Atomistic Simulations of Adsorption of Water onto Forsterite and Fayalite Planar Surfaces: Implication for the Origin of Water in the Inner Solar System

Details Atomistic Simulations of Adsorption of Water onto Forsterite and Fayalite Planar Surfaces: Implication for the Origin of Water in the Inner Solar System Atomistic Simulations of Adsorption of Water onto Forsterite and Fayalite Planar Surfaces: Implication for the Origin of Water in the Inner Solar System

Mar 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010lpi....41.2493s&link_type=abstract

41st Lunar and Planetary Science Conference, held March 1-5, 2010 in The Woodlands, Texas. LPI Contribution No. 1533, p.2493

Physics

Scientific paper

Using atomistic and electronic structure calculations, it is shown that
adsorption is a significant source of terrestrial planetary water.

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