Water in the Accretion Disk: Effect of Composition and Surface Structure on the Energy of Adsorption onto Olivine Grains

Details Water in the Accretion Disk: Effect of Composition and Surface Structure on the Energy of Adsorption onto Olivine Grains Water in the Accretion Disk: Effect of Composition and Surface Structure on the Energy of Adsorption onto Olivine Grains

Mar 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007lpi....38.1183s&link_type=abstract

38th Lunar and Planetary Science Conference, (Lunar and Planetary Science XXXVIII), held March 12-16, 2007 in League City, Texas

Physics

2

Scientific paper

The surface of olivine presents a variety of bonding environments for
the adsorbed molecular water. Binding energies range from <44 kJ/mole
to >200 kJ/mole. These interactions are strong enough to retain water
on the surfaces at high temperature.

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