HR: 0800h
AN: DI31A-0262 [Abstracts]
TI: Phase Relations of Iron and Iron-Nickel Alloys up to 3 Mbars
AU: * Kuwayama, Y
AF: IFREE, JAMSTEC, 2-15 Natsushima-cho, Yokosuka, 237-0061, Japan
AU: * Kuwayama, Y
AF: Department of Earth and Planetary Sciences, Tokyo Institute of Technology, 2-12-1,
Ookayama, Meguro-ku, Tokyo, 152-8551, Japan
AU: Hirose, K
AF: IFREE, JAMSTEC, 2-15 Natsushima-cho, Yokosuka, 237-0061, Japan
AU: Hirose, K
AF: Department of Earth and Planetary Sciences, Tokyo Institute of Technology, 2-12-1,
Ookayama, Meguro-ku, Tokyo, 152-8551, Japan
AU: Sata, N
AF: IFREE, JAMSTEC, 2-15 Natsushima-cho, Yokosuka, 237-0061, Japan
AU: Ohishi, Y
AF: Japan Synchrotron Radiation Research Institute, 1-1-1, Kouto, Sayo-gun, Hyogo, 679-5198,
Japan
AB:
Iron is believed to be the major component of the Earth's core because it is the most abundant element that
satisfies the observed seismic densities. Based on cosmochemical models and the studies of iron meteorites, it
is generally accepted that the Earth's core also contains substantial amounts of nickel. Therefore, the high
pressure behaviour of iron-nickel alloys is crucially important for interpreting and constraining geophysical and
geochemical models of the Earth's core. The phase relation of iron at relatively low pressure has been well
established. α-Fe with bcc structure at ambient condition transforms to γ-Fe at high temperature
and to ε-Fe with hcp structure at above ~ 10 GPa. In contrast, the phase relation and the crystal
structure at high pressure and temperature are still highly controversial. The phase relations of iron-nickel alloys
were also studied in an externally-heated diamond-anvil cell (Huang et al. 1988, 1992) and in a laser-heated
diamond-anvil cell (Lin et al. 2002, Mao et al. 2005, Dubrovinsky et al. 2007), but these experiments were limited
to the pressure of 225 GPa. Applications of the previous results to the Earth's inner core conditions required
significant extrapolations.
In this study, we have investigated the phase relations of iron and a number of iron-nickel alloys in a wide range
of pressures (>300 GPa), temperatures (>2000 K) and compositions (0-80 wt% Ni) using a laser-heated
diamond-anvil cell with synchrotron x-ray diffraction. For iron, in-situ x-ray diffraction studies showed a wide range
of stability of ε-Fe with an hcp structure up to 300 GPa and 2000 K and up to 343 GPa at room
temperature. No evidence for the existence of phases other than ε-Fe, such as β-Fe with a dhcp
structure (suggested by Dubrovinsky et al. 2000) or orthorhombic structure (suggested by Andrault et al. 1997),
was observed. For iron-nickel alloys, high pressure and temperature experiments were conducted on Fe-18.4
wt% Ni, Fe-24.9 wt% Ni, Fe-35.7 wt% Ni, Fe-50.0 wt% Ni and Fe-80.0 wt% Ni up to 300 GPa. The
experimental results indicate that the iron-nickel alloys strongly favour an fcc structure under multimegabar
pressures. Our results can directly apply to the Earthfs inner core pressures and the phase relations of iron-
nickel alloys may interpret seismically observed anisotropy and discontinuity in the Earth's inner core.
DE: 1015 Composition of the core
DE: 3924 High-pressure behavior
DE: 3954 X-ray, neutron, and electron spectroscopy and diffraction
DE: 7207 Core (1212, 1213, 8124)
DE: 8124 Earth's interior: composition and state (1212, 7207, 7208, 8105)
SC: Study of the Earth's Deep Interior [DI]
MN: 2007 Fall Meeting