TY - JOUR
T1 - Compressibility change in iron-rich melt and implications for core formation models
AU - Sanloup, C.
AU - van Westrenen, W.
AU - Dasgupta, R.
AU - Maynard-Casely, H.
AU - Perrillat, J.P.
PY - 2011
Y1 - 2011
N2 - Metallic iron, in both solid and liquid states, is the dominant component of Earth's core. Density measurements of molten iron containing an appropriate amount of light elements (5.7. wt.% carbon) identified a liquid-liquid transition by a significant compressibility increase in the vicinity of the δ-γ-liquid triple point at 5.2. GPa. This transition pressure coincides with a marked change in the pressure evolution of the distributions of nickel, cobalt and tungsten between liquid metal and silicate melt that form a cornerstone of geochemical models of core formation. The identification of a clear link between molten metal polymorphism and metal-silicate element partitioning implies that reliable geochemical core formation models will need to incorporate the effects of these additional liquid metal transitions. © 2011 Elsevier B.V.
AB - Metallic iron, in both solid and liquid states, is the dominant component of Earth's core. Density measurements of molten iron containing an appropriate amount of light elements (5.7. wt.% carbon) identified a liquid-liquid transition by a significant compressibility increase in the vicinity of the δ-γ-liquid triple point at 5.2. GPa. This transition pressure coincides with a marked change in the pressure evolution of the distributions of nickel, cobalt and tungsten between liquid metal and silicate melt that form a cornerstone of geochemical models of core formation. The identification of a clear link between molten metal polymorphism and metal-silicate element partitioning implies that reliable geochemical core formation models will need to incorporate the effects of these additional liquid metal transitions. © 2011 Elsevier B.V.
U2 - 10.1016/j.epsl.2011.03.039
DO - 10.1016/j.epsl.2011.03.039
M3 - Article
VL - 2011
SP - 118
EP - 122
JO - Earth and Planetary Science Letters
JF - Earth and Planetary Science Letters
SN - 0012-821X
IS - 306
ER -