Pressure-temperature evolution of primordial solar system solids during impact-induced compaction
Prior to becoming chondritic meteorites, primordial solids were a poorly consolidated mix of mm-scale igneous inclusions (chondrules) and high-porosity sub-μm dust (matrix). We used high-resolution numerical simulations to track the effect of impact-induced compaction on these materials. Here we sho...
| Main Authors: | , , , , , , |
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| Format: | Journal Article |
| Published: |
Nature Publishing Group
2014
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| Online Access: | http://hdl.handle.net/20.500.11937/41242 |