Igneous Petrology John Winter. The Earth’s Interior Crust: Oceanic crust Thin: 10 km Relatively uniform stratigraphy = ophiolite suite: = ophiolite suite:

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Igneous Petrology John Winter

The Earth’s Interior Crust: Oceanic crust Thin: 10 km Relatively uniform stratigraphy = ophiolite suite: = ophiolite suite: F Sediments F pillow basalt F sheeted dikes F more massive gabbro F ultramafic (mantle) Continental Crust Thicker: km average ~35 km Highly variable composition u Average ~ granodiorite

The Earth’s Interior Mantle: Peridotite (ultramafic) Upper to 410 km (olivine  spinel) u Low Velocity Layer km Transition Zone as velocity increases ~ rapidly  660 spinel  perovskite-type  Si IV  Si VI Lower Mantle has more gradual velocity increase Figure 1-2. Major subdivisions of the Earth. Winter (2001) An Introduction to Igneous and Metamorphic Petrology. Prentice Hall.

The Earth’s Interior Core: Fe-Ni metallic alloy Outer Core is liquid u No S-waves Inner Core is solid Figure 1-2. Major subdivisions of the Earth. Winter (2001) An Introduction to Igneous and Metamorphic Petrology. Prentice Hall.

Figure 1-3. Variation in P and S wave velocities with depth. Compositional subdivisions of the Earth are on the left, rheological subdivisions on the right. After Kearey and Vine (1990), Global Tectonics. © Blackwell Scientific. Oxford.

Figure 1-5. Relative atomic abundances of the seven most common elements that comprise 97% of the Earth's mass. An Introduction to Igneous and Metamorphic Petrology, by John Winter, Prentice Hall.

The Pressure Gradient P increases =  gh P increases =  gh l Nearly linear through mantle u ~ 30 MPa/km   1 GPa at base of ave crust Core:  incr. more rapidly since alloy more dense Core:  incr. more rapidly since alloy more dense Figure 1-8. Pressure variation with depth. From Dziewonski and Anderson (1981). Phys. Earth Planet. Int., 25, © Elsevier Science.

Heat Sources in the Earth 1. Heat from the early accretion and differentiation of the Earth u still slowly reaching surface

Heat Sources in the Earth 1. Heat from the early accretion and differentiation of the Earth u still slowly reaching surface 2. Heat released by the radioactive breakdown of unstable nuclides

Heat Transfer 1. Radiation 2. Conduction 3. Convection

The Geothermal Gradient Figure 1-11(new). Estimates of oceanic (blue curves) and continental shield (red curves) geotherms to a depth of 300 km. The thickness of mature (> 100Ma) oceanic lithosphere is hatched and that of continental shield lithosphere is yellow. Data from Green and Falloon ((1998), Green & Ringwood (1963), Jaupart and Mareschal (1999), McKenzie et al. (2005 and personal communication), Ringwood (1966), Rudnick and Nyblade (1999), Turcotte and Schubert (2002).

The Geothermal Gradient Pattern of global heat flux variations compiled from observations at over 20,000 sites and modeled on a spherical harmonic expansion to degree 12. From Pollack, Hurter and Johnson. (1993) Rev. Geophys. 31, Cross-section of the mantle based on a seismic tomography model. Arrows represent plate motions and large-scale mantle flow and subduction zones represented by dipping line segments. EPR =- East pacific Rise, MAR = Mid- Atlantic Ridge, CBR = Carlsberg Ridge. Plates: EA = Eurasian, IN = Indian, PA = Pacific, NA = North American, SA = South American, AF = African, CO = Cocos. From Li and Romanowicz (1996). J. Geophys. Research, 101, 22,

Figure 1-9. Estimated ranges of oceanic and continental steady- state geotherms to a depth of 100 km using upper and lower limits based on heat flows measured near the surface. After Sclater et al. (1980), Earth. Rev. Geophys. Space Sci., 18,

Plate Tectonic - Igneous Genesis 1. Mid-ocean Ridges 2. Intracontinental Rifts 3. Island Arcs 4. Active Continental Margins 5. Back-arc Basins 6. Ocean Island Basalts 7. Miscellaneous Intra- Continental Activity u kimberlites, carbonatites, anorthosites...