Constraints on the thermal and mixing history of lunar surface materials and comparisons with basaltic meteorites

Journal of Geophysical Research: Planets

Volumn 102, Issue E8, 1997, Pages 19321-19334

  Batchelor, J D ^a,b   Symes, S J K ^a,c   Benoit, P H ^a   Sears, D W G ^a  

^a UNIVERSITY OF ARKANSAS   (United States)

^b Department of Social Sciences   (United States)

^c NASA JOHNSON SPACE CENTER   (United States)

Author keywords

Ab initio calculations; Electron capture; High resolution; Keto enol tautomerization; Neutralization reionization mass spectrometry; Oxalacetic acid; Tandem mass spectrometry; Translational energy spectroscopy

Indexed keywords

BASALT; LUNAR SURFACE; REGOLITH; THERMAL EVOLUTION; THERMOLUMINESCENCE;

MOON;

EID: 0031405752     PISSN: 01480227     EISSN: None     Source Type: Journal    
DOI: 10.1029/97JE01688     Document Type: Article

References (6)

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3. Basaltic Volcanism Study Project (BVSP), Basaltic Volcanism on the Terrestrial Planets, Lunar and Planet. Inst., Houston, Texas, 1981.
4. Basu, A., and D. S. McKay, Lunar soil and evolution and Apollo 16 core 60013/60014, Meteoritics, 30, 162-168, 1995.
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