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Coordinated analysis of space weathering characteristics in lunar samples to understand water distribution on the Moon

Published online by Cambridge University Press:  30 July 2021

Alexander Kling ,
Michelle Thompson ,
Jennika Greer  and
Philipp Heck
Alexander Kling
Affiliation:
Department of Earth, Atmospheric, and Planetary Sciences, Purdue University, West Lafayette, IN, 47907, Lafayette, Indiana, United States
Michelle Thompson
Affiliation:
Purdue University - Department of Earth, Atmospheric, and Planetary Sciences, United States
Jennika Greer
Affiliation:
Department of the Geophysical Sciences, University of Chicago, Chicago, Illinois, 60637 USA, United States
Philipp Heck
Affiliation:
Robert A. Pritzker Center for Meteoritics and Polar Studies, Field Museum of Natural History, Chicago, Illinois, 60605 USA, United States

Abstract

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Type
Moon Dust, Minerals and Microscopy
Information
Microscopy and Microanalysis , Volume 27 , Supplement S1 , August 2021 , pp. 2260 - 2262
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Copyright
Copyright © The Author(s), 2021. Published by Cambridge University Press on behalf of the Microscopy Society of America

References

Pieters, Carle M., & Noble, S. K. (2016). Space weathering on airless bodies. Journal of Geophysical Research: Planets, 121(10), 1865–1884. https://doi.org/10.1002/2016JE005128CrossRefGoogle ScholarPubMed
Keller, Lindsay P., & McKay, D. S. (1993). Discovery of vapor deposits in the lunar regolith. Science, 261(5126), 1305–1307. https://doi.org/10.1126/science.261.5126.1305Google ScholarPubMed
Keller, Lindsay P, & McKay, D. S. (1997). The nature and origin of rims on lunar soil grains. Geochimica et Cosmochimica Acta, 61, 2311–2341.Google Scholar
Bradley, J. P., Ishii, H. A., Gillis-Davis, J. J., Ciston, J., Nielsen, M. H., Bechtel, H. A., & Martin, M. C. (2014). Detection of solar wind-produced water in irradiated rims on silicate minerals. Proceedings of the National Academy of Sciences of the United States of America, 111(5), 1732–1735. https://doi.org/10.1073/pnas.1320115111CrossRefGoogle ScholarPubMed
Farrell, W. M., Hurley, D. M., Esposito, V. J., McLain, J. L., & Zimmerman, M. I. (2017). The statistical mechanics of solar wind hydroxylation at the Moon, within lunar magnetic anomalies, and at Phobos. Journal of Geophysical Research: Planets, 122(1), 269–289. https://doi.org/10.1002/2016JE005168CrossRefGoogle Scholar
Tucker, O. J., Farrell, W. M., Killen, R. M., & Hurley, D. M. (2019). Solar Wind Implantation Into the Lunar Regolith: Monte Carlo Simulations of H Retention in a Surface With Defects and the H 2 Exosphere. Journal of Geophysical Research: Planets, 124(2), 278–293. https://doi.org/10.1029/2018JE005805CrossRefGoogle Scholar
Chamberlin, S., Christoffersen, R., & Keller, L. (2008) Space plasma ion processing of the lunar soil: Modeling of radiation-damaged rim widths on lunar grains. Lunar and Planetary Science Conference, Abstract #2302Google Scholar
Thompson, M. S., Zega, T. J., Becerra, P., Keane, J. T., & Byrne, S. (2016). The oxidation state of nanophase Fe particles in lunar soil: Implications for space weathering. Meteoritics and Planetary Science, 51(6), 1082–1095. https://doi.org/10.1111/maps.12646Google Scholar