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The end of the lunar dynamo.
Mighani, Saied; Wang, Huapei; Shuster, David L; Borlina, Cauȇ S; Nichols, Claire I O; Weiss, Benjamin P.
Afiliación
  • Mighani S; Department of Earth, Atmospheric, and Planetary Sciences, Massachusetts Institute of Technology (MIT), 77 Massachusetts Avenue, Cambridge, MA 02139, USA.
  • Wang H; Department of Earth, Atmospheric, and Planetary Sciences, Massachusetts Institute of Technology (MIT), 77 Massachusetts Avenue, Cambridge, MA 02139, USA.
  • Shuster DL; School of Earth Sciences, China University of Geosciences (Wuhan), 388 Lumo Road, Wuhan, Hubei 430074, P. R. China.
  • Borlina CS; Department of Earth and Planetary Science, University of California, Berkeley, Berkeley, CA 94720, USA.
  • Nichols CIO; Berkeley Geochronology Center, 2455 Ridge Road, Berkeley, CA 94709, USA.
  • Weiss BP; Department of Earth, Atmospheric, and Planetary Sciences, Massachusetts Institute of Technology (MIT), 77 Massachusetts Avenue, Cambridge, MA 02139, USA.
Sci Adv ; 6(1): eaax0883, 2020 01.
Article en En | MEDLINE | ID: mdl-31911941
Magnetic measurements of the lunar crust and Apollo samples indicate that the Moon generated a dynamo magnetic field lasting from at least 4.2 until <2.5 billion years (Ga) ago. However, it has been unclear when the dynamo ceased. Here, we report paleomagnetic and 40Ar/39Ar studies showing that two lunar breccias cooled in a near-zero magnetic field (<0.1 µT) at 0.44 ± 0.01 and 0.91 ± 0.11 Ga ago, respectively. Combined with previous paleointensity estimates, this indicates that the lunar dynamo likely ceased sometime between ~1.92 and ~0.80 Ga ago. The protracted lifetime of the lunar magnetic field indicates that the late dynamo was likely powered by crystallization of the lunar core.

Texto completo: 1 Bases de datos: MEDLINE Idioma: En Revista: Sci Adv Año: 2020 Tipo del documento: Article País de afiliación: Estados Unidos

Texto completo: 1 Bases de datos: MEDLINE Idioma: En Revista: Sci Adv Año: 2020 Tipo del documento: Article País de afiliación: Estados Unidos