Magnetic evidence concerning a lunar core

Details Magnetic evidence concerning a lunar core Magnetic evidence concerning a lunar core

Apr 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976lpsc....7.3321g&link_type=abstract

In: Lunar Science Conference, 7th, Houston, Tex., March 15-19, 1976, Proceedings. Volume 3. (A77-34651 15-91) New York, Pergamon

Computer Science

1

Lunar Core, Lunar Magnetic Fields, Magnetic Permeability, Chemical Composition, Diamagnetism, Error Analysis, Geomagnetic Tail, Iron, Lunar Evolution, Magnetic Dipoles, Magnetic Induction

Scientific paper

Two different methods were used to determine the lunar electromagnetic response: (1) comparison of Apollo 12 and Explorer 35 magnetometer data; and (2) observation of the dipole field configuration by orbiting Apollo 15 and 16 subsatellites. The methods give significantly different results. The subsatellite observations require the existence of a core, while the Apollo 12 and Explorer magnetometer measurements allow, but do not require, the existence of a core. Despite this, an upper limit of 580 km has been computed for the radius of the core.

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