V14C-05
Structure and Viscosity of Carbonate-Silicate Melts Using in situ Techniques

Monday, 14 December 2015: 17:00
103 (Moscone South)
Daniel R Hummer1, Craig E Manning2, Abby Kavner2, Yoshio Kono3, Changyong Park4 and Curtis Kenney-Benson4, (1)Carnegie Institution for Science, Washington, DC, United States, (2)University of California Los Angeles, Los Angeles, CA, United States, (3)Carnegie Institution for Science Washington, Washington, DC, United States, (4)Carnegie Instituion of Washing, Argonne, IL, United States
Abstract:
The chemical properties of carbon-rich magmas at high pressures and temperatures are a major factor controlling the deep-Earth carbon cycle, and may play a crucial role in global magmatism at depth. We have measured the structure of carbonate-silicate liquids as a function of carbon content along the calcite-wollastonite (CaCO3-CaSiO3) and calcite-forsterite (CaCO3-Mg2SiO3) compositional joins at ~1800 oC, and 3 or 6 GPa in a Paris-Edinburgh press using X-ray diffuse scattering. Pair distribution functions calculated from the scattering data confirm that CaCO3 behaves as an ionic liquid, while compositions with 40-100 wt% wollastonite contain polymerized silicate with an average connectivity (Qn) of at least two bridging O per Si (Q2). Even liquid compositions with as little as 35 wt% forsterite component contain silicate polymers, despite the absence of bridging O in the crystalline orthosilicate. As the carbonate content of the melt is increased, the average connectivity of SiO4 units linearly increases from ~Q2 for pure wollastonite liquid to >Q3 for 40 wt% wollastonite, even though less silicate is present. Analysis of Ca-Ca and Ca-Si pair correlations, as well as Ca-O bond distances, indicate that Ca2+ bonds more strongly to the silicate framework as carbonate content increases. Increasing pressure from 3 to 6 GPa at constant composition causes Qn to fall near Q0. The trends in local atomic structure with composition and pressure explain falling sphere viscometry measurements in carbonate-silicate liquids at upper mantle conditions. These viscosities are as low as 6x10-3 Pa-s for pure CaCO3, only half a log unit higher than that of water, and span ~1.6 log units between the carbonate and silicate end-members. Structural and viscosity trends taken together indicate carbonate-rich, depolymerized and highly mobile liquid at depth which transitions into silicate-rich, polymerized and much less mobile liquid as the melt ascends into the crust.