O. Jaoul et al., FE-MG INTERDIFFUSION IN OLIVINE UP TO 9 GPA AT T=600-900-DEGREES-C - EXPERIMENTAL-DATA AND COMPARISON WITH DEFECT CALCULATIONS, Physics of the earth and planetary interiors, 89(3-4), 1995, pp. 199-218
Interdiffusion data at high pressures are needed to provide good estim
ates of the closure temperatures of geothermometers based on Fe-Mg exc
hange in olivine in contact with other phases and to understand the pr
essure dependence of high-temperature deformation in olivine. We repor
t here measurements of the interdiffusion coefficient of Fe/Mg in San
Carlos olivine of mean composition Mg/(Mg + Fe) = 0.90, in the range o
f temperatures T = 600-900 degrees C and pressures P = 0.5-9 GPa. The
measurements were performed by preparing olivine samples covered by a
thin layer of fayalite. These specimens were annealed in a uniaxial sp
lit-sphere apparatus (USSA-2000). The Fe-Mg interdiffusion profiles we
re analysed by Rutherford back-scattering (RES). The results yield a p
re-exponential factor D-o = 7.7 x 10(-8) cm(2)s(-1) (7.7 x 10(-12) m(2
) s(-1)), and an activation energy E() = 147 +/- 58 kJmol(-1) (or 62
+/- 58 (2 SD) kJ mol(-1) if a p(2)(1/6) correction is performed), corr
esponding to the expression D = D(o)exp(-E()/RT)exp(epsilon X(Fe))exp
(-PV/RT). Our data are fitted best with epsilon = 3; X(Fe) = Fe/(Fe Mg) is between zero and one (in the present experiments X(Fe) is arou
nd 0.1), P is the pressure and V- is found to be -0.5 +/- 0.6 cm(3) m
ol(-1) (or 1 +/- 0.9 cm(3) mol(-1) if a pO(2)(1/6) correction is perfo
rmed), i.e. about zero in the P and T range investigated. Comparisons
between the present results, obtained at relatively low temperature un
der extrinsic conditions for diffusion, with other Fe-Mg interdiffusio
n data at high temperature (1125 degrees C or more) under intrinsic co
nditions allow us to deduce that the migration activation volume for p
oint defects is V-M() approximate to 0 whereas that for formation is
V-F() = 5.5 cm(3) mol(-1). This has important implications for the cr
eep sensitivity to pressure. Numerical simulations involving energy mi
nimizations and performed with the CASCADE and PARAPOCS codes confirm
these conclusions: one finds V-M() = 0 and V-F(*) = 4.8 cm(3) mol(-1)
. The activation energy E() deduced from the experiments as well as t
he pre-exponential factor Do now permit precise estimation of the clos
ure temperatures of geothermometers based on the Fe-Mg exchange betwee
n olivine and spinel.