Shape and porosity of refractory inclusions in CV3 chondrites: A micro‐computed tomography (µCT) study-Reference-Cited by-同舟云学术

Shape and porosity of refractory inclusions in CV3 chondrites: A micro‐computed tomography (µCT) study

Published:2021-03 Issue:3 Volume:56 Page:500-514
ISSN:1086-9379
Container-title:Meteoritics & Planetary Science
language:en
Short-container-title:Meteorit Planet Sci

Author:

Zhang Mingming¹²^ORCID,Clark Brett³,King Ashley J.¹⁴^ORCID,Russell Sara S.¹^ORCID,Lin Yangting²^ORCID

Affiliation:

1. Department of Earth Sciences The Natural History Museum Cromwell Road SW7 5BD London UK

2. Key Laboratory of Earth and Planetary Physics Institute of Geology and Geophysics Chinese Academy of Sciences Beijing 100029 China

3. Core Research Laboratories The Natural History Museum Cromwell Road SW7 5BD London UK

4. School of Physical Sciences The Open University Walton Hall MK7 6AA Milton Keynes UK

Funder

Science and Technology Facilities Council

Publisher

Wiley

Subject

Space and Planetary Science,Geophysics

Link

https://onlinelibrary.wiley.com/doi/pdf/10.1111/maps.13635

Reference52 articles.

1. AlmeidaN. V. SmithC. L. SykesD. DownesH. AhmedF. andRussellS. S.2015.Quantifying the deformation of Leoville chondrules in 3D: Implications for the post‐accretional history of the CV3 parent body (abstract #1856). 78th Annual Meeting of the Meteoritical Society.Meteoritics & Planetary Science50.

2. Resolved images of a protostellar outflow driven by an extended disk wind

3. The Growth Mechanisms of Macroscopic Bodies in Protoplanetary Disks

4. Mixing in the solar nebula: Implications for isotopic heterogeneity and large-scale transport of refractory grains

5. Structural deformation of the Leoville chondrite

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