کد مقاله کد نشریه سال انتشار مقاله انگلیسی نسخه تمام متن
4678069 1634828 2011 5 صفحه PDF دانلود رایگان
عنوان انگلیسی مقاله ISI
Compressibility change in iron-rich melt and implications for core formation models
موضوعات مرتبط
مهندسی و علوم پایه علوم زمین و سیارات علوم زمین و سیاره ای (عمومی)
پیش نمایش صفحه اول مقاله
Compressibility change in iron-rich melt and implications for core formation models
چکیده انگلیسی

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.

Research highlights
► Density of Fe-rich melt up to 8 GPa.
► Compressibility change identified at 5 GPa.
► Provides a mechanism for the change in siderophile elements partitioning.
► Core formation models must account for physical changes in core melts.

ناشر
Database: Elsevier - ScienceDirect (ساینس دایرکت)
Journal: Earth and Planetary Science Letters - Volume 306, Issues 1–2, 1 June 2011, Pages 118–122
نویسندگان
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