REVERSAL OF THE ORTHOFERROSILITE-HIGH-P CLINOFERROSILITE TRANSITION, A PHASE-DIAGRAM FOR FESIO3 AND IMPLICATIONS FOR THE MINERALOGY OF THE EARTHS UPPER-MANTLE
Ab. Woodland et Rj. Angel, REVERSAL OF THE ORTHOFERROSILITE-HIGH-P CLINOFERROSILITE TRANSITION, A PHASE-DIAGRAM FOR FESIO3 AND IMPLICATIONS FOR THE MINERALOGY OF THE EARTHS UPPER-MANTLE, European journal of mineralogy, 9(2), 1997, pp. 245-254
The reconstructive phase transition between orthoferrosilite (OFS) and
high-pressure C2/c clinoferrosilite (HCFS) has been reversed for the
FeSiO3 composition over the pressure range of 5.0 to 7.5 GPa in a mult
i-anvil press. The position of the boundary is best fit by: P (GPa) =
0.00457(11) T (K) -0.084(153) From this result and Delta V-298K = -0.9
0(4) cm(3) mol(-1) from X-ray diffraction, we obtain Delta S-298K = -4
.11(21) J mol(-1) K-1 and Delta H-298K = -76(138) J mol(-1) for the OF
S-->HCFS transformation. The OFS-HCFS-LCFS (low-P clinoferrosilite) tr
iple point is located at 820(10)degrees C and 4.9(2) GPa from the inte
rsection of the OFS-HCFS boundary with the LCFS-OFS boundary previousl
y reversed by Lindsley (1965). The topology of the FeSiO3 phase diagra
m is, therefore, the same as that for MgSiO3, but with the orthorhombi
c to high-P monoclinic and low-P monoclinic to high-P monoclinic struc
tural transformations occurring at lower pressures. When combined with
previous work on the MgSiO3 end-member, our results that high-P clino
pyroxene is a stable phase in a pyrolite mantle below approximate to 3
00 km. However, its occurrence is limited by the progressive dissoluti
on of pyroxene into garnet at higher pressures. High-P C2/c clinopyrox
ene should be an even more important phase in the deeper portions of s
ubduction zones where a cooler thermal regime will stabilise this phas
e at shallower depths. The orthorhombic - high-P monoclinic transition
in Ca-poor pyroxene, producing a approximate to 3% density increase,
provides a reasonable petrologic explanation for the ''X seismic disco
ntinuity'' (Revenaugh & Jordan, 1991), which lies at a depth of approx
imate to 300 km.