Conditions on Early Earth
Faraday Disk Dynamo
Sulfur Assimilation
The Sulfur Cycle
Energetics of Solution Formation
Magnetism
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Updated: Dec 27, 2025

Simulation of the Planetary Interior Differentiation Processes in the Laboratory
Published on: November 15, 2013
Lars Stixrude1,2, Roberto Scipioni3, Michael P Desjarlais4
1Department of Earth, Planetary, and Space Sciences, University of California, Los Angeles, CA, 90095, USA. lstixrude@epss.ucla.edu.
The early Earth's magnetic field was generated by its basal magma ocean. High electrical conductivity in this molten silicate layer, simulated under extreme pressure and temperature, supports dynamo theory for the ancient magnetic field.
11:50Metal-silicate Partitioning at High Pressure and Temperature: Experimental Methods and a Protocol to Suppress Highly Siderophile Element Inclusions
Published on: June 13, 2015
06:29Simulation of Early Earth Hydrothermal Chimneys in a Thermal Gradient Environment
Published on: February 27, 2021
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