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Journal article

Microstructural and paleomagnetic insight into the cooling history of the IAB parent body

Abstract:

The IABs represent one of only two groups of iron meteorites that did not form by fractional crystallization of liquid Fe-Ni in the core of a differentiated planetesimal. Instead, they are believed to originate from a partially differentiated body that was severely disrupted by one or more impacts during its early history. We present a detailed microstructural and paleomagnetic study of the Odessa and Toluca IAB meteorites, with a view to further constraining the complex history of the IAB pa...

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Publication status:
Published
Peer review status:
Peer reviewed

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Publisher copy:
10.1016/j.gca.2018.03.009

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Institution:
University of Oxford
Division:
MPLS
Department:
Earth Sciences
Role:
Author
Publisher:
Elsevier
Journal:
Geochimica et Cosmochimica Acta More from this journal
Volume:
229
Pages:
1-19
Publication date:
2018-03-15
Acceptance date:
2018-03-07
DOI:
ISSN:
0016-7037
Language:
English
Keywords:
Pubs id:
1123736
Local pid:
pubs:1123736
Deposit date:
2020-08-06

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