Shock temperature and melting in iron sulfides at core pressures

نویسندگان

  • William W. Anderson
  • Thomas J. Ahrens
چکیده

The temperatures of shock-compressed FeS and FeS 2in the pressure ranges 125-170 GPa nd 100-244 GPa, respectively, are reported and used to constrain the melting curves and thermodynamic properties to core pressures. A fit of the Lindemann lawparameters corresponding to the usual functional form for the lattice Grtineisen parameter gives YL = 1.17:L'0.13 andnœ = 0.5_+0.5 for the high-pressure phase ofFeS at p = 5340 kg/m 3 and YL TM 2.18:L-0.32 and nL = 1.6_+0.7 for FeS 2at p = 5011 kg/rn 3.The entropies of fusion are -203 J kg '1 K -• for FeS at 120 GPa nd -180 J kg '1 K '1 for FeS 2at 220 GPa. We find that the melting temperature ofFeS is 3240-•00 K, 4210-!-_700 K, and 4310-2:750 K at 136 GPa, 330 GPa, and 360 GPa, respectively. For FeS 2, the melting temperatures are 3990'•_300 K, 5310-!-_700 K, and 5440-!-_750 K, respectively, for the same pressures. The electronic specific heat for FeS is given by Ce= [•0 (P0/P) • with •0 = 0.25:L-0.10 J kg '1K -2 and 7e = 1.34 for P0 TM 5340 kg/m 3 for the highpressure solid phase and •o = 0.05 J kg -1 K -2 and 3⁄4e =1.34 for P0 = 5150 kg/m 3 for the liquid phase. For FeS 2, there is no detectable electronic contribution, and the lattice specific heat is only 67% of the Dulong-Petit limit, possibly implying tight S-S binding in S 2 units. A reexamination of all shock wave melting data for Fe indicates these approximately agree, but they do not resolve the disagreement between the extrapolated static diamond anvil cell data sets. Fe should melt at -6600 K at 243 GPa and 69003:750 K at 330 GPa (the pressure of the inner coreouter core boundary). Because the FeS melting curve falls well below that of FeS 2, FeS may eventually undergo petitecftc melting at high pressures, while FeS 2 melts congmently.

برای دانلود متن کامل این مقاله و بیش از 32 میلیون مقاله دیگر ابتدا ثبت نام کنید

ثبت نام

اگر عضو سایت هستید لطفا وارد حساب کاربری خود شوید

منابع مشابه

Shock temperature measurements in metals New results for an Fe alloy

The temperature of a Fe-Cr-Ni alloy (304 stainless steel) has been measured during shock compression using a high-speed radiometric technique. Experiments were performed on highquality thick films deposited on sapphire and LiF windows. The samples had no observable porosity or defects and closely meet the ideal criteria for shock temperature measurements. Data obtained with both A1203 and LiF w...

متن کامل

Melting of Fe - alloys and the thermal structure of the core

11 The temperature of the Earth’s core has significant implications in many areas of 12 geophysics, including applications to Earth’s heat flow, core composition, age of the 13 inner core, and energetics of the geodynamo. The temperature of the core at the inner 14 core boundary is equal to the melting temperature of the core’s Fe-rich alloy at the inner 15 core boundary pressure. This chapter ...

متن کامل

High Pressure and High Temperature Equation-of-state of Gamma and Liquid Iron

Shock-wave experiments on pure iron preheated to 1573 K were conducted in the 17-73 GPa range. The shock-wave equation of state ofy-iron at an initial temperature of 1573 K can be fit with u, = 4.102 (0.015) km/s + 1.610(0.014) up with p 0 = 7.413±0.012 Mg/m• We obtain for y-iron's bulk modulus and pressure derivative the values: 124.7±1.1 GPa and 5.44±0.06, respectively. We present new data fo...

متن کامل

Temperature of the inner-core boundary of the Earth: Melting of iron at high pressure from first-principles coexistence simulations

The Earth’s core consists of a solid ball with a radius of 1221 Km, surrounded by a liquid shell which extends up to 3480 km from the center of the planet, roughly half way toward the surface the mean radius of the Earth is 6373 km . The main constituent of the core is iron, and therefore the melting temperature of iron at the pressure encountered at the boundary between the solid and the liqui...

متن کامل

Melting in super-earths.

We examine the possible extent of melting in rock-iron super-earths, focusing on those in the habitable zone. We consider the energetics of accretion and core formation, the timescale of cooling and its dependence on viscosity and partial melting, thermal regulation via the temperature dependence of viscosity, and the melting curves of rock and iron components at the ultra-high pressures charac...

متن کامل

ذخیره در منابع من


  با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید

برای دانلود متن کامل این مقاله و بیش از 32 میلیون مقاله دیگر ابتدا ثبت نام کنید

ثبت نام

اگر عضو سایت هستید لطفا وارد حساب کاربری خود شوید

عنوان ژورنال:

دوره   شماره 

صفحات  -

تاریخ انتشار 2007