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dc.contributor.authorLeeuw, N.
dc.contributor.authorCatlow, C.
dc.contributor.authorKing, H.
dc.contributor.authorPutnis, Andrew
dc.contributor.authorMuralidharan, K.
dc.contributor.authorDeymier, P.
dc.contributor.authorStimpfl, M.
dc.contributor.authorDrake, M.
dc.date.accessioned2017-01-30T12:37:58Z
dc.date.available2017-01-30T12:37:58Z
dc.date.created2016-09-12T08:36:36Z
dc.date.issued2010
dc.identifier.citationLeeuw, N. and Catlow, C. and King, H. and Putnis, A. and Muralidharan, K. and Deymier, P. and Stimpfl, M. et al. 2010. Where on Earth has our water come from?. Chemical Communications. 46 (47): pp. 8923-8925.
dc.identifier.urihttp://hdl.handle.net/20.500.11937/23557
dc.identifier.doi10.1039/c0cc02312d
dc.description.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. © 2010 The Royal Society of Chemistry.

dc.publisherThe Royal Society of Chemistry
dc.titleWhere on Earth has our water come from?
dc.typeJournal Article
dcterms.source.volume46
dcterms.source.number47
dcterms.source.startPage8923
dcterms.source.endPage8925
dcterms.source.issn1359-7345
dcterms.source.titleChemical Communications
curtin.departmentDepartment of Applied Geology
curtin.accessStatusFulltext not available


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