E N D
1. Structure of the Ocean Lithosphere How do we know the structure of the lithosphere?
Geophysical data
Seismic reflection and refraction, magnetics, gravity, heat flow
Dredges and cores (fracture zones)
Seafloor mapping
Side scan sonar, Gloria (Geological Long Range Inclined Asdic), swath mapping, deep tow mapping, direct observation (Alvin)
Ophiolites
2. Structure of the Ocean Lithosphere
3. Ocean Lithosphere Layer 1
Deep sea sediments, often include radiolarian cherts
4. Ribbon Chert
5. Structure of the Ocean Lithosphere
6. Layer 2
2A, 2B and 2C- change in seismic velocity
2A = pillow lavas and sheet flows (extrusive) with voids
2B = pillow lavas and sheet flows (extrusive) with void filling clays and minerals
2C = sheeted dikes- injected into fractures in the ocean crust (intrusive), ~ 1 m wide Ocean Lithosphere
7. Structure of the Ocean Lithosphere
8. Layer 3
Massive gabbro
Layer 4
Layered peridotite – ultramafic cumulates
Massive peridotite
Ocean Lithosphere
9. Ocean Lithosphere- Seismic Velocities
10. Ocean Lithosphere- The Moho
11. Ocean Lithosphere Models
12. Data indicate large magma chambers are short-lived or non existent
Instead injection of crystal mush- starts to crystallize during ascent
Fast-spreading- lens of magma over the xl mush
Slow-spreading- narrower mush zone (less supply), no lens of magma Ocean Lithosphere
13. Ocean Lithosphere- Geochemistry (abridged) MORB = tholeiitic basalts
Produced by partial melt of depleted mantle material
Depleted Mantle- subject to previous melt event which removed already removed incompatible elements
14. Ocean Lithosphere- Geochemistry (abridged) Incompatible Elements (partitioned into melt)
Elements that that have difficulty in entering cation sites of the minerals
are concentrated in the melt phase of magma
HFS (High Field Strength)- high charge, highly insoluble in water dominated fluids, (Nb, Ta, Ti. Zr, Hf)
LIL (Large Ion Lithophile)- 1+ and 2+ large ion elements that tend to be concentrated in silica melts, high radius/charge (K, Rb, Cs, Sr, Pb, Ba)
15. Ocean Lithosphere-Geochemistry
16. Ocean Lithosphere-Geochemistry Magma Series- evolution of mafic magma
Tholeiites- lower Na, produced from reduced magmas. First xlz Mg-rich olivines and pyroxenes (Bowen’s Rxn Series), Mg/Fe decreases
Rifting environments- partial melt of depleted mantle
Calc-Alkaline- higher Na, produced from oxidized magmas. Fe oxidized ? magnetite , Mg/Fe more constant
Subduction zones- partial melt of depleted mantle plus subducted material (hydrated)
17. Ocean Lithosphere-Geochemistry Magma Series
Alkaline- higher Na and K relative to SiO2. More enriched in incompatibles.
Ocean island-hotspot environments- partial melt of more primitive mantle
18. Ocean Lithosphere-Geochemistry
19. What happens to the crust after it forms?
Aging process
Contracts, cools, deepens (density)
Increase in seismic velocity of the upper crust
Decrease in conductive and convective heat flow
Decrease in remnant magnetism Ocean Lithosphere
20. Age-Depth relationship
Young, hot, buoyant ? older, cooler, more dense
Depth to the ocean crust increases systematically with age Aging of Ocean Crust
21. Aging of Ocean Crust
22.
Limitations
Only applicable to ~80 Ma, after that lithosphere mostly cooled, nearing equilibrium
Not all ridges start at 2500 m Aging of Ocean Crust
23. Increased seismic velocity
Rocks become more dense with age due to:
Cooling and contracting
Infilling of pore spaces and fractures (calcite and zeolite cements- usually related to fluid flow Aging of Ocean Crust
24. Aging of CrustSeismic Velocity
25. Heat Flow
Lithosphere cools through
Conduction- diffusion of heat from hot lithosphere to cold seawater or sediment interface
Convection- transfer of heat by mass movement
Heat flow decreases with age Aging of Ocean Crust
26. Aging of Ocean Crust
27. Decreased remnant magnetization
Remnant = permanent magnetization induced by an applied field
Low temperature alteration of the crust includes oxidation of titanomagnetites ? decreased magnetization
Greatest change over the first 20 Ma Aging of Ocean Crust
28. Where is ocean crust forming?
29. Spreading Centers
Mid ocean ridges (tholeiitic basalt)
Hotspots tracks/Aseismic Ridges
Hawaii, Line Islands
Walvis Ridge, Rio Grande Rise, Ninety-east Ridge
Large igneous provinces- voluminous outpourings of mafic material
Ontong Java Plateau, Kerguelen, Deccan Formation of Ocean Crust
30.
33. Formation of Ocean Crust Today ~90% of new ocean crust is formed at the mid ocean ridge
Crustal production rate ~1.8 x 106 km3/my
During Cretaceous ~70% of new ocean crust formed at the mid ocean ridge, 30% formed at hot spots (large igneous provinces)
Crustal production rate ~3.3 x 106 km3/my
Hotspot activity may exceed ridge processes for short intervals
34. Formation of Ocean Crust
35. Formation of Ocean Crust Implications of LIPs
Thickening of ocean crust
Ontong Java ~40 km; Kerguelen ~25 km
Reheat and uplift surrounding lithosphere
Resist subduction? Nucleus for continent?
Sea level
Greenhouse gases
36. Suggests 2 modes of heat and mass transfer from the mantle
Prevalence of each mode varies through time
Related to activity at the core/mantle boundary?
Heat flux from plumes ~ cooling of the core
Present day
60% of plume flux in the Pacific
Formation of Ocean Crust
37. Hot Spots What are their source depths?
CMB (D”), 670 discontinuity, both…
What is the link to climate?
Greenhouse gases, sea level, circulation…
What determines the location of a hotspot?
Distance from ridge, random…
What triggers hotspot activity?
Continental breakup, plate reorganization, core processes…