Classifying Matter by Composition
Magnetic Susceptibility and Permeability
Theory of Metallic Conduction
Magnetostatic Boundary Conditions
Equation of State
Fluid Mosaic Model
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Updated: Apr 29, 2026

Simulation of the Planetary Interior Differentiation Processes in the Laboratory
Published on: November 15, 2013
James Badro1, Alexander S Côté2, John P Brodholt3
1Institut de Physique du Globe de Paris, Sorbonne Paris Cité-Université Paris Diderot, Unité Mixte de Recherche 7154, Centre National de la Recherche Scientifique, 75005 Paris, France;Earth and Planetary Sciences Laboratory, École Polytechnique Fédérale de Lausanne, CH-1015 Lausanne, Switzerland; and badro@ipgp.fr.
Earth's core contains light elements like oxygen, silicon, carbon, and sulfur. Simulations show oxygen is essential for the outer core's composition, suggesting high-pressure, high-temperature core formation.
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Published on: June 13, 2015
06:06Sediment Core Extrusion Method at Millimeter Resolution Using a Calibrated, Threaded-rod
Published on: August 17, 2016
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