CORDIS Project
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This project aims to integrate astrophysical and geochemical models to understand the formation and evolution of terrestrial planets in our Solar System. By studying the processes of planetary accretion and core formation, the research seeks to reveal how these planets developed both physically and chemically over bill…
Formation of the Earth and the other terrestrial planets of our Solar System (Mercury, Venus and Mars) commenced 4.568 billion years ago and occurred on a time scale of about 100 million years.
These planets grew by the process of accretion, which involved numerous collisions with smaller (Moon- to Mars-size) bodies.
Impacts with such bodies released sufficient energy to cause large-scale melting and the formation of deep “magma oceans”.
Such magma oceans enabled liquid metal to separate from li…
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