Gas-driven filter pressing in magmas: insights into in-situ melt segregation from crystal mushes

Friday, 18 December 2015: 16:15
308 (Moscone South)
Mattia Pistone, Smithsonian Institution - National Museum of Natural History, Mineral Sciences, Washington, DC, United States, Fabio Arzilli, Istituto Nazionale di Geofisica e Vulcanologia, Pisa, Italy; Elettra - Sincrotrone Trieste, Basovizza (Trieste), Italy, Katherine J Dobson, Ludwig Maximilians University of Munich, Munich, Germany, Benoit Cordonnier, Independent Scientist, Pescara, Italy, Eric Reusser, ETH-Zurich, Zurich, Switzerland, Peter Ulmer, ETH Swiss Federal Institute of Technology Zurich, Zurich, Switzerland, Federica Marone, Swiss Light Source - PSI, Villigen, Switzerland, Alan G Whittington, University of Missouri Columbia, Dept. Geological Sciences, Columbia, MO, United States, Lucia Mancini, Stanford Earth Sciences, Stanford, CA, United States, Julie Fife, Paul Scherrer Institute, Swiss Light Source, Villingen, Switzerland and Jonathan David Blundy, University of Bristol, Bristol, BS8, United Kingdom
Gas-driven filter pressing is the process of melt expulsion from a volatile-saturated crystal mush, induced by the buildup and subsequent release of gas pressure. Filter pressing is inferred to play a major role in magma fractionation at shallow depths (<10 km) by moving melt and gas relative to the solid, crystalline framework. However, the magmatic conditions at which this process operates remain poorly constrained. We present novel experimental data that illustrate how the crystal content of the mush affects the ability of gas-driven filter pressing to segregate melt. Hydrous haplogranite (2.1 wt% water in the melt) and dacite (4.2 wt% water in the melt) crystal mushes, with a wide range of crystallinities (34–80 vol% crystals), were investigated using in-situ, high temperature (500–800 °C) synchrotron X-ray tomographic microscopy with high spatial (3 micron/pixel) and temporal resolution (~8 s per 3D data set). The experimental results show that gas-driven filter pressing operates only below the maximum packing of bubbles and crystals (~74 vol%). Above this threshold, the mush tends to fracture and gas escapes via fractures. Therefore, the efficiency of gas-driven filter pressing is promoted close to the percolation threshold and in situations where a mush inflates slowly relative to build-up of pressure and expulsion of melt. Such observations offer a likely explanation for the production of eruptible, crystal-poor magmas within Earth’s crust.

Figure = Synchrotron X-ray tomographic microscopy 3D renderings of representative haplogranite (A–D) and dacite (E–H) samples, with different crystal (Φ) and bubble fractions (β) at representative temperatures and experimental times (t, in minutes). Black objects are bubbles and fractures; dark gray field is silicic glass/melt; light gray objects are corundum crystals in haplogranite sample, and quartz in dacite sample. White and black arrows indicate representative fractures and directions of melt expulsion during vesiculation, respectively. In H, white contours highlight quartz cluster boundaries and melt channels where melt is driven by gas bubbles. During experiments, gas exsolution mainly consists of (1) bubble nucleation and growth (white circles) and (2) crystal clustering and/or compaction (white rectangles).