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Title: Determining the origins of lunar remanent crustal magnetism
Primary Author: Jasper Halekas
Secondary Author(s): M. Fuller, I. Garrick-Bethell, L. L. Hood, C. L. Johnson, K.
Lawrence, R. J. Lillis, R. P. Lin, M. Manga, M. E. Purucker, B. P. Weiss
Institution: University of California Berkeley
Summary: The discovery of lunar magnetic fields of crustal origin was a major scientific surprise of the Apollo program. Solving the enigma of lunar remanent crustal magnetization will provide fundamental insights into the thermal history of the lunar core/dynamo, mantle, and crust, and into the processes by which crustal magnetization is acquired on airless bodies - for instance, large basin-forming impacts. Determining the origin and history of lunar crustal magnetism will require the return of oriented samples...
Panel Selection: Inner Planets: Mercury, Venus, and the Moon.
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These documents have been prepared in coordination with the National Academies of Science in support of the National Academies Planetary Science Decadal Survey. These documents are being made available for information purposes only, and any views and opinions expressed herein do not necessarily state or reflect those of NASA, JPL, or the California Institute of Technology.