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Updated: May 11, 2026

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Published on: November 15, 2013
Persistence and origin of the lunar core dynamo
Clément Suavet1, Benjamin P Weiss, William S Cassata
1Department of Earth, Atmospheric, and Planetary Sciences, Massachusetts Institute of Technology, Cambridge, MA 02139, USA. csuavet@mit.edu
Ancient lunar core dynamo persisted longer than previously thought, indicating a stable, intense magnetic field. This suggests a continuous power source, ruling out impact-driven rotation changes as the sole mechanism.
Area of Science:
- Lunar science
- Geophysics
- Paleomagnetism
Background:
- The ancient lunar core dynamo's power source and field generation mechanism remain debated.
- Understanding the dynamo's lifetime is crucial for lunar evolution models.
Purpose of the Study:
- To determine the lifetime and intensity of the ancient lunar dynamo.
- To constrain the power source and generation mechanism of the lunar magnetic field.
Main Methods:
- Analysis of two mare basalts aged 3.56 billion years.
- Paleomagnetic analysis to determine the strength and stability of the ancient magnetic field.
Main Results:
- Mare basalts were magnetized in a stable dynamo magnetic field of at least ~13 μT.
- The lunar dynamo's lifetime is extended by ~160 million years.
- The field was likely continuously active after the last major basin-forming impact.
Conclusions:
- Impact-driven rotation changes likely did not power the dynamo at this late stage.
- A persistent power source, such as lunar mantle precession or compositional convection, is required.
- The findings necessitate revisions to models of the Moon's internal evolution and magnetic field history.
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