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Endogenous Lunar VolatilesThe chapter will begin with an introduction that defines magmatic volatiles (e.g., H, F, Cl, S) versus geochemical volatiles (e.g., K, Rb, Zn). We will discuss our approach of understanding both types of volatiles in lunar samples and lay the ground work for how we will determine the overall volatile budget of the Moon. We will then discuss the importance of endogenous volatiles in shaping the "Newer Views of the Moon", specifically how endogenous volatiles feed forward into processes such as the origin of the Moon, magmatic differentiation, volcanism, and secondary processes during surface and crustal interactions. After the introduction, we will include a re-view/synthesis on the current state of 1) apatite compositions (volatile abundances and isotopic compositions); 2) nominally anhydrous mineral phases (moderately to highly volatile); 3) volatile (moderately to highly volatile) abundances in and isotopic compositions of lunar pyroclastic glass beads; 4) volatile (moderately to highly volatile) abundances in and isotopic compositions of lunar basalts; 5) volatile (moderately to highly volatile) abundances in and isotopic compositions of melt inclusions; and finally 6) experimental constraints on mineral-melt partitioning of moderately to highly volatile elements under lunar conditions. We anticipate that each section will summarize results since 2007 and focus on new results published since the 2015 Am Min review paper on lunar volatiles [9]. The next section will discuss how to use sample abundances of volatiles to understand the source region and potential caveats in estimating source abundances of volatiles. The following section will include our best estimates of volatile abundances and isotopic compositions (where permitted by available data) for each volatile element of interest in a number of important lunar reservoirs, including the crust, mantle, KREEP, and bulk Moon. The final section of the chapter will focus upon future work, outstanding questions, and any in-sights on the types of samples or experimental studies that will be needed to answer these questions.
Document ID
20170004974
Acquisition Source
Johnson Space Center
Document Type
Conference Paper
Authors
McCubbin, F. M.
(NASA Johnson Space Center Houston, TX, United States)
Liu, Y.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Barnes, J. J.
(NASA Johnson Space Center Houston, TX, United States)
Boyce, J. W.
(NASA Johnson Space Center Houston, TX, United States)
Day, J. M. D.
(Scripps Institution of Oceanography La Jolla, CA, United States)
Elardo, S. M.
(Carnegie Institution of Washington Washington, DC, United States)
Hui, H.
(Nanjing Univ. China)
Magna, T.
(Geological Survey of Czech Republic Prague, Czech Republic)
Ni, P.
(Michigan Univ. Ann Arbor, MI, United States)
Tartese, R.
(Manchester Univ. United Kingdom)
Vander Kaaden, K. E.
(Jacobs Technology, Inc. Houston, TX, United States)
Date Acquired
June 2, 2017
Publication Date
May 4, 2017
Subject Category
Lunar And Planetary Science And Exploration
Report/Patent Number
JSC-CN-39247
Report Number: JSC-CN-39247
Meeting Information
Meeting: New Views of the Moon - Europe
Location: Meunster
Country: Germany
Start Date: May 4, 2017
End Date: May 5, 2017
Distribution Limits
Public
Copyright
Public Use Permitted.
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