Impact-induced compaction of primitive solar system solids: The need for mesoscale modelling and experiments

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Impact-induced compaction of primitive solar system solids: The need for mesoscale modelling and experiments

Primitive solar system solids were accreted as highly porous bimodal mixtures of mm-sized chondrules and sub-µm matrix grains. To understand the compaction and lithification of these materials by shock, it is necessary to investigate the process at the mesoscale; i.e., the scale of individual chondr...

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Bibliographic Details
Main Authors:	Davison, T., Derrick, J., Collins, G., Bland, Phil, Rutherford, M., Chapman, D., Eakins, D.
Format:	Journal Article
Published:	2017
Online Access:	http://hdl.handle.net/20.500.11937/65622

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