PUBLICATIONS Journal of Geophysical Research: Planets RESEARCH ARTICLE Further evidence for early lunar magnetism 10.1002/2016JE005154 from troctolite 76535 Key Points: Ian Garrick-Bethell1,2, Benjamin P. Weiss3, David L. Shuster4,5, Sonia M. Tikoo6, and • Using mutually oriented subsamples 4,5 of lunar troctolite 76535, we find Marissa M. Tremblay further evidence for a dynamo on the 1 2 Moon 4.25 Ga Department of Earth and Planetary Sciences, University of California, Santa Cruz, Santa Cruz, California, School of Space 3 • We find that the magnetizing field had Research, Kyung Hee University, Yongin-si, South Korea, Department of Earth, Atmospheric and Planetary Sciences, a paleointensity of 20-40 microteslas Massachusetts Institute of Technology, Cambridge, Massachusetts, USA, 4Department of Earth and Planetary Science, 40 39 • New Ar/ Ar thermochronometry University of California, Berkeley, Berkeley, California, USA, 5Berkeley Geochronology Center, Berkeley, California, USA, measurements provide an improved 6 sample age estimate of 4249 {plus Department of Earth and Planetary Sciences, Rutgers University, Piscataway Township, New Jersey, USA minus} 12 Ma Abstract The earliest history of the lunar dynamo is largely unknown and has important implications Supporting Information: for the thermal state of the Moon and the physics of dynamo generation. The lunar sample with the • Supporting Information S1 oldest known paleomagnetic record is the 4.25 billion year old (Ga) troctolite 76535. Previous studies of fi Correspondence to: unoriented subsamples of 76535 found evidence for a dynamo eld with a paleointensity of several tens I. Garrick-Bethell, of microteslas. However, the lack of mutual subsample orientation prevented a demonstration that the
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