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dc.contributor.authorBland, Phil
dc.contributor.authorJackson, M.
dc.contributor.authorCoker, R.
dc.contributor.authorCohen, B.
dc.contributor.authorWebber, J.B.
dc.contributor.authorLee, M.
dc.contributor.authorDuffy, C.
dc.contributor.authorChater, R.
dc.contributor.authorArdakani, M.
dc.contributor.authorMcPhail, D.
dc.contributor.authorMcComb, D.
dc.contributor.authorBenedix, Gretchen
dc.date.accessioned2017-01-30T14:55:29Z
dc.date.available2017-01-30T14:55:29Z
dc.date.created2014-11-19T01:13:27Z
dc.date.issued2009
dc.identifier.citationBland, P. and Jackson, M. and Coker, R. and Cohen, B. and Webber, J.B. and Lee, M. and Duffy, C. et al. 2009. Why aqueous alteration in asteroids was isochemical: High porosity [not equal] high permeability. Earth and Planetary Science Letters. 287 (3-4): pp. 559-568.
dc.identifier.urihttp://hdl.handle.net/20.500.11937/41816
dc.publisherElsevier Science BV
dc.titleWhy aqueous alteration in asteroids was isochemical: High porosity [not equal] high permeability
dc.typeJournal Article
dcterms.source.volume287
dcterms.source.number3-4
dcterms.source.startPage559
dcterms.source.endPage568
dcterms.source.issn0012821X
dcterms.source.titleEarth and Planetary Science Letters
curtin.accessStatusFulltext not available


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