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Effect of Silicon on Activity Coefficients of P, Bl, CD, SN, and AG in Liquid Fe-Si, and Implications for Differentiation and Core FormationCores of differentiated bodies (Earth, Mars, Mercury, Moon, Vesta) contain light elements such as S, C, Si, and O. We have previously measured small effects of Si on metal-silicate partitioning of Ni and Co [1,2], and larger effects for Mo, Ge, Sb, As [2]. The effect of Si on many siderophile elements could be an important, and as yet unquantified, influence on the core-mantle partitioning of SE. Here we report new experiments designed to quantify the effect of Si on the partitioning of Bi, Cd, Sn, Ag, and P between metal and silicate melt. The results will be applied to Earth, Mars, Mercury, Moon, and Vesta, for which we have excellent constraints on the mantle Bi, Cd, Sn, Ag, and P concentrations from mantle and/or basalt samples.
Document ID
20170006937
Acquisition Source
Johnson Space Center
Document Type
Conference Paper
Authors
Righter, K.
(NASA Johnson Space Center Houston, TX, United States)
Pando, K.
(Jacobs Technologies Engineering Science Contract Group Houston, TX, United States)
Ross, D. K.
(Jacobs Technology, Inc. Houston, TX, United States)
Date Acquired
July 25, 2017
Publication Date
July 23, 2017
Subject Category
Lunar And Planetary Science And Exploration
Report/Patent Number
JSC-CN-39724
Report Number: JSC-CN-39724
Meeting Information
Meeting: Annual Meeting of The Meteoritical Society
Location: Santa Fe, NM
Country: United States
Start Date: July 23, 2017
End Date: July 28, 2017
Sponsors: Meteoritical Society
Distribution Limits
Public
Copyright
Public Use Permitted.
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