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Long-lived magnetism from solidification-driven convection on the pallasite parent body

Author

Listed:
  • James F. J. Bryson

    (University of Cambridge, Downing Street, Cambridge CB2 3EQ, UK)

  • Claire I. O. Nichols

    (University of Cambridge, Downing Street, Cambridge CB2 3EQ, UK)

  • Julia Herrero-Albillos

    (Centro Universitario de la Defensa, Carretera de Huesca s/n, E-50090 Zaragoza, Spain
    Instituto de Ciencia de Materiales de Aragón, CSIC—Universidad de Zaragoza, Pedro Cerbuna 12, E-50009 Zaragoza, Spain)

  • Florian Kronast

    (Helmholtz-Zentrum Berlin für Materialien und Energie, Albert-Einstein-Strasse 15, 12489 Berlin, Germany)

  • Takeshi Kasama

    (Center for Electron Nanoscopy, Technical University of Denmark, DK-2800 Kongens Lyngby, Denmark)

  • Hossein Alimadadi

    (Center for Electron Nanoscopy, Technical University of Denmark, DK-2800 Kongens Lyngby, Denmark)

  • Gerrit van der Laan

    (Diamond Light Source, Chilton, Didcot, Oxfordshire OX11 0DE, UK)

  • Francis Nimmo

    (University of California)

  • Richard J. Harrison

    (University of Cambridge, Downing Street, Cambridge CB2 3EQ, UK)

Abstract

Nanomagnetic imaging has been used to obtain a palaeomagnetic time series of two pallasite meteorites, revealing that their convection was driven by core solidification, which would have caused long-lived magnetic fields in the cores of early Solar System planetary bodies.

Suggested Citation

  • James F. J. Bryson & Claire I. O. Nichols & Julia Herrero-Albillos & Florian Kronast & Takeshi Kasama & Hossein Alimadadi & Gerrit van der Laan & Francis Nimmo & Richard J. Harrison, 2015. "Long-lived magnetism from solidification-driven convection on the pallasite parent body," Nature, Nature, vol. 517(7535), pages 472-475, January.
  • Handle: RePEc:nat:nature:v:517:y:2015:i:7535:d:10.1038_nature14114
    DOI: 10.1038/nature14114
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