partial melting

Post on 02-Feb-2016

48 Views

Category:

Documents

0 Downloads

Preview:

Click to see full reader

DESCRIPTION

Partial melting. 1. Binary and ternary phase diagrams; melting of the mantle. 1 - C Systems. The system SiO 2. After Swamy and Saxena (1994) , J. Geophys. Res., 99 , 11,787-11,794 . AGU. 1900. 1890. Liquid. a. 1700. b. c. Olivine. T o C. plus. Liquid. d. 1500. Olivine. 1300. - PowerPoint PPT Presentation

TRANSCRIPT

Partial melting

1. Binary and ternary phase diagrams; melting of the mantle

1 - C Systems1 - C SystemsThe system SiOThe system SiO22

Stishovite

Coesite

- quartz

- quartz

Liquid

TridymiteCristobalite

600 1000 1400 1800 2200 2600

2

4

6

8

10P

ress

ure

(GP

a)

Temperature oC

After Swamy and Saxena (1994), J. Geophys. Res., 99, 11,787-11,794. AGU

The Olivine SystemThe Olivine SystemFo - FaFo - Fa (Mg (Mg22SiOSiO44 - Fe - Fe22SiOSiO44))

also a solid-solution seriesalso a solid-solution series

Isobaric T-X phase diagram at atmospheric pressure (After Bowen and Shairer (1932), Amer. J. Sci. 5th Ser., 24, 177-213.

Fo20 40 60 80Fa

1300

1500

1700

1890

1205

T oC

Olivine

Liquid

Liquid

plus

1900

a

b c

d

Wt.% Forsterite

Olivine

2-C Eutectic Systems2-C Eutectic Systems Example: Diopside - AnorthiteExample: Diopside - Anorthite

No solid solutionNo solid solution

1274

Di 20 40 60 80 An

1200

1300

1400

1500

1600

T oC

Anorthite + Liquid

Liquid Liquidus

Diopside + Liquid

Diopside + Anorthite

1553

1392

Wt.% Anorthite

Isobaric T-X phase diagram at atmospheric pressure (After Bowen (1915), Amer. J. Sci. 40, 161-185.

Melting in a binary system

• An-rich composition (right of the eutectic)

• Di-rich composition

C = 3: Ternary Systems:Example 1: Ternary Eutectic

Di - An - Fo

TT

MM

AnorthiteAnorthite

ForsteriteForsterite

DiopsideDiopside

Note three binary Note three binary eutecticseutectics

No solid solutionNo solid solution

Ternary eutectic = MTernary eutectic = M

T - X Projection of Di - An - Fo

Figure 7-2. Isobaric diagram illustrating the liquidus temperatures in the Di-An-Fo system at atmospheric pressure (0.1 MPa). After Bowen (1915), A. J. Sci., and Morse (1994)(1994), Basalts and , Basalts and Phase Diagrams. Phase Diagrams. Krieger Publishers.Krieger Publishers.

An + Liq

Liquid

Di + Liq

Di + An

aAn

Melting in a ternary

• Consider a composition close to the Fo apex and with Di>An (mantle-like)

Effect of pressureEffect of pressure

Figure 7-16. Effect of lithostatic pressure on the liquidus and eutectic composition in the diopside-anorthite system. 1 GPa data from Presnall et al. (1978). Contr. Min. Pet., 66, 203-220.

Pressure effects:

Figure 10-8 Figure 10-8 After Kushiro (1968), After Kushiro (1968), J. Geophys. Res.J. Geophys. Res., , 7373, 619-634., 619-634.

NeNe

FoFo EnEn

AbAb

SiOSiO22

Oversaturated(quartz-bearing)tholeiitic basalts

Highly undesaturated

(nepheline - b

earing)

alkali basalts

Undersaturated

tholeiitic basalts

EE3GPa3GPa

EE 2Gpa2Gpa

EE1GPa1GPa

EE 1atm1atm

Volatile-freeVolatile-free

NB

• Do you remember – alkaline vs. Sub-alkaline series?

Effect of waterEffect of water

Figure 7-25. The effect of H2O on the

diopside-anorthite liquidus. Dry and 1 atm from Figure 7-16, PH2O = Ptotal curve

for 1 GPa from Yoder (1965). CIW Yb 64.

Figure 7-20.Figure 7-20. Experimentally determined melting intervals of gabbro under H Experimentally determined melting intervals of gabbro under H22O-free (“dry”), and O-free (“dry”), and

HH22O-saturated conditions. After Lambert and Wyllie (1972).O-saturated conditions. After Lambert and Wyllie (1972). J. Geol., 80, 693-708. J. Geol., 80, 693-708.

Ne

Fo En

Ab

SiO2

Oversaturated(quartz-bearing)tholeiitic basalts

Highly undesaturated(nepheline-bearing)

alkali olivinebasalts

Undersaturated

tholeiitic basalts

3GPa2GPa

1GPa

1atm

Volatile-free

Ne

Fo En

Ab

SiO2

Oversaturated(quartz-bearing)tholeiitic basalts

Highly undesaturated(nepheline-bearing)

alkali olivinebasalts

Undersaturated

tholeiitic basalts

CO2

H2Odry

P = 2 GPa

Effect of Pressure, Water, and COEffect of Pressure, Water, and CO2 2 on the positionon the position

of the eutectic in the basalt systemof the eutectic in the basalt systemIncreased pressure moves theIncreased pressure moves theternary eutectic (first melt) fromternary eutectic (first melt) fromsilica-saturated to highly undersat.silica-saturated to highly undersat.alkaline basaltsalkaline basalts

Water moves the (2 Gpa) eutecticWater moves the (2 Gpa) eutectictoward higher silica, while COtoward higher silica, while CO22

moves it to more alkaline typesmoves it to more alkaline types

> 4 Components

Figure 7-13. Pressure-temperature phase diagram for the melting of a Snake River (Idaho, USA) tholeiitic basalt under anhydrous conditions. After Thompson (1972). Carnegie Inst. Wash Yb. 71

Experiments on melting mantle samples:

• Tholeiite easily created

by 10-30% PM

• More silica saturated

at lower P

• Grades toward alkalic

at higher PFigure 10-17a. Figure 10-17a. After Jaques and Green (1980).After Jaques and Green (1980). Contrib. Mineral. Petrol., 73, 287-310.Contrib. Mineral. Petrol., 73, 287-310.

• Figures not used

15

10

5

00.0 0.2 0.4 0.6 0.8

Wt.

% A

l 2O3

Wt.% TiO2

DuniteHarzburgite

Lherzolite

Tholeiitic basalt

Partia

l Melt

ing

Residuum

Source, melt and residuum:Source, melt and residuum:

Figure 10-1 Figure 10-1 Brown and Brown and Mussett, A. E. (1993), Mussett, A. E. (1993), The Inaccessible Earth: The Inaccessible Earth: An Integrated View of Its An Integrated View of Its Structure and Structure and Composition. Composition. Chapman Chapman & Hall/Kluwer.& Hall/Kluwer.

ObliqueObliqueViewView

IsothermalIsothermalSectionSection

Figure 7-8.Figure 7-8. Oblique view illustrating an isothermal section through the diopside-albite-anorthite Oblique view illustrating an isothermal section through the diopside-albite-anorthite system. system. Figure 7-9.Figure 7-9. Isothermal section at 1250 Isothermal section at 1250ooC (and 0.1 MPa) in the system Di-An-Ab. Both from C (and 0.1 MPa) in the system Di-An-Ab. Both from Morse (1994)Morse (1994), Basalts and Phase Diagrams. Krieger Publishers., Basalts and Phase Diagrams. Krieger Publishers.

Partial melting

2. Melting reactions, experimental petrology

Melting of the crust

Qz-Ab-Or + H2O

At 1 kbar (supersolvus) At 5 kbar (subsolvus)

Chapter 18: Granitoid Rocks Chapter 18: Granitoid Rocks

Figure 18-3. The Ab-Or-Qtz system with the ternary cotectic curves and eutectic minima from 0.1 to 3 GPa. Included is the locus of most granite compositions from Figure 11-2 (shaded) and the plotted positions of the norms from the analyses in Table 18-2. Note the effects of increasing pressure and the An, B, and F contents on the position of the thermal minima. From Winter (2001) An Introduction to Igneous and Metamorphic Petrology. Prentice Hall.

5um powder

12.7mm

Incongruent melting reactions

(Limpopo SMZ, Ga-Mathule village, E. of Bandelierkop)

Chapter 18: Chapter 18: Granitoid Rocks Granitoid Rocks

Figure 18-5. a. Simplified P-T phase diagram and b. quantity of melt generated during the melting of muscovite-biotite-bearing crustal source rocks, after Clarke (1992) Granitoid Rocks. Chapman Hall, London; and Vielzeuf and Holloway (1988) Contrib. Mineral. Petrol., 98, 257-276. Shaded areas in (a) indicate melt generation. Winter (2001) An Introduction to Igneous and Metamorphic Petrology. Prentice Hall.

• 2 generations of melt in a single outcrop ?– M1: Bt still stable

(Q+KSp+Ph+H2O=M)

– M2: incongruent melting yielding crd

(Velay dome, french hercynian belt)

Melting of an heterogeneous crust

• Orthogneiss: Qz-Pg-Bt

• Paragneiss: Or-Ab-Qz-Bt-AlS

• Shear zone: add water to the above

• What will melt, at what temperature, with which melting reaction?

NB- this is a simplified model!

• Slides not used

Figure 18-8. Schematic models for the uplift and extensional collapse of orogenically thickened continental crust. Subduction leads to thickened crust by either continental collision (a1) or compression of the continental arc (a2), each with its characteristic orogenic magmatism. Both mechanisms lead to a thickened crust, and probably thickened mechanical and thermal boundary layers (“MBL” and “TBL”) as in (b) Following the stable situation in (b), either compression ceases (c1) or the thick dense thermal boundary layer is removed by delamination or convective erosion (c2). The result is extension and collapse of the crust, thinning of the lithosphere, and rise of hot asthenosphere (d). The increased heat flux in (d), plus the decompression melting of the rising asthenosphere, results in bimodal post-orogenic magmatism with both mafic mantle and silicic crustal melts. Winter (2001) An Introduction to Igneous and Metamorphic Petrology. Prentice Hall.

Partial melting

3. Migmatites and melt extraction

Partially molten rocks

MESOSOME = Not melted

LEUCOSOME = Liquid = granitic magma

MELANOSOME = Residue

Biot

Plg

QzKF

Biot

Plg

Qz KF

MetatexitesDiatexites

« Dirty » granites

Rheology of partially molten systems

Melt extraction

Brown, 1994

Melt depletion

An experimental study of melt extraction

J. Barraud, PhD 2000

Films

Exp39.avi

(Films)

Exp32.avi

Exp43.avi

Evolution de la déformation1) 5% shortening

2) 22% shortening

4) 36% shortening

3) 30% shortening

Asymetrical fold; shear zone on one flank

Strain localization in liquid patches.

Zone de cisaillement

Bande de cisaillement

Melt extraction: role of deformation

Burg et al., 1994

Melting and migmatitic domes – migmatites in orogenic belts

The Velay dome

• Slides not used

top related