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Granite melt convecting in an experimental micro-magma chamber at 1050 °C, 15 kbar

Carroll, Michael R. and Wyllie, Peter J. (1989) Granite melt convecting in an experimental micro-magma chamber at 1050 °C, 15 kbar. European Journal of Mineralogy, 1 (2). pp. 249-260. ISSN 0935-1221. http://resolver.caltech.edu/CaltechAUTHORS:20160120-154811132

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Abstract

Equal masses of powdered granite and serpentinized peridotite packed into gold capsules with the materials separated by a sharp vertical boundary were held for between 0 minute and 11 hours at 1 050 °C, 15 kbar to investigate contamination of hydrous granite melt by reaction with ultramafic rocks, as might occur near the crust-mantle boundary. The shorter duration runs show a melting front advancing from the vertical granite-peridotite boundary, where water is released from serpentine dehydration in the peridotite. The rate of advance of the melt front decreases from over 10^(-4) cm/s in the first minutes to less than 10^(-5) cm/s after 1 hour, suggesting that water diffusion to the melting front controls the melting rate. Experiments of longer duration show evidence of convective flow of the granitic melt, and the flow features defined by graphite distributed in glass develop continuously with time. A 7 hour run shows a small concentration of residual quartz and feldspar at the far end of the capsule, with trails of graphite and entrained crystals tracing flow lines from the crystal-rich area towards the center of the peridotite boundary, then around in a near-circular swirl in the lower half of the capsule. The graphite forms by reduction of the small amount of CO_2 in the starting materials. Glass analyses reveal initial steep compositional gradients adjacent to the peridotite (e.g. up to 2 wt.% MgO ; 0.1 wt.% in granite initially) but with increasing run duration the gradients become less steep and compositional changes are spread throughout the main body of melt. After 11 hours, the granite is completely melted, graphite which traced flow patterns in shorter runs has disappeared (presumably due to oxidation), and the granite is similar in composition to the starting material ; the most notable changes are an approximately 1.0 wt.% increase in MgO (0.1 wt.% initially), 0.4 wt.% increase in FeO (from 0.64 wt.% initially), and less than 1 wt.% decreases in A1_2O_3 and SiO_2. The driving forces for the observed flow are not known but the most likely explanations involve a small horizontal temperature gradient and/or small variations in melt water content.


Item Type:Article
Related URLs:
URLURL TypeDescription
http://dx.doi.org/10.1127/ejm/1/2/0249DOIArticle
https://www.schweizerbart.de/papers/ejm/detail/1/82487/Granite_melt_converting_in_an_experimental_micro_magma_chamber_at_1050degC_15_kbarPublisherArticle
Additional Information:© 1989 E. Schweizerbart'sche Verlagsbuchhandlung. Received 9 April 1988; Accepted 21 November 1988; Published: May 3, 1989. Research supported by NSF Earth Sciences, EAR85-06857. We thank Dave Stevenson and Steve Sparks for helpful discussions regarding convection in melts but the materials and interpretations presented herein remain solely the responsibilities of the authors. Caltech contribution number 4737.
Funders:
Funding AgencyGrant Number
NSFEAR85-06857
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Caltech Division of Geological and Planetary Sciences4737
Record Number:CaltechAUTHORS:20160120-154811132
Persistent URL:http://resolver.caltech.edu/CaltechAUTHORS:20160120-154811132
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:63814
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:21 Jan 2016 00:51
Last Modified:21 Jan 2016 00:51

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