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Updated: Jul 12, 2026

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Simulating Imaging of Large Scale Radio Arrays on the Lunar Surface
Published on: July 30, 2020
Magnetic properties of lunar samples
Summary
Magnetic properties of Apollo 11 lunar samples reveal submicroscopic native iron as the primary magnetic constituent. Some samples exhibit weak, unstable remanent magnetization, crucial for understanding lunar magnetic history.
Area of Science:
- Lunar geology
- Geophysics
- Mineralogy
Background:
- Apollo 11 mission returned lunar rock and fines.
- Understanding the magnetic properties of lunar samples is key to deciphering the Moon's magnetic field history.
Purpose of the Study:
- Characterize the magnetic properties of Apollo 11 lunar samples.
- Identify the primary magnetic constituents and their contribution to magnetization.
- Assess the remanent magnetization stability of different sample types.
Main Methods:
- Magnetic property measurements on rock, fines, and magnetic separates.
- Microscopic analysis to identify mineralogical constituents.
Main Results:
- Submicroscopic native iron (or nickel-iron) is the dominant magnetic component.
- Ilmenite, paramagnetic iron minerals, and iron-titanium oxides contribute minor magnetic effects.
- Micro-breccia samples quickly acquired viscous magnetization with little stable remanence.
- Crystalline samples showed weak but somewhat stable natural remanence.
Conclusions:
- Native iron is the principal source of magnetism in these Apollo 11 samples.
- The magnetic stability varies significantly between different lunar sample types.
- Findings contribute to the understanding of lunar magnetic fields and sample magnetization.
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