Sephton, M. A.; Howard, L. E.; Bland, P. A.; James, R. H.; Russell, S. S.; Prior, D. J. and Zolensky, M. E.
|DOI (Digital Object Identifier) Link:||http://dx.doi.org/10.1111/j.1468-4004.2006.47637.x|
|Google Scholar:||Look up in Google Scholar|
Meteorites such as Allende - type III carbonaceous chondrites - contain strange dark clasts that would have been formed as part of early planet-forming processes in the early solar system. Opinion has been divided for years on the provenance of these components. Formation of source materials in the protoplanetary disc, impact-induced fragmentation of the parent asteroid or complex aqueous and thermal histories have all been suggested. We describe new analytical approaches that have cast light on these dark objects and their origins.
|Item Type:||Journal Article|
|Copyright Holders:||2006 Royal Astronomical Society|
|Academic Unit/Department:||Science > Environment, Earth and Ecosystems
|Interdisciplinary Research Centre:||Centre for Earth, Planetary, Space and Astronomical Research (CEPSAR)|
|Depositing User:||Users 8955 not found.|
|Date Deposited:||06 May 2009 13:42|
|Last Modified:||15 Jan 2016 11:16|
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