The paradox between low shock-stage and evidence for compaction in CM carbonaceous chondrites explained by multiple low-intensity impacts-Reference-Cited by-同舟云学术

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The paradox between low shock-stage and evidence for compaction in CM carbonaceous chondrites explained by multiple low-intensity impacts

Published:2015-01 Issue: Volume:148 Page:159-178
ISSN:0016-7037
Container-title:Geochimica et Cosmochimica Acta
language:en
Short-container-title:Geochimica et Cosmochimica Acta

Author:

Lindgren Paula,Hanna Romy D.,Dobson Katherine J.,Tomkinson Tim,Lee Martin R.

Funder

UK Science and Technology Facilities Council

UK Engineering and Physical Sciences Research Council

NASA Earth and Space Sciences Fellowship Program

Publisher

Elsevier BV

Subject

Geochemistry and Petrology

Reference77 articles.

1. The classification of CM and CR chondrites using bulk H, C and N abundances and isotopic compositions;Alexander;Geochim. Cosmochim. Acta,2013

2. Astrometric masses of 26 asteroids and observations on asteroid porosity;Baer;Astron. J.,2011

3. Matrix phyllosilicates and associated minerals in C2M carbonaceous chondrites;Barber;Geochim. Cosmochim. Acta,1981

4. Deformation twinning in calcite, dolomite, and other rhombohedral carbonates;Barber;Phys. Chem. Miner.,1979

5. Carbonates in CM2 chondrites: constraints on alteration conditions from oxygen isotopic compositions and petrographic observations;Benedix;Geochim. Cosmochim. Acta,2003

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4. Brecciation at the grain scale within the lithologies of the Winchcombe Mighei‐like carbonaceous chondrite;Meteoritics & Planetary Science;2024-04-15

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