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Mid-Ocean Ridge Basalts (MORB), oceanic crust and ophiolites The Mid-Ocean Ridge System Figure 13-1. After Minster et al. (1974) Geophys. J. Roy. Astr. Soc., 36, 541-576. Rifting of continental crust to form a new ocean basin Subducting oceanic lithosphere deforms sediment at edge of continental plate Collision – welding together of continental crust Post-collision: two continental plates are welded together, mountain stands where once was ocean Ophiolites in Himalaya Zanskar Indian crust MHT Distribution of European Ophiolites European ophiolites are related to the collision of Europe with Africa. They represent remnants of the Jurassic Tethyan Ocean Oman (Semail) Ophiolite Greenschist facies shear zones Layered … massive gabbros Dykes Pillows Obduction Oceanic Crust and Upper Mantle Structure 4 layers distinguished via seismic velocities Deep Sea Drilling Program Dredging of fracture zone scarps Ophiolites Oceanic Crust and Upper Mantle Structure Typical Ophiolite Figure 13-3. Lithology and thickness of a typical ophiolite sequence, based on the Samial Ophiolite in Oman. After Boudier and Nicolas (1985) Earth Planet. Sci. Lett., 76, 84-92. Oceanic Crust and Upper Mantle Structure Layer 1 A thin layer of pelagic sediment Figure 13-4. Modified after Brown and Mussett (1993) The Inaccessible Earth: An Integrated View of Its Structure and Composition. Chapman & Hall. London. Oceanic Crust and Upper Mantle Structure Layer 2 is basaltic Subdivided into two sub-layers Layer 2A & B = pillow basalts Layer 2C = vertical sheeted dikes Figure 13-4. Modified after Brown and Mussett (1993) The Inaccessible Earth: An Integrated View of Its Structure and Composition. Chapman & Hall. London. Pillow lavas in the Semail Ophiolite Basaltic pillows Pillow Lavas in the Josephine Ophiolite Submarine eruptions and pillows Sheeted Dyke / Lava Transition The vertical slabs of rock are dikes intruding into lavas that erupted on the seafloor. This section represents the transition from lavas to sheeted dikes and is thought to correspond to seismic Layer 2B Sheeted Dykes in Semail Ophiolite Layer 3 more complex and controversial Believed to be mostly gabbros, crystallized from a shallow axial magma chamber (feeds the dikes and basalts) Layer 3A = upper isotropic and lower, somewhat foliated (“transitional”) gabbros Layer 3B is more layered, & may exhibit cumulate textures Layered Gabbros and Moho Semail Gabbros Oceanic Crust and Upper Mantle Structure Discontinuous diorite and tonalite (“plagiogranite”) bodies = late differentiated liquids Figure 13-3. Lithology and thickness of a typical ophiolite sequence, based on the Samial Ophiolite in Oman. After Boudier and Nicolas (1985) Earth Planet. Sci. Lett., 76, 84-92. Plagiogranites Layer 4 = ultramafic rocks Ophiolites: base of 3B grades into layered cumulate wehrlite & gabbro Wehrlite intruded into layered gabbros Below cumulate dunite with harzburgite xenoliths Below this is a tectonite harzburgite and dunite (unmelted residuum of the original mantle) Serpentinites (weathered peridotites) Evidence for melting in serpentinites 16 14 Na2O+K2O 12 10 8 6 F = FeO total 4 2 0 38 48 58 68 78 SiO2 A = Na2O + K2O M = MgO Petrography and Major Element Chemistry Q Quartzolite 90 A “typical” MORB is an olivine tholeiite with low K2O (< 0.2%) and low TiO2 (< 2.0%) 90 Quartz-rich Granitoid 60 60 Granite Alkali Fs. 20 Quartz Syenite Alkali Fs. 5 Syenite A 10 Granodiorite 20 Quartz Monzodiorite Syenite35 Monzonite 65 Monzodiorite90 10 (Foid)-bearing (Foid)-bearing (Foid)-bearing Syenite Monzonite Monzodiorite Quartz Syenite Quartz Monzonite Qtz. Diorite/ Qtz. Gabbro 5 Diorite/Gabbro/ Anorthosite P 10 (Foid)-bearing Diorite/Gabbro (Foid)-bearing Alkali Fs.Syenite (Foid) (Foid) Monzosyenite Monzodiorite 60 60 (Foid)olites F The major element chemistry of MORBs Table 13-2. Average analys es and Norm s of MORB glas s es (BVTP Table 1.2.5.2). Oxide W t% All MAR EPR IOR SiO 2 50.53 50.68 50.19 50.93 TiO2 Al 2O3 FeO* MgO CaO Na 2O K 2O 1.56 15.27 10.46 7.47 11.49 2.62 0.16 1.49 15.60 9.85 7.69 11.44 2.66 0.17 1.77 14.86 11.33 7.10 11.44 2.66 0.16 1.19 15.15 10.32 7.69 11.84 2.32 0.14 P 2O5 Total Mg# (m ol) a Norm Q or ab an di hy mt il ap 0.13 99.69 56 0.12 99.7 58 0.14 99.65 53 0.10 99.68 57 0.94 0.95 22.17 29.44 21.62 17.19 4.44 2.96 0.30 0.76 1.00 22.51 30.13 20.84 17.32 4.34 2.83 0.28 0.93 0.95 22.51 28.14 22.50 16.53 4.74 3.36 0.32 1.60 0.83 19.64 30.53 22.38 18.62 3.90 2.26 0.23 A ll: A ve f rom A tlantic, Pacif ic and Indian Ocean ridges. MA R: A ve. f rom Mid-A tlantic Ridge. EPR: A ve. f rom EPR. IOR: A ve. Indian Ocean. a Min. value since all Fe as FeO The major element chemistry of MORBs Originally considered to be extremely uniform, interpreted as a simple petrogenesis More extensive sampling has shown that they display a (restricted) range of compositions MgO and FeO Al2O3 and CaO SiO2 Na2O, K2O, TiO2, P2O5 Figure 13-5. “Fenner-type” variation diagrams for basaltic glasses from the Afar region of the MAR. Note different ordinate scales. From Stakes et al. (1984) J. Geophys. Res., 89, 6995-7028. The common crystallization sequence is: olivine ( Mg-Cr spinel), olivine + plagioclase ( Mg-Cr spinel), olivine + plagioclase + clinopyroxene Figure 7-2. After Bowen (1915), A. J. Sci., and Morse (1994), Basalts and Phase Diagrams. Krieger Publishers. Figure 13-15. After Perfit et al. (1994) Geology, 22, 375-379. The crystal mush zone contains perhaps 30% melt and constitutes an excellent boundary layer for the in situ crystallization process proposed by Langmuir Figure 11-12 From Winter (2001) An Introduction to Igneous and Metamorphic Petrology. Prentice Hall Melt body continuous reflector up to several kilometers along the ridge crest, with gaps at fracture zones, devals and OSCs Large-scale chemical variations indicate poor mixing along axis, and/or intermittent liquid magma lenses, each fed by a source conduit Figure 13-16 After Sinton and Detrick (1992) J. Geophys. Res., 97, 197-216. Some complications N-MORBs and E-MORBs Fast and slow spreading ridges, Harzburgite and Lherzolite ophiolites There must be incompatible-rich and incompatible-poor source regions for MORB magmas in the mantle beneath the ridges N-MORB (normal MORB) taps the depleted upper mantle source Mg# > 65: K2O < 0.10 TiO2 < 1.0 E-MORB (enriched MORB, also called P-MORB for plume) taps the deeper fertile mantle Mg# > 65: K2O > 0.10 TiO2 > 1.0 Trace Element and Isotope Chemistry REE diagram for MORBs Figure 13-10. Data from Schilling et al. (1983) Amer. J. Sci., 283, 510-586. E-MORBs (squares) enriched over N-MORBs (red triangles): regardless of Mg# Lack of distinct break suggests three MORB types E-MORBs La/Sm > 1.8 N-MORBs La/Sm < 0.7 T-MORBs (transitional) intermediate values Figure 13-11. Data from Schilling et al. (1983) Amer. J. Sci., 283, 510-586. N-MORBs: 87Sr/86Sr < 0.7035 and 143Nd/144Nd > 0.5030, depleted mantle source E-MORBs extend to more enriched values stronger support distinct mantle reservoirs for Ntype and E-type MORBs Figure 13-12. Data from Ito et al. (1987) Chemical Geology, 62, 157-176; and LeRoex et al. (1983) J. Petrol., 24, 267-318. Lower enriched mantle reservoir may also be drawn upward and an E-MORB plume initiated Figure 13-13. After Zindler et al. (1984) Earth Planet. Sci. Lett., 70, 175-195. and Wilson (1989) Igneous Petrogenesis, Kluwer. Fast and slow spreading ridges Table 13-1. Spreading rates of some mid-ocean ridge segments. • Slow-spreading ridges: < 3 cm/a • Fast-spreading ridges: > 4 cm/a are considered • Temporal variations are also known Category Ridge Fast East Pacific Rise Slow Latitude Rate (cm/a)* o 21-23 N 3 o 13 N 5.3 o 11 N 5.6 o 8-9 N 6 o 2N 6.3 o 20-21 S 8 o 33 S 5.5 o 54 S 4 o 56 S 4.6 Indian Ocean SW 1 SE 3-3.7 Central 0.9 o Mid-Atlantic Ridge 85 N 0.6 o 45 N 1-3 o 36 N 2.2 o 23 N 1.3 o 48 S 1.8 From Wilson (1989). Data from Hekinian (1982), Sclater (1976), Jackson and Reid (1983). *half spreading et al . Two extension models on ridges High magma flux, magmatism > tectonic Lower magma influx, tectonic > magmatism The Futuna Ridge (W. Pacific), a fast-spreading ridge OSC = Overlaping Spreading Center Schematic view of a fast ridge Oceanic crust of a fast ridge The Vema Fracture Zone (N. Atlantic) A slow ridge The “FAMOUS” area, N. Atlantic Model of a slow ridge Oceanic crust in a slow ridge Pillow-lavas: ophiolitic pillows in the French alps Moho Fast vs. slow ridges No axial valley Important magmatism “complete” sequence (peridotite-gabbrosbasalts) Deep axial valley Moderate magmatism Incomplete sequence “HOT” vs. “LOT” Abundant basalts => thick crust => fast ridge = HOT Moderate amounts of basalts => finer crust => slow ridge = LOT Thermal modelling: melt fraction under fast and slow ridges K2O MgO CaO MORB 0.16 7.5 11.5 DM 0.1 31 5 Residues for successive F values: Restite composition F= 0.10 31.24 4.93 0.02 0.10 31.48 4.87 0.05 0.10 32.24 4.66 0.1 0.09 33.61 4.28 0.2 0.09 36.88 3.38 0.25 0.08 38.83 2.83 0.3 0.07 41.07 2.21 0.4 0.06 46.67 0.67 0.43 0.05 48.73 0.10 14.00 12.00 MORB 10.00 CaO 0.01 8.00 6.00 DM 4.00 Residues for increasing F 2.00 0.00 0.00 10.00 20.00 30.00 MgO 40.00 50.00 60.00 Melt abundant = fast ridge = thick crust = depleted mantle, HOT Melt moderate = slow ridge = fine crust = less depleted mantle, LOT