T. Inoue et al., DECOMPOSITION OF K-AMPHIBOLE AT HIGH-PRESSURES AND IMPLICATIONS FOR SUBDUCTION ZONE VOLCANISM, Physics of the earth and planetary interiors, 107(1-3), 1998, pp. 221-231
The stability of K-amphibole has been studied at pressures 12.6-16.5 G
Pa, and at temperatures 940-1450 degrees C. K-amphibole decomposes int
o an assemblage of clinoenstatite + diopside + an unknown phase (X) stishovite + fluid at pressures above 16 GPa and temperatures below 12
00 degrees C. The phase boundary has a negative Clapeyron slope, and t
he high temperature assemblage is clinoenstatite + diopside + X + wade
ite-type K2Si4O9 + fluid at pressures 14-16 GPa. The X phase has a cat
ion ratio of approximately K:Mg:Si = 1:2:2, and contains 1.7 +/- 0.1 w
t.% H2O as determined by SIMS measurements, leading to a formula of K4
Mg8Si8O25(OH)(2). The present results suggest that the decomposition o
f K-amphibole in the dragged hydrous peridotite layer at the base of t
he mantle wedge may produce certain amounts of H2O-rich fluid at 14-16
GPa(similar to 450 km depth), while some of H2O is trapped in the new
hydrous phase X and is further carried into deeper regions of the man
tle. The aqueous fluid released by the decomposition of K-amphibole sh
ould react with beta-phase to form hydrous beta-phase in the mantle tr
ansition region. Thus, the dehydration of K-amphibole would not cause
any volcanic activities in the back are regions, in contrast to the de
hydrations of amphibole, chlorite and phlogopite, which are presumably
responsible for the first and the second volcanic chains. However, so
me of the volcanic activities such as in Muriah, Indonesia, may be rel
ated to the dehydration of K-amphibole in unusually hot regions above
the subducting slab. (C) 1998 Elsevier Science B.V. All rights reserve
d.