Liquid segregation parameters from amphibolite dehydration melting experiments
- Creators
- Wolf, Michael B.
- Wyllie, Peter J.
Abstract
We have experimentally obtained some of the parameters necessary for understanding the segregation of silicate liquid from amphibolite undergoing dehydration melting at 1 GPa and 750–1000°C. The solidus for this calcic amphibolite (68% Mg-Hb, 32% Pl (An_(90))) is <750°C. Amphibolites begin to melt at relatively high temperatures in the garnet-absent field, but the solidus appears to backbend at ∼1 GPa, coincident with the garnet-in boundary. Hornblende breakdown due to garnet formation releases H_2O and causes melting. Thus, in the garnet-present field (≥1 GPa), the amphibolite dehydration melting solidus may be coincident with the H_2O-saturated solidus. Liquid interconnectivity may be achieved at <900°C and <5 vol % liquid, based on both physical and chemical data from solid rock runs. Mass balance calculations from powdered rock runs suggest that small amounts (∼5–15 vol %) of hydrous (≥4 wt % H_2O), low-viscosity (10^3–10^4 Pa s), heavy rare earth element-depleted, felsic liquid may be segregated during amphibolite dehydration melting at ≥875°C. The rapid breakdown of coarse-grained Hb cores may lead to the formation of transient H_2O-saturated liquids with even lower viscosities (∼10^2 Pa s). Although comprising only a small portion of the melting cycle, these H_2O-rich conditions may enhance the segregation of liquid by reduction of liquid viscosities and by mechanical effects on the restite (e.g., increased deformation and liquid fracturing). During anatexis of coarse-grained (natural) rocks, transient conditions may control the initial stages of liquid segregation.
Additional Information
Copyright 1995 by the American Geophysical Union. (Received July 15, 1994; revised January 13, 1995; accepted February 24, 1995.) Paper number 95JB00660. This research was supported by the Earth Science section of NSF, grant EAR 89-04375. We thank A. Patiño Douce, D. Laporte, and T. Rushmer for their thoughtful reviews.Attached Files
Published - jgrb10024.pdf
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Additional details
- Eprint ID
- 51322
- Resolver ID
- CaltechAUTHORS:20141105-134311354
- NSF
- EAR 89-04375
- Created
-
2014-11-05Created from EPrint's datestamp field
- Updated
-
2021-11-10Created from EPrint's last_modified field
- Caltech groups
- Division of Geological and Planetary Sciences (GPS)