Thermal and chemical evolution of the terrestrial magma ocean

Details Thermal and chemical evolution of the terrestrial magma ocean Thermal and chemical evolution of the terrestrial magma ocean

Mar 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997pepi..100...27a&link_type=abstract

Physics of the Earth and Planetary Interiors, v. 100, p. 27-39.

Physics

57

Scientific paper

The Earth is likely to have experienced a magma ocean stage during accretion. Thermal and chemical evolution of magma ocean is investigated based on a one-dimensional two-phase-flow heat and mass transfer model. Differentiation at lower mantle pressure depends on the type of magma ocean and surrounding atmosphere. If the magma ocean is formed by the blanketing effect of a solar-type proto-atmosphere, extensive differentiation proceeds at lower mantle pressure. If the magma ocean is formed by the blanketing effect of an impact-induced steam atmosphere, no differentiation at lower mantle pressure is likely. If a very deep magma ocean is formed by a giant impact, whether differentiation proceeds at lower mantle pressure or not depends on grain size, viscosity of melt and/or properties of a transient atmosphere. On the contrary, chemical differentiation likely proceeds at upper mantle pressure irrespective of magma ocean type. A shallow magma ocean can remain for 100 ~ 200 My without any heating processes.

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