| Literature DB >> 20967372 |
Nora H de Leeuw1, C Richard A Catlow, Helen E King, Andrew Putnis, Krishna Muralidharan, Pierre Deymier, Marilena Stimpfl, Michael J Drake.
Abstract
The presence of water in the Earth has long been an enigma. However, computer modelling techniques have shown that the adsorption of water onto the fractal surfaces of interplanetary dust particles, which are present in the planetary accretion disk, is sufficiently strong to provide a viable origin of terrestrial water.Entities:
Year: 2010 PMID: 20967372 DOI: 10.1039/c0cc02312d
Source DB: PubMed Journal: Chem Commun (Camb) ISSN: 1359-7345 Impact factor: 6.222