petrology petrology igneous and metamorphic convection demo “lava lamp” density displacement...
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PetrologyPetrologyIgneous and Metamorphic
Convection demo “Lava Lamp”Density displacement demo: oil and water are immiscible.Marble Demo :Fractionation
The Texts
• An Introduction to Igneous and
Metamorphic Petrology 1st ed by J. D. Winter• or Principles of Igneous and Metamorphic
Petrology J.D. Winter 2nd ed.
The Earth’s InteriorThe Earth’s InteriorCrust:Oceanic crust
Usually < 10 km
ophiolite suite: list
Continental CrustThicker: 20-90 km average ~35 km
Variable composition but average a granodiorite
O2 -
O2 -
O2 -
O2 -
Si4+
2_25
The Silicate Tetrahedron
The basis of most rock-forming minerals, charge - 4
The Earth’s InteriorThe Earth’s InteriorMantle:Mantle:Peridotite (ultramafic)Peridotite (ultramafic)
Upper Mantle Upper Mantle to 410 kmto 410 km
olivine, pyroxenes, spinel - structure minerals, olivine, pyroxenes, spinel - structure minerals, and garnet and garnet
Low Velocity Layer Low Velocity Layer 60-220 km 60-220 km AesthenosphereAesthenosphere
Transition Zone Transition Zone as velocity increases 410 - as velocity increases 410 - 660 km , olivine not stable, replaced by 660 km , olivine not stable, replaced by high P polymorphs with ~ same high P polymorphs with ~ same composition: wadsleyite (beta-spinel composition: wadsleyite (beta-spinel structure), and ringwoodite (gamma-spinel structure), and ringwoodite (gamma-spinel structure) structure)
Lower Mantle Lower Mantle 660 Upper minerals unstable, 660 Upper minerals unstable, perovskite-type structure perovskite-type structure SiSiIVIV Si SiVIVI
The Earth’s InteriorThe Earth’s Interior
Core: Core: Fe-Ni metallic alloyFe-Ni metallic alloy
SulfurSulfur
Outer CoreOuter Core is liquidis liquid No S-wavesNo S-waves
Inner CoreInner Core is solidis solid
Discussions: Differentiation Iron Meteorites, ImpactorDensity and Buoyancy
Source: Recommended Text Kearey and Vine (1990), Global Tectonics.
Note how S-wave velocities drop to zero in the Liquid outer core
LVZ
Upper Mantle SamplesUpper Mantle Samples• Samples of the upper mantle occasionally appear Samples of the upper mantle occasionally appear
where faulting has exposed it in oceanic fracture where faulting has exposed it in oceanic fracture zones, thrust it up in collision zones, or where brought zones, thrust it up in collision zones, or where brought up in diatreme and basalt eruptions. The rock revealed up in diatreme and basalt eruptions. The rock revealed is usually is usually PeridotitePeridotite, which is three-quarters Dunite , which is three-quarters Dunite (pure olivine) and one-quarter basalt. The Basalt forms (pure olivine) and one-quarter basalt. The Basalt forms by the partial melting of this peridotite, which drives off by the partial melting of this peridotite, which drives off the basaltic melt, leaving behind the solid “the basaltic melt, leaving behind the solid “depleteddepleted “ “ dunite (basaltic components removed). dunite (basaltic components removed).
• The original (fertile) mantle has more Al, Ca, Ti, Na, and K and The original (fertile) mantle has more Al, Ca, Ti, Na, and K and lower Mg# = Mg/(Mg +Fe) than Dunitelower Mg# = Mg/(Mg +Fe) than Dunite
So some of the above go into the basalt.
Molten- Molten- VERYVERY Hot HotNo solids
Molten- Not so hotMolten- Not so hot
100% Solid
First mineral to crystallize outIndependent TetrahedraIndependent Tetrahedra
SingleSinglechainschains
DoubleDoublechainschains
sheetssheets
3-D3-D
3-D3-D3-D3-D
“Basaltic”
“Andesitic”
“Granitic”
Fo Mg++ 1900C Fa Fe++ 1500C
1900 oC
1553 oC
3-D3-D
sheets
Fine crystalsNeed a microscope
Course crystalsEasily seen
Low silica, HOT, fluid High silica, warm, viscousIntermediate
Dark Green Gray Pink to SalmonGray
If crystals are left in contact with melt …If crystals are left in contact with melt …
• Ultramafic to Basaltic• Gray needles are
Plagioclase (Plag) Feldspar, Yellow-brown crystals are Pyroxene (Py), brightly colored crystals are Olivine (Ol). At lower Temps, the Olivine xtals have been partially resorbed by the melt, their atoms reused to make Py & Plag.
http://www4.nau.edu/meteorite/Meteorite/Eucrite.html
Plagioclase Feldspar
Zoned feldspar (plagioclase) showing change in composition with time in magma chamber (calcium-rich in core to sodium-rich at rim)
If the first formed crystals of Calcium-rich (Ca) Plagioclase Feldspar are left in contact with the melt , as the melt cools more stable sodium-rich layers will be deposited on their outer rims
Stable composition varies with Temperature
Isolated Olivine crystalsIsolated Olivine crystals
• Early formed Olivine crystals can sink to the bottom of a magma chamber, so they are isolated from the very reactive ions in the melt.
If early crystals are removed (isolated), the If early crystals are removed (isolated), the melt becomes richer in Silicamelt becomes richer in Silica
A melt will crystallize its mafic components first, and the remaining melt may be granitic
Remove Fe, Mg, CaSome Si
Left withK and AlMost of Si
You can start with aMafic (silica-poor) magmaand end up with some Felsic (silica-rich)Granites.
Marble Demo
Pressure GradientPressure Gradient
• P increases = gh
1 GPa at base of crust
• Linear increase mantle~ 30 MPa/km
• Core: increases more rapidly since Fe-Ni alloy more dense
We need to be able to estimate pressures
Pressure Calcs Pressure Calcs
• To calculate pressures at the base of a stack of layers with different densities, start from the top layer, calculate the pressure at the base as
• P0-1 = 0-1gh0-1
• For the second layer,
• P2 = P0-1 + 1-2gh1-2
Etc.
Multi-layer Pressure Calc Example Multi-layer Pressure Calc Example • Upper crust 25 km thick, density 2.75 Mg/m3
0-1 = 2.75 Mg/m3 x 1000 kg/1Mg = 2.75 x 103 kg/m3
• P1 = 0-1gh0-1
• = 2.75 x 103kg/m3 2 x 9.81 m/s2 x 25 x 103 m• = 6.744 x 108 kg . m/s2 x 1/m2 (aka “Pascals”)• Next layer down, 10 km basalt 1-2 = 3 x 103 kg/m3
• P2 = P1 + 1-2gh1-2
Etc. See the handout, after the lecture
Olivine ExampleOlivine Example• At high TP, the At high TP, the olivine structure is no longer stable. olivine structure is no longer stable.
• Below depths of about 410 km olivine undergoes an Below depths of about 410 km olivine undergoes an exothermicexothermic phase phase transition to the sorosilicate, wadsleyite , the transition to the sorosilicate, wadsleyite , the Olivine Olivine
• At about 520 km depth, wadsleyite transforms exothermically into ringwoodite, At about 520 km depth, wadsleyite transforms exothermically into ringwoodite, the the Olivine, which has the spinel structure. Olivine, which has the spinel structure.
• At a depth of about 670 – 700 km ringwoodite decomposes into silicate At a depth of about 670 – 700 km ringwoodite decomposes into silicate
perovskite ((Mg,Fe)SiO3) and ferropericlase ((Mg,Fe)O) in an perovskite ((Mg,Fe)SiO3) and ferropericlase ((Mg,Fe)O) in an endothermicendothermic reaction. reaction.
• These phase transitions lead to a discontinuous increase in the density of the These phase transitions lead to a discontinuous increase in the density of the Earth's mantle that can be observed by seismic methods. They are also thought Earth's mantle that can be observed by seismic methods. They are also thought to influence the dynamics of mantle convection in that the exothermic transitions to influence the dynamics of mantle convection in that the exothermic transitions reinforce flow across the phase boundary, whereas the endothermic reaction reinforce flow across the phase boundary, whereas the endothermic reaction hampers it.hampers it.
• This leads some workers to believe that the 700 km boundary blocks convection This leads some workers to believe that the 700 km boundary blocks convection from the core mantle boundary, and upper mantle convection cells are distinct.from the core mantle boundary, and upper mantle convection cells are distinct.
Exothermic materials heat, expand, more buoyant
Phase diagram for aluminous Phase diagram for aluminous 4-phase Lherzolite:4-phase Lherzolite:
Ca++ PlagioclaseCa++ Plagioclase shallow (< 50 km)shallow (< 50 km)
Spinel Spinel Lherzolite Spinel is MgAl2O4
50-80 km50-80 km Garnet Garnet Lherzolite
80-400 km80-400 km Si[4] Si[4] Si[6] coord. Si[6] coord.
> 400 km> 400 km
Al-phase =Al-phase =
Figure 10-2 Figure 10-2 Phase diagram of aluminous Lherzolite with melting interval (gray), sub-solidus Phase diagram of aluminous Lherzolite with melting interval (gray), sub-solidus reactions, and geothermal gradient. After reactions, and geothermal gradient. After Wyllie, P. J. (1981). Geol. Rundsch. 70, 128-153.Wyllie, P. J. (1981). Geol. Rundsch. 70, 128-153.
Notice the mantle will not melt under normal ocean geotherm!
Si [4] => Si [6]
Heat Sources Heat Sources in the Earthin the Earth
• Impact heat from the early accretion and differentiation of the Earth
– Convection cells redistribute heat to cold surface
Heat Sources Heat Sources in the Earthin the Earth
1.1. Heat from the early accretion and Heat from the early accretion and differentiation of the differentiation of the
EarthEarth still slowly reaching surfacestill slowly reaching surface
2.2. Heat released by the radioactive Heat released by the radioactive breakdown of unstable nuclidesbreakdown of unstable nuclides
Heat TransferHeat Transfer1. Radiation
Requires transparent mediumRocks aren’t (except perhaps at great depth)
2. ConductionRocks are poor conductorsVery slow
3. ConvectionMaterial movement (requires ductility)Heat-induced expansion and buoyancyMuch more efficient than conduction
Geothermal Geothermal
GradientGradient Silica-rich rocks (with Quartz, K-feldspar) melt at cooler temperatures. Melts are viscous
Silica-poor rocks (with Olivine, Pyroxene, Ca-feldspar) melt at higher temperatures Melts are very fluid Hot
Cool
Ocean and Continental Ocean and Continental Lithosphere Thermal GradientsLithosphere Thermal Gradients
Melting depths vary w\ volcanic provinceMelting depths vary w\ volcanic provinceMost within upper few hundred kilometersMost within upper few hundred kilometers
Origin of Basaltic Magma - MOROrigin of Basaltic Magma - MOR
• Role of Role of Pressure in divergent marginPressure in divergent margin– Reducing the pressure lowers the melting Reducing the pressure lowers the melting
temperature – the mantle partially meltstemperature – the mantle partially melts– Mid-ocean ridge and rift valley: called Mid-ocean ridge and rift valley: called
decompression meltingdecompression melting
Harry Hess’ Seafloor Spreading
http://volcanoes.usgs.gov/about/edu/dynamicplanet/nutshell.php
Mantle loses heat at Mantle loses heat at surface, becomes surface, becomes denser. Pulls denser. Pulls lithosphere down into lithosphere down into “Subduction Zone”“Subduction Zone”
Origin of Basaltic Magma 2 Origin of Basaltic Magma 2 Subduction ZoneSubduction Zone
• Role of volatiles - WATERRole of volatiles - WATER
INITIALLY BASALTIC
Assimilation and magmatic Assimilation and magmatic differentiation differentiation
Show Samples
Why are the continents so silica rich? Weathering dissolves high-temp. minerals, but also:
Fractionation: if early crystals settle out, remaining melt is relatively richer in silica
Origin of Andesite & Diorite:Origin of Andesite & Diorite: intermediate silica contentintermediate silica content
Good diagram for the Andes Mountains
Small blobs, not much heat in themAssimilate some crust, fractionate
Basaltic here
Origin of Granitic RocksOrigin of Granitic Rocks
Can also get small amounts of granites from deep felsic rock passed by ascending magma
Huge blobs w/ low temps but lots of magma, fractionation & assimilation => Granite Batholiths
Magma rises further distance, more fractionation. Passes through thicker crust, more assimilation.
Plate Tectonic - Igneous GenesisPlate Tectonic - Igneous Genesis
1. Mid-ocean Ridges
2. Intracontinental Rifts
3. Island Arcs
4. Active Continental
Margins
5.5. Back-arc BasinsBack-arc Basins
6.6. Ocean Island BasaltsOcean Island Basalts
7.7. Miscellaneous Intra-Miscellaneous Intra-Continental Continental
ActivityActivity kimberlites, carbonatites, kimberlites, carbonatites,
anorthosites...anorthosites...
Or, for Kimberlites (7)Or, for Kimberlites (7)
Many workers think plumes from the core-mantle boundary can punch through the endothermic 670-700 km transition. Diamonds formed from subducted organic carbon are lifted by rising plumes that happen to hit a subducted slab of ocean lithosphere.