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Decline of the lunar core dynamo

Journal Article · · Earth and Planetary Science Letters
 [1];  [1];  [2];  [3];  [4];  [1];  [1];  [5];  [6]
  1. Massachusetts Inst. of Technology (MIT), Cambridge, MA (United States)
  2. Lawrence Livermore National Lab. (LLNL), Livermore, CA (United States)
  3. Univ. of California, Berkeley, CA (United States); Berkeley Geochronology Center, Berkeley, CA (United States)
  4. Massachusetts Inst. of Technology (MIT), Cambridge, MA (United States); Univ. Aix-Marseille (France)
  5. Univ. of California, Santa Cruz, CA (United States)
  6. Univ. of Hawaii at Manoa, Honolulu, HI (United States)

Recent analyses of Apollo samples have demonstrated that a core dynamo existed on the Moon between at least 4.25 and 3.56 billion years ago (Ga) with surface field intensities reaching ~70 μT. However, it is unknown when the Moon's magnetic field declined. Determining the temporal evolution of the dynamo is important because it constrains secular changes in power at the lunar core–mantle boundary and, by implication, the Moon's thermal and orbital evolution and the field generation mechanism. In this work, we present paleomagnetic data from several younger mare basalts which demonstrate that the surface magnetic field had declined precipitously to <~ 4μT by 3.19 Ga. It is currently unclear whether such a rapid decrease in field strength reflects either the cessation of the dynamo during this period or its persistence beyond 3.19 Ga in a drastically weakened state.

Research Organization:
Lawrence Livermore National Laboratory (LLNL), Livermore, CA (United States)
Sponsoring Organization:
USDOE National Nuclear Security Administration (NNSA)
Grant/Contract Number:
AC52-07NA27344
OSTI ID:
1762851
Report Number(s):
LLNL-JRNL--701457; 833825
Journal Information:
Earth and Planetary Science Letters, Journal Name: Earth and Planetary Science Letters Vol. 404; ISSN 0012-821X
Publisher:
ElsevierCopyright Statement
Country of Publication:
United States
Language:
English

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Cited By (15)

Preservation and detectability of shock-induced magnetization: PRESERVATION AND DETECTABILITY OF SRM journal September 2015
The sustainability of habitability on terrestrial planets: Insights, questions, and needed measurements from Mars for understanding the evolution of Earth-like worlds: Mars and Terrestrial Planet Habitability journal October 2016
The Case Against an Early Lunar Dynamo Powered by Core Convection: Lunar Dynamo: A Case Against Convection journal January 2018
Strength, Depth, and Geometry of Magnetic Sources in the Crust of the Moon From Localized Power Spectrum Analysis journal January 2018
Advanced Curation of Astromaterials for Planetary Science journal November 2019
Constraining the Evolutionary History of the Moon and the Inner Solar System: A Case for New Returned Lunar Samples journal December 2019
Lunar Swirl Morphology Constrains the Geometry, Magnetization, and Origins of Lunar Magnetic Anomalies: LUNAR MAGNETIC SOURCES CONSTRAINED BY SWIRLS journal August 2018
Distribution of Radioactive Heat Sources and Thermal History of the Moon journal December 2018
Domain State and Temperature Dependence of Pressure Remanent Magnetization in Synthetic Magnetite: Implications for Crustal Remagnetization journal May 2019
Early Dynamics of the Lunar Core journal November 2019
The potential for metal contamination during Apollo lunar sample curation journal March 2018
A two-billion-year history for the lunar dynamo journal August 2017
The end of the lunar dynamo journal January 2020
The lunar dynamo journal December 2014
Lifetime of the solar nebula constrained by meteorite paleomagnetism journal February 2017

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