Sun YichengORCID,Zhou Huiqun,Liu Xiandong,Yin KunORCID,Lu Xiancai

Funder

National Key R&D Program of China

National Basic Research Program of China

National Natural Science Foundation of China

China Postdoctoral Science Foundation

Fundamental Research Funds for the Central Universities

Publisher

Elsevier BV

Subject

Space and Planetary Science,Earth and Planetary Sciences (miscellaneous),Geochemistry and Petrology,Geophysics

Reference51 articles.

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

2. Mg2SiO4 liquid under high pressure from molecular dynamics;Adjaoud;Chem. Geol.,2008

3. Transport properties of Mg2SiO4 liquid at high pressure: physical state of a magma ocean;Adjaoud;Earth Planet. Sci. Lett.,2011

4. Thermal expansion of molten Fe2SiO4 at high pressure;Agee;Geophys. Res. Lett.,1992

5. Computer Simulation of Liquids;Allen,1989

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