Petrology Lecture 5

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Petrology Lecture 5

Reaction Series and Melting Behavior

GLY 4310 - Spring, 2016

1

Norman Levi Bowen

• Canadian geologist who was one of the most important pioneers in the field of experimental petrology

• Widely recognized for his phaseequilibrium studies of silicate systems as they relate to the origin of igneous rocks

Reaction principle . He recognized two types of reaction, continuous and discontinuous . (1922)

• 1887 - 1956

2

Continuous Reaction

Mineral

A

 Melt

X

 Mineral

B

 Melt

Y

Melt

X

 Mineral  Melt

Y

3

Discontinuous Reaction

Melt

Mineral Mineral

2

Mineral Melt  Mineral

2

• The second reaction was seen before in the phase diagrams shown in mineralogy

• What was that type of reaction called?

4

Name of reaction?

Leucite Melt

• This was the reaction

5

Bowen’s Reaction Series

6

Gibbs Free Energy Definition

G

H

TS

• We can formulate a differential equation to represent changing geologic conditions: dG

VdP

SdT

• In igneous petrology, we are most often interested in the conditions involved at the liquid-solid phase boundary

7

Solid-Liquid Reaction

• Considering a reaction between a solid and a liquid (S ↔ L) we can rewrite the previous equation as d G

 

VdP

 

SdT

• Δ represents a change as the result of a reaction here, going from solid to liquid or vice versa

8

ΔV

V

V

L

V

S

• Since most solids are denser than their liquids at the melting point, ΔV is positive on going from solid to liquid

• Water is a notable exception

9

Melting Reaction

• Schematic P-T diagram of a melting reaction

• This figure shows the behavior of an arbitrary phase

• In the region labeled

“Solid” the solid phase is stable, because G

S

< G

L

• In the region labeled

“Liquid” the liquid phase is stable, because G

S

> G

L

10



Isobaric System

G

T



P

 

S

• Because S liquid

> S solid

, the slope of G vs. T is greater for the liquid than the solid

• At low temperatures the solid phase is more stable, but as temperature increases, the liquid phase becomes stable

11

Equilibrium Temperature

• Relationship between

Gibbs Free Energy and temperature for the solid and liquid forms of a substance at constant pressure.

• T eq is the equlibrium temperature

12

Isothermal System



 

G

P

 

T

V

• Because V liquid

> V solid

, the slope of G vs. P is greater for a liquid than a solid

• The liquid phase has lower G, and is thus more stable, at low pressure, but the solid phase is more stable at higher pressure

• This is why the inner core is solid

13

Equilibrium Presssure

• V is positive, and therefore the slope of

(δG/δP) is positive.

14

Equilibrium Curve

• Any two points on the equilibrium curve for a solid-liquid interface must have ΔG = 0, and therefore dΔG = 0

• Substituting gives

0

 

Vdp

 

Sdt

15

Clapeyron Equation

• Rearranging the previous equation gives: dP dT

S

V

16

Diopside – Anorthite System

Figure 6-11.Isobaric T-X phase diagram at atmospheric pressure. After Bowen (1915), American Journal of Science,

40, 161-185.

17

Fluid Saturation

• A fluid-saturated melt contains the maximum amount of dissolved volatile species possible at a given set of P-T-X conditions

• Any increase in volatile content will produce one or more additional phases

18

Fluid Pressure

• The fluid pressure (P f

) is used to define the state of volatiles in a melt

• If P f

= P volatiles total

, the melt is saturated with

• If P f

= 0, the system does not contain volatiles, and is often called “dry”

19

Le Châtlier’s Principle

• Any change imposed on a system at equilibrium will drive the system in the direction that reduces the imposed change

20

Melting of Hydrous Minerals

Solid

H O

Liq

( aq )

• Adding water to the system should cause melting, according to Le Châtlier’s Principle

• Adding water drives the reaction from left to right

• Removing water, such as by loss of volatiles near the surface, should cause crystallization

21

H

2

O Solubility

• Solubility of H

2

O at 1100°C in three natural rock samples and albite

• After Burnham

(1979)

22

Albite – H

2

O

• Effect of H

2

O saturation on the melting of albite

• After Burnham and Davis, 1974

• Dry melting curve from Boyd and England,

1963

23

Melting of Albite

H O

( vapor )

albite liquid

( aq )

• This reaction has a large negative ΔV on going from left to right, thus stabilizing the liquid phase and lowering the melting point

• At higher pressures, ΔV is less negative, and the slope of the line is less

24

Application of Clapeyron Equation dP

S dT 

V

• For the dry case, ΔV is positive, and the slope of the melting curve is positive

• For the wet case, ΔV is negative, and the slope of the melting curve is negative (melting point is depressed with increasing pressure)

25

Melting of

Gabbro

• Effect of H

2

O saturation on the melting of gabbro

(Burnham and

David, 1974)

• Dry melting curve from

Boyd and

England

(1963)

26

Melting Curves

• H

2

O saturated curves are solid

• H

2

O free curves are dashed

• Mafic rocks have higher melting points than felsic rocks

27

Albite –

H

2

O System

• Pressure-temperature projection of the melting relationships in the system albite –

H

2

O

• After Burnham and

Davis, 1974

Red curves = melting for a fixed mol % water in the melt (X w

Blue curves tell the water content of a water-saturated melt

)

28

Albite Melting

Percentage

• Percentage of melting for albite with 10 mol % H

2

O at

0.6 GPa as a function of temperature along traverse e-i

29

Albite – H

2

O

System

• Pressure-temperature projection of the melting relationships in the system albite –

H

2

O

• After Burnham and

Davis, 1974

30

Melting

Relationships

• Pressure-temperature projection of the melting relationships in the system albite –

H

2

O with curves representing constant activity of H

2

O

• After Burnham and

Davis, 1974

31

Diopside-Anorthite Liquidus

• The affect of H

2

O on the diopsideanorthite liquidus

32

Albite Melting with Fluids

• Experimentally determined melting of albite

 Dry

 H

2

O saturated

In presence of fluid containing 50% each of

H

2

O and CO

2

33

System

CO

2

Solubility

Pressure CO

2

Solubility

5-6% Albite-H

2

O-CO

2

2 GPa

Enstatite-H

2

O-CO

2

2 GPa

Diopside-H

2

O-CO

2

2 GPa

18%

35%

34

Ternary Eutectic

Fo

P = 2 GPa

CO

2 dry

Highly undesaturated

(nepheline-bearing) alkali olivine basalts

H

2

O

Ab

En

Ne

Oversaturated

(quartz-bearing) tholeiitic basalts

SiO

2

• Effect of volatiles on ternary eutectic in the system Forsterite –

Nepheline – Silica at 2

Gpa

• Water moves the (2

GPa) eutectic toward higher silica, while

CO

2 moves it to more alkaline types

35

Fo

Ternary Eutectic

Ne

Volatile-free

3GPa

Highly undesaturated

(nepheline-bearing) alkali olivine basalts

2GPa

1GPa

Ab

1atm

En

Oversaturated

(quartz-bearing) tholeiitic basalts

• Effect of Pressure on the position of the eutectic in the basalt system

SiO

2

• Increased pressure moves the ternary eutectic (first melt) from silica-saturated to highly undersat.alkaline basalts

36

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