recipe for rifting
play

Recipe for Rifting Cindy Ebinger Tulane University King Cake AGU - PowerPoint PPT Presentation

Recipe for Rifting Cindy Ebinger Tulane University King Cake AGU 2017 in New Orleans Volcanic systems respond to tectonic forces; density contrasts, fluid pressures modify ambient stress field glacial unloading rheology-dependent


  1. Recipe for Rifting Cindy Ebinger Tulane University

  2. King Cake AGU 2017 in New Orleans

  3. Volcanic systems respond to tectonic forces; density contrasts, fluid pressures modify ambient stress field glacial unloading rheology-dependent behavior Ebinger et al., 2013

  4. Foundations I Scales and architecture of extensional systems spatially variable. Endmembers, plus all between 1) ‘cratonic’ rifts – develop in cold lithosphere 2) ‘orogenic’ rifts – develop in collapsing orogens where crust is hot, mantle may be hydrated Differences confirm critical importance of crust and mantle rheology

  5. Rheology - We know we need to know hydration state and composition of lower crust, but we have few tools to measure in situ: Density Vp, Vs, Vp/Vs Xenoliths Magma petrology Volatiles as inclusions, soil and water measurements AR Lowry & M Pérez-Gussinye Nature 471 , 353-357 (2011) doi:10.1038/ nature09912

  6. Mineralogical reactions and enhanced geothermall gradients = considerable complexity in Vp and Vs; Compressible (volatiles) vs incompressible fluids (magma) changes Vp/Vs

  7. � � � � � � W (35,2.33S) Natron-Magadi Basin A-A’ E(37, 2.33S) 5 4 Initiation of magmatic Intrusion zone? 3 segment? 2 CO 2 CO 2 1 0 Archaean -10 craton -20 Vp/Vs 1.75 Vp/Vs 1.75 Vp/Vs = 1.70 -30 Vp/Vs 1.82 mantle lithosphere Vp/Vs 1.7 -40 0 20 40 60 80 100 120 140 160 180 200 220 Vp/Vs ~1.65 -CO2 as pore-filling fluid S-wave velocities; ANT, body wave, gravity joint inversion –Roecker et al., GJI, 2017; RF – Plasman et al. GJI, 2017; Weinstein et al., in review

  8. Foundations II Rocks are weak in extension Extensional strains widely distributed in continental regions • Scale with mantle upwelling • Orogen

  9. Hammond and Thatcher, JGR, 2007

  10. 15˚ Extensional strain and magmatism beneath > 100 Afar 10˚ km-thick lithosphere widely MER distributed – what is stable? 5˚ Turkana A-E-K Seismic moment release Eastern Rift Lakes 0˚ using NEIC (complete to ca M 4.5). TZ Divergence -5˚ Tangan- M 0 = µ As where is shear yika modulus of rock at EQ Malawi -10˚ source, and A is area of fault plane, and s is slip Davie Ridge -15˚ South ~10^2 y of 10^3-10^5 y Western -20˚ interseismic cycle -25˚ 30˚ 25˚ 35˚ 40˚ 45˚ km Lindsey et al., submi tu ed -4 -3 -2 -1 0 1 2 3 4 Fig. 3

  11. Foundations III Cratons are too strong to rift, yet they do. Magma- assisted rifting is important, but can’t generate magma under thick lithosphere. Additional forces + strength reducers: A) Cratonic roots and slabs divert mantle flow, enabling enhanced melt production and tractions + volatile release. B) Metasomatism – volatile-enriched mantle from prior subduction; mantle upwelling Jolante, Tyrone talks

  12. Edge-driven convection initiates at sharp boundary. Craton edge preserved only where cratonic mantle is dry and > 5 times stronger Currie, van Wijk, J. Geodynamics, 2016

  13. Aims: Use shear wave splitting Sleep et patterns (SKS, SKKS) to evaluate al. 2002 craton edge flow diversion; fluids Sensitive to LAB dip Contributions from LPO; oriented melt pockets (OMP); layered melt Up to 2 s splitting Data: New results from E, SW, NW margins of Tanzania craton (Tepp, Obrebski et al.) Holtzman and Kendall, 2010

  14. Gabrielle Tepp a-axis aligned with flow diverted between cratonic keels along rift thin zones? 17-0 Ma Rungwe volcanic province

  15. Craton-edge signal? Barruol & Ismail KMBO Archaean mantle (xenoliths) Albaric et al., G-cubed, 2014 + this study

  16. Foundations IV Strain localization within the crust strongly influenced by volatiles and magma Rapid stressing by magma intrusion, high pore pressures, super-critical CO 2 may induce lower crustal fault zones that localize strain and promote creep/slow-slip processes. – Muirhead talk to follow

  17. Large strain, steady-state rheological models for phyllosilicates allow for foliation development, cataclasis, pressure-solution - show velocity- dependent behavior A = plastic flow in 25 o C/km phyllosilicates B = frictional slip over 15 o C/km foliae C = pressure solution 35 o C/km controlled strength D = dilatational Fluid-assisted cataclasis – sliding by weakening dilatation 25 o C/km – what Niemeijer & Spiers, about greater depths, Geol Soc London super-critical CO 2 , higher gradients? 2005;

  18. Recipe for Strain Localization • Start with LAB topography and enhanced mantle tractions/small- scale convection. Use this to produce: • Small volume melting. • Release some volatiles to explode some kimberlites, lamproites,and to • Metasomatise mantle lithosphere and lower crust to reduce strength, increase melt production. If ‘rapid rise’ results needed, start with previously metasomatised mantle. • Keep elevated to encourage high GPE • Allow volatile expansion to increase fluid pathways, and fill pores to further reduce strength • Intrude magma to expedite heat transfer and enhance strain localization • Volatile percolation along fault zones to reduce friction and enable slip at lower stressing rates • Enhanced erosion and sediment loading = icing on ‘cake’ * Note: If rupture required, maintain upwelling or far-field stresses * Take with pinch of salt

  19. What do we need to enjoy a better rift ‘cake’ ? • ! Rock mechanics experiments at lower crustal conditions – super-critical CO 2 and fault friction • ! Direct observation of lower crust and upper mantle hydration - xenolith, fluid inclusion, Vp/Vs, MT • ! Continuous GPS and seismic monitoring along active fault zones – does aseismic creep occur in fluid-rich rift zones? • ! Quantify magma intrusion rates across range of settings • ! Compare and contrast crustal and mantle anisotropy patterns – role of fluid-filled fractures vs strain fabrics

Download Presentation
Download Policy: The content available on the website is offered to you 'AS IS' for your personal information and use only. It cannot be commercialized, licensed, or distributed on other websites without prior consent from the author. To download a presentation, simply click this link. If you encounter any difficulties during the download process, it's possible that the publisher has removed the file from their server.

Recommend


More recommend