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Igneous Petrology
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Lecture 1 Introduction and the Earth’s Interior
Wednesday, January 26th, 2005
IGNEOUSand
METAMORPHIC PETROLOGY
GEO - 321
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PETROLOGY – comes from petros for rock – hence the study of rocks
Sedimentary – deposition of material from water or air
Igneous – formed through the solidification of molten material
Metamorphic – formed from a previously existing rock (usually at high temperatures and pressures)
PETROLOGY encompasses:-1. Description of rocks2. Their classification3. Generation and interpretation of data4. Theories on how these rocks formed
Tools of the trade include:-1. Field relationships2. Hammer and hand lens3. Thin sections and petrological microscope4. Mineralogy and electron microprobe5. Major element data6. Trace element data7. Isotopic data8. High pressure and temperature experiments
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The Earth’s InteriorCrust:Oceanic crust
Thin: 5-10 kmRelatively uniform stratigraphy
= ophiolite suite:Sedimentspillow basaltsheeted dikesmore massive gabbroultramafic (mantle)
Continental CrustThicker: 20-90 km average ~35 kmHighly variable composition
Average ~ granodiorite
The Earth’s Interior
Mantle:Peridotite (ultramafic)
Upper to 410 km (olivine → spinel) Low Velocity Layer 60-220 km
Transition Zone as velocity increases ~ rapidly660 spinel → perovskite-type
SiIV → SiVI
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.
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The Earth’s Interior
Core: Fe-Ni metallic alloy
Outer Core is liquidNo 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.
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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 = ρghNearly linear through mantle
~ 30 MPa/km≈ 1 GPa at base of ave crust
Core: P incr. more rapidly since alloy more dense
Figure 1-8. Pressure variation with depth. From Dziewonski and Anderson (1981). Phys. Earth Planet. Int., 25, 297-356. © Elsevier Science.
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Some useful pressure conversions:
1 bar = 102 * 103 Pa1 kbar = 102 * 106 Pa = 102 MPa = 0.1 Gpa10 kbar = 1.02 * 109 Pa = 1 GPa
Approximate pressure gradients in the crust and mantle
Crust: 30 MPa/km or 0.29 kb/km
Mantle: 35 MPa/km or 0.35 Kb/km
What will the gradients be in GPa?
Calculate pressure at depthPressure = Density x Acceleration due to gravity x Depth
Garnet peridotite is thought to start melting at a depth ofabout 130 km in the mantle to produce Hawaiian basalts.Assuming the density of mantle peridotite is 3.3 gm/cc, Calculate the pressure of melting
IMPORTANT for Pa, units need to be in kg and m
P (Pa) = 3300 kg x 9.8 m x 130,000 mm3 s2
= 4.2 x 109
= 4.2 GPa
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Heat Sources in the Earth
1. Heat from the early accretion and differentiation of the Earthstill slowly reaching surface
Heat Sources in the Earth
1. Heat from the early accretion and differentiation of the Earthstill slowly reaching surface
2. Heat released by the radioactive breakdown of unstable nuclides
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The Geothermal Gradient
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, 269-311.
Plate Tectonic - Igneous Genesis
1. Mid-ocean Ridges2. Intracontinental Rifts3. Island Arcs4. Active Continental
Margins
5. Back-arc Basins6. Ocean Island Basalts7. Miscellaneous Intra-
Continental Activitykimberlites, carbonatites, anorthosites...