Koichi Sakamaki, Eiichi Takahashi, Yoichi Nakajima, Yu Nishihara, Ken-ichi Funakoshi, Toshihiro Suzuki, Yuh Fukai
Physics of the Earth and Planetary Interiors 174 1-4 192 - 201 2009年05月
[査読有り] 研究論文(学術雑誌)
High-pressure and high-temperature X-ray diffraction experiments on FeHx up to 20 GPa and 1598 K were performed using a Kawai-type multi-anvil apparatus, SPEED-MkII, installed at BL04B1 beam line of SPring-8 synchrotron facility. Iron powder was packed in a container made of NaCl, a very efficient sealing material for hydrogen under high pressure, together with a hydrogen source, LiAlH4. The temperature of hydrogenation, transition of iron hydride phases, and melting of gamma-FeHx were all determined in situ in the pressure range between 10 and 20 GPa. Hydrogen concentration in both epsilon'- and gamma-FeHx phases reached x = 1.0 above 10 GPa. Melting temperatures of gamma-FeH were determined to be 1473, 1448 +/- 25, 1538 +/- 15, 1548 +/- 25 and 1585 +/- 13 K at 10, 11.5,15,18 and 20 GPa, respectively. These temperatures are nearly 700 K lower than that of pure iron under the corresponding pressures. The Clapeyron-slope (dT/dP slope) of the melting curve of gamma-FeH is 13 K/GPa, which is significantly smaller than those of other possible core constituents (Fe, FeO, FeS). By extrapolating the epsilon'-gamma phase boundary linearly and the melting curve of gamma-FeH based on Lindemann's melting law, the triple point of epsilon'- and gamma-FeH and iron hydride melt is located at P = 60 GPa and T = 2000 K. Beyond the triple point, an attempt to construct a melting curve of epsilon'-FeH by the Lindemann's law using estimated thermal equation of state of epsilon'-FeH was unsuccessful. Therefore, we decided, instead, to extrapolate the melting curve of gamma-FeH beyond the triple point to 135 GPa yielding the melting temperature of FeH similar to 2600 K at core mantle boundary (CMB). Based on these results, we propose that the temperature of the Earth's outer core could be much lower than current estimates, if the Earth's outer core incorporated significant amounts of hydrogen. (C) 2008 Elsevier B.V. All rights reserved.