Copy the page URI to the clipboard
Hauri, Erik H.; Saal, Alberto E.; Nakajima, Miki; Anand, Mahesh; Rutherford, Malcolm J.; Van Orman, James A. and Le Voyer, Marion
(2017).
DOI: https://doi.org/10.1146/annurev-earth-063016-020239
Abstract
Nearly forty years after the return of the first lunar samples to Earth, improvements in laboratory detection limits made possible the first definitive discovery of magmatic water in lunar volcanic samples. The intervening decade has seen an exponential increase in the amount of data on the abundance of magmatic water, and its hydrogen isotope composition, in various rock types recovered from the Moon. Here we review these data and describe how the abundance of water in the lunar interior places important constraints on models for the high-temperature origin and evolution of the Moon.
Viewing alternatives
Metrics
Public Attention
Altmetrics from AltmetricNumber of Citations
Citations from DimensionsItem Actions
Export
About
- Item ORO ID
- 50321
- Item Type
- Journal Item
- ISSN
- 1545-4495
- Project Funding Details
-
Funded Project Name Project ID Funding Body Astronomy and Planetary Sciences at the Open University ST/L000776/1 STFC (Science & Technology Facilities Council) Not Set ST/I001298/1 STFC (Science & Technology Facilities Council) - Keywords
- Moon; water; volcanism; pyroclastic; hydrogen; deuterium
- Academic Unit or School
-
Faculty of Science, Technology, Engineering and Mathematics (STEM) > Physical Sciences
Faculty of Science, Technology, Engineering and Mathematics (STEM) - Research Group
- ?? space ??
- Copyright Holders
- © 2017 Annual Reviews
- Depositing User
- Mahesh Anand