title mariana melting and thermal structure james a. conder dept. of earth and planetary sciences...
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Title
Mariana melting and thermal structure
Mariana melting and thermal structure
James A. ConderDept. of Earth and Planetary
SciencesWashington University
James A. ConderDept. of Earth and Planetary
SciencesWashington University
Subduction system melting & thermal componentsSubduction system melting & thermal components
From Zyzzy2 on Wikipedia (aka Bob Stern)
backarcbackarc arcarc forearcforearc slabslab
First order thermal controlsFirst order thermal controls
Convergence rate moderate/?
Backarc spreading slow/cold Slab age
old/cold
Geophysical constraints
Geophysical constraints
Wiens, Kelley, and Plank, 2006
Mariana mantle is relatively cool
Mariana mantle is relatively cool
Secondary thermal controlsSecondary thermal controls
Forearc depth extent
2D vs 3D flow 3D/warm?
Temperature-difference gridsfor different numerical modelsTemperature-difference gridsfor different numerical models
Conder, 2005, PEPI
Temp-dep viscosity - isoviscous Yield strength - Temp-dep visc
- Seismicity begins west of Big Blue Seamount
-Shallow seismicity ends at ~55 km depth
Courtesy of Erica Emry
60
40
20
80
Seismicity with depth near Big Blue (18ºN)
serpentinized forearc: receiver functions
serpentinized forearc: receiver functions
Tibi and Wiens, submitted
Yield strengthYield strength
+ serpentine+ serpentine
SSTs Top 350m above wet
basalt solidus
Likely extent of crustal
dewatering
Basalt facies & solidus from Hacker et al., 2003
“…melting of fluid-saturated subducted sediment or basalt in normal, steady-state subduction may be inevitable, rather than impossible.”Kelemen et al., 2003
Kincaid and Griffiths mantle motion
Kincaid & Griffiths, 2003
RollbackRollback
SlabtemperaturesSlabtemperatures
Melting
Decompression meltingDecompression melting + rehydration to 120km+ rehydration to 120km
Wedge melting structureWedge melting structure
Melting
+ rehydration to 200km+ rehydration to 200km+ rehydration to 120km+ rehydration to 120km
Wedge melting structureWedge melting structure
Crustal addition rateCrustal addition rate
Diamalanta et al., 2002Tori-Shima (Izu), 2002
Backarc-Arc relationship
Backarc-Arc relationship
Pagan vs.
Guam
Pagan vs.
Guam
Pagan seismic attenuation structurePagan seismic attenuation structure
Pozgay, 2007
Pagan Backarc Spreading moviePagan Backarc Spreading movie
Pagan melt structure
Pagan melt structure
Backarc-Arc relationship
Backarc-Arc relationship
Pagan vs.
Guam
Pagan vs.
Guam
Guam Backarc Spreading movieGuam Backarc Spreading movie
SummarySummary• Forearc/Slab: Serpentinization of the deep Mariana forearc
mantle extends the decoupling zone defining the forearc, potentially leading to warmer slab surface temperatures and possible slab melting.
• Arc: Melting beneath the Mariana arc may have significant contributions from multiple mechanisms: decompression melting ~20 km3/Myr/km; decomp+flux ~45; decomp+flux+slab <~ 50.
• Backarc: Arc and backarc melting have a history of intermixing with melting loci that become more distinct and less intermingled as spreading matures. Pagan is in the latter stages with distinct melting loci for arc and backarc. Melting loci are less distinct near Guam with more intermixing of melting regimes.
• Forearc/Slab: Serpentinization of the deep Mariana forearc mantle extends the decoupling zone defining the forearc, potentially leading to warmer slab surface temperatures and possible slab melting.
• Arc: Melting beneath the Mariana arc may have significant contributions from multiple mechanisms: decompression melting ~20 km3/Myr/km; decomp+flux ~45; decomp+flux+slab <~ 50.
• Backarc: Arc and backarc melting have a history of intermixing with melting loci that become more distinct and less intermingled as spreading matures. Pagan is in the latter stages with distinct melting loci for arc and backarc. Melting loci are less distinct near Guam with more intermixing of melting regimes.
Anatahan, N. Mariana, 2003