Stability and bulk modulus of Ni3S, a new nickel sulfur compound, and the melting relations of the system Ni-NiS up to 10 GPa

被引:13
作者
Urakawa, Satoru [1 ]
Matsubara, Ryosuke [1 ]
Katsura, Tomoo [2 ]
Watanabe, Tohru [3 ]
Kikegawa, Takumi [4 ]
机构
[1] Okayama Univ, Dept Earth Sci, Kita Ku, Okayama 7008530, Japan
[2] Okayama Univ, Inst Study Earths Interior, Tottori 6820193, Japan
[3] Toyama Univ, Dept Earth Sci, Toyama 9308555, Japan
[4] High Energy Accelerator Res Org, Inst Mat Struct Sci, Tsukuba, Ibaraki 3050801, Japan
关键词
Nickel; sulfur; light element; melting; high pressure; core; X-RAY-DIFFRACTION; HIGH-PRESSURE; FE-FES; S SYSTEM; INTERNAL STRUCTURE; HIGH-TEMPERATURE; CORE; STATE; MARS; MINERALS;
D O I
10.2138/am.2011.3578
中图分类号
P3 [地球物理学]; P59 [地球化学];
学科分类号
0708 ; 070902 ;
摘要
We found a new nickel sulfide that is isostructural with Fe3S. The synthesized nickel sulfide is a non-stoichiometric compound with a Ni deficiency and its composition is Ni2.90 +/- 0.5S. In situ synchrotron X-ray observations indicate that Ni3-xS forms above 5.1 GPa and melts incongruently into Ni+liquid up to 10 GPa. The bulk modulus of Ni3-xS at 300 K was determined to be 140 +/- 2 GPa with a fixed K' = 4 by static compression with a liquid pressure medium. The eutectic point of the Ni-NiS system lies between Ni3S and Ni3S2 up to 10 GPa and its composition changes from Ni66.6S33.4 at 0.1 MPa to Ni70.7S29.3 at 10 GPa. The eutectic melting temperature of the Ni-NiS system decreases to 5.1 GPa and 720 K as the pressure increases where Ni and alpha-Ni3S2 are the eutectic solids. On the other hand, the eutectic melting temperature increases with a positive slope above 5.1 GPa where Ni3S+alpha-Ni3S2 is stable under subsolidus conditions. Intermediate compounds appear at a lower pressure in the Ni-NiS system than that for the Fe-FeS system. Ni3S2 is stable at atmospheric pressure and Ni3S forms at 5.1 GPa, whereas Fe3S2 and Fe3S form at 14 and 20 GPa, respectively. The addition of Ni coomplicates the melting relationship in the Fe-FeS system at high pressure because of the wider stability field of Ni3S. The low-melting temperature of the Fe-Ni-S system plays an important role in the percolative core-formation of planetesimals during planetary accretion.
引用
收藏
页码:558 / 565
页数:8
相关论文
共 34 条
[1]   Study of partial melting at high-pressure using in situ X-ray diffraction [J].
Andrault, D. ;
Morard, G. ;
Bolfan-Casanova, N. ;
Ohtaka, O. ;
Fukui, H. ;
Arima, H. ;
Guignot, N. ;
Funakoshi, K. ;
Lazor, P. ;
Mezouar, M. .
HIGH PRESSURE RESEARCH, 2006, 26 (03) :267-276
[2]   Effective hydrostatic limits of pressure media for high-pressure crystallographic studies [J].
Angel, Ross J. ;
Bujak, Maciej ;
Zhao, Jing ;
Gatta, G. Diego ;
Jacobsen, Steven D. .
JOURNAL OF APPLIED CRYSTALLOGRAPHY, 2007, 40 :26-32
[3]  
[Anonymous], 1958, Constitution of Binary Alloys
[4]   Partial melting in the iron-sulfur system at high pressure: A synchrotron X-ray diffraction study [J].
Campbell, Andrew J. ;
Seagle, Christopher T. ;
Heinz, Dion L. ;
Shen, Guoyin ;
Prakapenka, Vitali B. .
PHYSICS OF THE EARTH AND PLANETARY INTERIORS, 2007, 162 (1-2) :119-128
[5]   Eutectic melting in the system Fe-S to 44 GPa [J].
Chudinovskikh, Liudmila ;
Boehler, Reinhard .
EARTH AND PLANETARY SCIENCE LETTERS, 2007, 257 (1-2) :97-103
[6]   HIGH-PRESSURE EQUATION OF STATE FOR NACL, KCL, AND CSCL [J].
DECKER, DL .
JOURNAL OF APPLIED PHYSICS, 1971, 42 (08) :3239-&
[7]   STRUCTURE AND DENSITY OF FES AT HIGH-PRESSURE AND HIGH-TEMPERATURE AND THE INTERNAL STRUCTURE OF MARS [J].
FEI, YW ;
PREWITT, CT ;
MAO, HK ;
BERTKA, CM .
SCIENCE, 1995, 268 (5219) :1892-1894
[8]  
Fei YW, 2000, AM MINERAL, V85, P1830
[9]   High-pressure iron sulfur compound, Fe3S2, and melting relations in the Fe-FeS system [J].
Fei, YW ;
Bertka, CM ;
Finger, LW .
SCIENCE, 1997, 275 (5306) :1621-1623
[10]  
FLEET ME, 1977, AM MINERAL, V62, P341