A Time‐Resolved Paleomagnetic Record of Main Group Pallasites: Evidence for a Large‐Cored, Thin‐Mantled Parent Body-Reference-Cited by-同舟云学术

A Time‐Resolved Paleomagnetic Record of Main Group Pallasites: Evidence for a Large‐Cored, Thin‐Mantled Parent Body

Published:2021-07 Issue:7 Volume:126 Page:
ISSN:2169-9097
Container-title:Journal of Geophysical Research: Planets
language:en
Short-container-title:J Geophys Res Planets

Author:

Nichols Claire I. O.¹²^ORCID,Bryson James F. J.²,Cottrell Rory D.³^ORCID,Fu Roger R.⁴^ORCID,Harrison Richard J.⁵^ORCID,Herrero‐Albillos Julia⁶⁷^ORCID,Kronast Florian⁸,Tarduno John A.³^ORCID,Weiss Benjamin P.¹^ORCID

Affiliation:

1. Department of Earth, Atmospheric and Planetary Sciences Massachusetts Institute of Technology Cambridge MA USA

2. Department of Earth Sciences University of Oxford Oxford UK

3. Department of Earth and Environmental Sciences University of Rochester Rochester NY USA

4. Department of Earth and Planetary Sciences Harvard University Cambridge MA USA

5. Department of Earth Sciences University of Cambridge Cambridge UK

6. Departamento de Ciencia y Tecnología de Materiales y Fluidos Universidad de Zaragoza Zaragoza Spain

7. Instituto de Nanociencia y Materiales de Aragón (INMA) CSIC—Universidad de Zaragoza Zaragoza Spain

8. Helmholtz‐Zentrum Berlin für Materialien und Energie Berlin Germany

Funder

FP7 Ideas: European Research Council

Simons Foundation

National Aeronautics and Space Administration

Royal Astronomical Society

Publisher

American Geophysical Union (AGU)

Subject

Space and Planetary Science,Earth and Planetary Sciences (miscellaneous),Geochemistry and Petrology,Geophysics

Link

https://onlinelibrary.wiley.com/doi/pdf/10.1029/2021JE006900

Reference55 articles.

1. Modelling the palaeo-evolution of the geodynamo

2. A petrological and chemical reexamination of Main Group pallasite formation

3. Intrinsic oxygen fugacity measurements on seven chondrites, a pallasite, and a tektite and the redox state of meteorite parent bodies

4. Nanomagnetic intergrowths in Fe–Ni meteoritic metal: The potential for time-resolved records of planetesimal dynamo fields

5. Constraints on asteroid magnetic field evolution and the radii of meteorite parent bodies from thermal modelling

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