The water content and parental magma of the second chassignite NWA 2737: Clues from trapped melt inclusions in olivine
Article first published online: 19 FEB 2013
© The Meteoritical Society, 2013.
Meteoritics & Planetary Science
Volume 48, Issue 3, pages 474–492, March 2013
How to Cite
He, Q., Xiao, L., Hsu, W., BALTA, J. B., McSween, H. Y. and Liu, Y. (2013), The water content and parental magma of the second chassignite NWA 2737: Clues from trapped melt inclusions in olivine. Meteoritics & Planetary Science, 48: 474–492. doi: 10.1111/maps.12073
- Issue published online: 18 MAR 2013
- Article first published online: 19 FEB 2013
- Manuscript Accepted: 18 DEC 2012
- Manuscript Received: 20 JUN 2012
- Natural Science Foundation of China. Grant Numbers: 41072045, 41173076, 41273079
- Doctoral Fund of Ministry of Education of China. Grant Number: 20090145110001
- Scientific Research Foundation for the Returned Overseas Chinese Scholars, State Education Ministry. Grant Number: 2010012009
- Minor Planet Foundation of China
Table S1: Melt-inclusion electron microprobe analyses of different minerals and glass for NWA 2737.
Table S2: Compositions of sulfides within the melt inclusions and intercumulate melts of NWA 2737.
Table S3: Electron microprobe analyses of apatite from the intercumulate melts of NWA 2737.
Table S4: The model abundances of phases (mole %) in each olivine-hosted inclusions for NWA 2737.
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