NASA Logo

NTRS

NTRS - NASA Technical Reports Server

Back to Results
Effect of Silicon on Activity Coefficients of P, Bi, Cd, Sn, and Ag in Liquid Fe-Si, and Implications for 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 Ni and Co, and larger effects on Mo, Ge, Sb, As metal/silicate partitioning. The effect of Si on metal-silicate partitioning has been quantified for many siderophile elements, but there are a few key elements for which the effects are not yet quantified. 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, Moon, and Vesta, for which we have good constraints on the mantle Bi, Cd, Sn, Ag, and P concentrations from mantle and/or basalt samples.
Document ID
20180002587
Acquisition Source
Johnson Space Center
Document Type
Conference Paper
Authors
Righter, K.
(NASA Johnson Space Center Houston, TX, United States)
Pando, K.
(Jacobs Technology, Inc. Houston, TX, United States)
Ross, D. K.
(Jacobs Technology, Inc. Houston, TX, United States)
Righter, M.
(Houston Univ. Houston, TX, United States)
Lapen, T. J.
(Houston Univ. Houston, TX, United States)
Date Acquired
April 27, 2018
Publication Date
March 19, 2018
Subject Category
Lunar And Planetary Science And Exploration
Report/Patent Number
JSC-E-DAA-TN52009
Report Number: JSC-E-DAA-TN52009
Meeting Information
Meeting: Lunar and Planetary Science Conference
Location: Woodlands, TX
Country: United States
Start Date: March 19, 2018
End Date: March 23, 2018
Sponsors: Universities Space Research Association
Funding Number(s)
CONTRACT_GRANT: NNJ13HA01C
Distribution Limits
Public
Copyright
Public Use Permitted.
No Preview Available