Calculated melting curves for phases of iron

被引:56
作者
Anderson, OL [1 ]
Isaak, DG
机构
[1] Univ Calif Los Angeles, Inst Geophys & Planetary Phys, Ctr Phys & Chem Planets, Los Angeles, CA 90095 USA
[2] Azusa Pacific Univ, Dept Math & Phys, Azusa, CA 91702 USA
关键词
D O I
10.2138/am-2000-2-317
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 present a method by which the melting curves and corresponding densities along the liquidus of iron phases are calculated at high pressure. The melting curve of the epsilon(hcp) iron phase is calculated from P = 0 to P = 330 GPa. The melting curve of the gamma(i)(fcc) iron phase is calculated fr om P = 0 to P = 100 GPa. The point where these curves cross, near P = 50 GPa, is the location of the upper triple point on the melting curve. Our method combines the Lindemann melting equation with the Vinet isothermal equation of state. These equations are coupled by means of the Gruneisen parameter, gamma, which is given by K-T'(the pressure derivative of the isothermal bulk modulus, K-T) of the equation of state. By this thermodynamic formalism, we fmd values of volume, V; temperature, T; and the Gruneisen parameter, gamma, along the melting curve. This calculation requires the following thermal parameters: thermal expansivity, alpha(v), at high T; (partial derivative K-T/partial derivative(T)), at high T;the melting temperature, T-m, at P=0; q = (partial derivative ln gamma/partial derivative ln rho)(T) at high T; and gamma. The method also requires zero-pressure equation-of-state parameters: density, rho, at T = 300 ii, K-T at T = 300 K; and (partial derivative K-T/partial derivative P)(T) at T = 300 K. Our results do not confirm or deny the existence of the recently proposed beta phase. We demonstrate that with our existing knowledge the physical parameters of the beta and epsilon phases may be so close to each other that these two phases need not be considered separately in discussing the physics of iron at core P,T conditions. We find that one set of reasonable thermoelastic parameters of the epsilon phase reproduces the melting temperature and density at pressures of 50 and 240 GPa. Further, these parameters give agreement with previous estimates of the melting temperature and density at 330 GPa.
引用
收藏
页码:376 / 385
页数:10
相关论文
共 60 条
[1]  
Anderson O., 1995, EQUATIONS STATE SOLI
[2]   THE PHASE-DIAGRAM OF IRON AND THE TEMPERATURE OF THE INNER-CORE [J].
ANDERSON, OL .
JOURNAL OF GEOMAGNETISM AND GEOELECTRICITY, 1993, 45 (11-12) :1235-1248
[3]   THE HIGH-PRESSURE TRIPLE POINTS OF IRON AND THEIR EFFECTS ON THE HEAT-FLOW FROM THE EARTH CORE [J].
ANDERSON, OL .
JOURNAL OF GEOPHYSICAL RESEARCH-SOLID EARTH AND PLANETS, 1990, 95 (B13) :21697-21707
[4]   High pressure geophysics - Iron: Beta phase frays [J].
Anderson, OL .
SCIENCE, 1997, 278 (5339) :821-822
[5]   THE EARTHS CORE AND THE PHASE-DIAGRAM OF IRON [J].
ANDERSON, OL .
PHILOSOPHICAL TRANSACTIONS OF THE ROYAL SOCIETY A-MATHEMATICAL PHYSICAL AND ENGINEERING SCIENCES, 1982, 306 (1492) :21-35
[6]   The Gruneisen parameter for iron at outer core conditions and the resulting conductive heat and power in the core [J].
Anderson, OL .
PHYSICS OF THE EARTH AND PLANETARY INTERIORS, 1998, 109 (3-4) :179-197
[7]   PROPERTIES OF IRON AT THE EARTHS CORE CONDITIONS [J].
ANDERSON, OL .
GEOPHYSICAL JOURNAL OF THE ROYAL ASTRONOMICAL SOCIETY, 1986, 84 (03) :561-579
[8]  
ANDERSON OL, 1993, PHYS CHEM MINER, V19, P369, DOI 10.1007/BF00202974
[9]  
ANDERSON OL, 1994, HIGH PRESSURE SCI TE
[10]  
ANDERSON OL, 1988, GEOPHYSICAL MONOGRAP, V46