NASA Logo

NTRS

NTRS - NASA Technical Reports Server

Back to Results
Effect of Silicon on Activity Coefficients of Siderophile Elements (P, Au, Pd, As, Ge, Sb, and In) in Liquid Fe, with Application to Core FormationEarth's core contains approximately 10 percent light elements that are likely a combination of S, C, Si, and O, with Si possibly being the most abundant. Si dissolved into Fe liquids can have a large effect on the magnitude of the activity coefficient of siderophile elements (SE) in Fe liquids, and thus the partitioning behavior of those elements between core and mantle. The effect of Si can be small such as for Ni and Co, or large such as for Mo, Ge, Sb, As. The effect of Si on many siderophile elements is unknown yet 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 P, Au, Pd, and many other SE between metal and silicate melt. The results will be applied to Earth, for which we have excellent constraints on the mantle siderophile element concentrations.
Document ID
20160003888
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)
Danielson, L. R.
(Jacobs Technology, Inc. Houston, TX, United States)
Humayun, M.
(Florida State Univ. Tallahassee, FL, United States)
Righter, M.
(Houston Univ. Houston, TX, United States)
Lapen, T.
(Houston Univ. Houston, TX, United States)
Boujibar, A.
(Oak Ridge Associated Universities, Inc. Houston, TX, United States)
Date Acquired
March 25, 2016
Publication Date
March 21, 2016
Subject Category
Geophysics
Earth Resources And Remote Sensing
Report/Patent Number
JSC-CN-35649
Report Number: JSC-CN-35649
Meeting Information
Meeting: Lunar and Planetary Science Conference
Location: The Woodlands, TX
Country: United States
Start Date: March 21, 2016
End Date: March 25, 2016
Sponsors: Universities Space Research Association, NASA Headquarters, Lunar and Planetary Inst.
Distribution Limits
Public
Copyright
Public Use Permitted.
No Preview Available