Skip Navigation


Journal of Petrology Advance Access originally published online on August 21, 2009
Journal of Petrology 2009 50(9):1729-1764; doi:10.1093/petrology/egp051
This Article
Right arrow Full Text
Right arrow Full Text (PDF)
Right arrow Supplementary Data
Right arrow All Versions of this Article:
50/9/1729    most recent
egp051v1
Right arrow Alert me when this article is cited
Right arrow Alert me if a correction is posted
Services
Right arrow Email this article to a friend
Right arrow Similar articles in this journal
Right arrow Alert me to new issues of the journal
Right arrow Add to My Personal Archive
Right arrow Download to citation manager
Right arrowRequest Permissions
Google Scholar
Right arrow Articles by Johnson, E. R.
Right arrow Articles by Donegan, C. S.
Social Bookmarking
 Add to CiteULike   Add to Connotea   Add to Del.icio.us  
What's this?

© The Author 2009. Published by Oxford University Press. All rights reserved. For Permissions, please e-mail: journals.permissions@oxfordjournals.org

Subduction-related Volatile Recycling and Magma Generation beneath Central Mexico: Insights from Melt Inclusions, Oxygen Isotopes and Geodynamic Models

Emily R. Johnson1,2,*, Paul J. Wallace1, Hugo Delgado Granados3, Vlad C. Manea4, Adam J. R. Kent1, Ilya N. Bindeman1 and Colleen S. Donegan1,{dagger}

1Department of Geological Sciences, University of Oregon, Eugene, OR 97403, USA
2Codes ARC Centre of Excellence in ore Deposits, University of Tasmania, Private Bag 126, Hobart, Tasmania 7001, Australia
3Instituto de GeofÍsica, Universidad Nacional Autónoma de México, Distrito Federal, 04510 Mexico
4Computational Geodynamics Laboratory, Centro de Geociencias, Universidad Nacional Autónoma de México, Juriquilla, QueréTaro, 76230, Mexico

RECEIVED JULY 10, 2008; ACCEPTED JULY 21, 2009


   Abstract

The subduction-related Michoacán–Guanajuato Volcanic Field (MGVF) in central Mexico contains ~900 cinder cones and numerous larger shield volcanoes of Late Pliocene to Holocene age. We present data for major, trace and volatile (H2O, CO2, S, Cl) elements in olivine-hosted melt inclusions from eight calc-alkaline cinder cones with primitive magma characteristics and one more evolved alkali basalt tuff ring. The samples span a region extending from the volcanic front to ~175 km behind the front. Relationships between H2O and incompatible trace elements are used to estimate magmatic H2O contents for 269 additional volcanic centers across the MGVF and central Mexico. The results show that magmatic H2O remains high (3–5·75 wt %) for large distances (~150 km) behind the front. Chlorine and S concentrations are strongly correlated with melt H2O and are also high across most of the arc (700–1350 ppm Cl, 1500–2000 ppm S). The alkali basalt, located far behind the front (~175 km), has much lower volatile contents (<1·5 wt % H2O, 200 ppm Cl, 500 ppm S), and is compositionally similar to other melts erupted in this region. Oxygen isotope ratios of olivine phenocrysts (5·6–6{per thousand}) from the calc-alkaline samples are higher than for typical mantle-derived magmas but do not vary systematically across the arc. Calc-alkaline samples have high large ion lithophile element concentrations relative to Nb and Ta, as is typical of subduction-related magmas, but alkali basalt samples far behind the front have high Nb and Ta and lack enrichments in fluid-mobile elements. Modeling based on volatiles and trace elements suggests that the calc-alkaline magmas were generated by 6–15% partial melting of a variably depleted mantle wedge that was fluxed with H2O-rich components from the subducted slab. In contrast, the alkali basalts formed by small degrees of decompression melting of an ocean island basalt source that had not been fluxed by slab-derived components. Based on high {delta}18Oolivine values and trace element characteristics, the H2O-rich subduction components added to the mantle wedge beneath the MGVF are likely to be mixtures of oceanic crust derived fluids and sediment melts. Integrating these results with new 2-D thermo-mechanical models of the subduction zone beneath the MGVF, we demonstrate that the present-day plate configuration beneath the MGVF causes fluids to be released beneath the forearc and volcanic front, and that sediment melts can be produced beneath the volcanic front by the waning stages of fluid released from the oceanic crust percolating through already dehydrated sediments. Down-dragging of serpentine- and chlorite-bearing peridotite in the lowermost mantle wedge probably plays a role in fluid transport from the forearc to beneath the arc. H2O-rich magmas located more than ~50 km behind the volcanic front can be explained by mantle hydration related to a shallower slab geometry that existed at ~3 Ma. Rollback of the slab over the last ~2 Myr has resulted in strong mantle advection that forms low-H2O, high-Nb alkali basaltic magmas by decompression melting far behind the present-day volcanic front.

KEY WORDS: subduction; partial melting; oxygen isotopes; volatiles; devolatilization; melt inclusions


*Corresponding author. Telephone: +61 3 6226 7210. Fax: +61 3 6226 7662. E-mail: Emily.Johnson{at}utas.edu.au

{dagger}Present address: Department of Geology, Northern Arizona University, Flagstaff, AZ 86011, USA.


Add to CiteULike CiteULike   Add to Connotea Connotea   Add to Del.icio.us Del.icio.us    What's this?




Disclaimer: Please note that abstracts for content published before 1996 were created through digital scanning and may therefore not exactly replicate the text of the original print issues. All efforts have been made to ensure accuracy, but the Publisher will not be held responsible for any remaining inaccuracies. If you require any further clarification, please contact our Customer Services Department.