Abstract
Models of lunar magnetism have involved dynamo action in a fluid core in an early hot Moon; an early cold Moon magnetised some time before 4.0 × 109 yr ago, which has subsequently heated up; and local field sources which, in some models, are related to impact. Here we examine the second possibility and show that provided the Moon contained a few percent of metallic iron and was exposed to an extra-Lunar field of about 10 or 20 oersted while much of it was still below the Curie point of iron, a restricted class of thermal evolution models, which satisfy the known constraints, can be derived.
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Strangway, D., Sharpe, H. Lunar magnetism and an early cold Moon. Nature 249, 227–230 (1974). https://doi.org/10.1038/249227a0
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DOI: https://doi.org/10.1038/249227a0
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