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Chapter 11 - Diversification of Magmas - Faculty web pages

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<strong>Chapter</strong> <strong>11</strong>: <strong>Diversification</strong> <strong>of</strong><br />

<strong>Magmas</strong>


Magmatic Differentiation<br />

<br />

Any process by which a magma is able to<br />

diversify and produce a magma or rock <strong>of</strong><br />

different composition


Magmatic Differentiation<br />

<br />

Two essential processes affect magmatic<br />

differentiation:<br />

1. Creates a compositional difference in one or<br />

more phases (minerals)<br />

2. Segregation or fractionation <strong>of</strong> the chemically<br />

distinct portions


Partial Melting<br />

Separation <strong>of</strong> a partially melted liquid (the melt)<br />

from the solid residue (the residuum)


Eutectic Melting<br />

Eutectic point = the single point where two liquidus<br />

lines meet the solidus line<br />

Represents both T and composition <strong>of</strong> the lowest T melt<br />

M = eutectic point


Eutectic Melting<br />

First melt always = eutectic composition<br />

Major element composition <strong>of</strong> eutectic melt is<br />

constant until one <strong>of</strong> the source mineral phases is<br />

consumed<br />

Once a phase is consumed, the next increment <strong>of</strong> melt<br />

will be different composition (X) and T


Critical Melt Fraction<br />

<br />

Separation <strong>of</strong> a partially melted liquid from the<br />

solid residue requires a critical melt %<br />

<br />

Sufficient melt must be produced to<br />

1. Form a continuous, interconnected film<br />

2. Have enough volume so not all <strong>of</strong> it is<br />

adsorbed to the crystal surfaces


The ability to form an interconnected film is<br />

dependent upon the dihedral angle (θ)(<br />

- a property<br />

<strong>of</strong> the melt<br />

a. θ = dihedral angle <strong>of</strong><br />

melt droplets at<br />

multiple grain<br />

boundaries<br />

b. Low θ = continuous<br />

interconnected<br />

network<br />

c. Higher θ = isolated<br />

melt droplets<br />

Figure <strong>11</strong>-1 Illustration <strong>of</strong> the dihedral angle (θ)(<br />

) <strong>of</strong><br />

melt droplets that typically form at multiple grain<br />

junctions. After Hunter (1987) In I. Parsons (ed.),<br />

Origins <strong>of</strong> Igneous Layering. Reidel, , Dordrecht,<br />

pp. 473-504.


Factors affecting separation <strong>of</strong> melt<br />

Viscosity – high viscosity silicic melts, e.g., rhyolite,<br />

difficult to extract<br />

Critical melt fraction<br />

% <strong>of</strong> melt at which crystal mush (melt-dominated,<br />

fluid suspension) forms<br />

Theoretical calculations with spheres = 26% melt<br />

Irregular shapes and sizes = 30-50% for granitic<br />

compositions


Liquid separation by gravitational effects<br />

Buoyant liquid seeks to rise and escape xstal<br />

residue<br />

1) Filter pressing (compaction) crystal mush<br />

Xstal-liquid liquid system squeezed like a sponge<br />

Liquid migrates from compacted solids


Fractional Crystallization<br />

<br />

<br />

Process by which all xstals formed are removed<br />

from melt<br />

Causes continuously changing magma composition<br />

Dominant mechanism by which most magmas<br />

differentiate


Gravity settling<br />

Differential motion <strong>of</strong> crystals and liquid under<br />

the influence <strong>of</strong> gravity due to their differences in<br />

density<br />

Cumulate texture: mutually touching phenocrysts<br />

embedded in an interstitial matrix which is the<br />

crystallized residual melt


Gravity settling – Ternary Phase Diagram<br />

3 Phases = An (anorthite(<br />

anorthite), Di (diopside(<br />

diopside), and Fo<br />

(forsterite<br />

olivine)<br />

Point a → olivine layer<br />

at base <strong>of</strong> pluton<br />

if olivine sinks first<br />

Next get ol + cpx layer<br />

Last get ol + cpx + plag<br />

layer<br />

Figure 7-2. After Bowen (1915), A. J. Sci., and Morse (1994), Basalts and Phase<br />

Diagrams. Krieger Publishers.


Stoke’s Law – used to quantify crystal settling<br />

velocities<br />

V 2gr 2<br />

( ρ − ρ<br />

s l<br />

=<br />

)<br />

9η<br />

V = the settling velocity (cm/sec)<br />

g = the acceleration due to gravity (980 cm/sec 2 )<br />

r = the radius <strong>of</strong> a spherical particle (cm)<br />

ρ s = the density <strong>of</strong> the solid spherical particle (g/cm 3 )<br />

ρ l = the density <strong>of</strong> the liquid (g/cm 3 )<br />

η = the viscosity <strong>of</strong> the liquid (1 c/cm sec = 1 poise)


Olivine in basalt<br />

Olivine (ρ(<br />

s = 3.3 g/cm 3 , r = 0.1 cm)<br />

Basaltic liquid (ρ(<br />

l = 2.65 g/cm 3 , η = 1000 poise)<br />

V = 2·9802<br />

980·0.10.1 2 (3.3-2.65)/9<br />

2.65)/9·1000 = 0.0013 cm/sec


Rhyolitic melt<br />

η = 10 7 poise and ρ l = 2.3 g/cm 3<br />

<br />

hornblende crystal (ρ(<br />

s = 3.2 g/cm 3 , r = 0.1 cm)<br />

V = 2 x 10 -7 cm/sec, or 6 cm/year<br />

<br />

feldspars (ρ l = 2.7 g/cm 3 )<br />

V = 2 cm/year<br />

= 200 m in the 10 4 years that a stock might take to<br />

cool<br />

If 0.5 cm in radius (1 cm diameter), settle at 0.65<br />

meters/year, or 6.5 km in 10 4 years cooling <strong>of</strong><br />

stock


Stokes’ Law is overly simplified<br />

1. Crystals are not spherical<br />

2. Only basaltic magmas very near their<br />

liquidus temperatures behave as<br />

Newtonian fluids


Mechanisms that facilitate the separation <strong>of</strong> crystals<br />

and liquid<br />

1. Filter Pressing (compaction)– in xstal mushes<br />

that form as cumulates or xstal suspensions


Mechanisms that facilitate the separation <strong>of</strong> crystals<br />

and liquid<br />

2. Flow segregation – motion <strong>of</strong> magma past country rock<br />

walls results in velocity gradient near walls and creates<br />

shear in viscous magma<br />

Shear constricted between<br />

phenocrysts or in contact with<br />

country rock<br />

Force called grain-dispersive<br />

pressure pushes phenocrysts apart<br />

and away from contact<br />

Figures <strong>11</strong>-4 4 and <strong>11</strong>-5 Drever and Johnston (1958). Royal Soc. Edinburgh<br />

Trans., 63, 459-499.<br />

499.


Flow differentiation -<br />

Concentration <strong>of</strong> coarse<br />

phenocrysts toward center <strong>of</strong><br />

dikes and sills


Volatile Transport<br />

- separate vapor phase coexists with magma<br />

1. Vapor released by heating <strong>of</strong> hydrated or carbonated<br />

wall rocks<br />

2. As a volatile-bearing magma rises and pressure is<br />

reduced, magma becomes saturated in the vapor, and a<br />

free vapor phase will be released<br />

Produces hydrothermal effects such as alkali<br />

metasomatism called fenitization


3. . Late-stage fractional crystallization – forms separate<br />

fluid phase<br />

<br />

<br />

<br />

<br />

<br />

Fractional crystallization enriches late melt in<br />

H 2 O, other volatiles, incompatible elements<br />

Saturation point reached<br />

Hydrous vapor phase formed<br />

Produces boiling <strong>of</strong>f <strong>of</strong> H 2 O as magma cools (retrograde<br />

boiling)<br />

Results in<br />

silicate-saturated saturated vapor<br />

vapor-saturated late silicate liquid enriched in volatiles<br />

and incompatible elements


Volatile release increases P - fractures ro<strong>of</strong> rocks <strong>of</strong><br />

magma chamber<br />

<br />

Vapor and melt escape along fractures as dikes<br />

Silicate melt composed <strong>of</strong> quartz and feldspar<br />

forms small dikes <strong>of</strong> aplite<br />

Vapor phase forms pegmatites (coarser-<br />

grained dikes)


Pegmatites: : Concentrate incompatible elements<br />

Complex varied mineralogy with very large unusual<br />

minerals<br />

MacDonald<br />

Pegmatite<br />

Bancr<strong>of</strong>t, Ont.


Hornblende<br />

retrograde boiling<br />

Silver Crater Pegmatite<br />

Bancr<strong>of</strong>t, Ont.<br />

Apatite


8 cm tourmaline crystals<br />

from pegmatite<br />

5 mm gold from a<br />

hydrothermal deposit


Liquid Immiscibility – Italian Salad Dressing<br />

<br />

<br />

<br />

Analogy<br />

Widely accepted as phenomenon in natural<br />

magmas<br />

Extent <strong>of</strong> process in question<br />

Importance in generating large intrusive bodies<br />

questionable


Liquid Immiscibility – Some examples<br />

Late silica-rich immiscible droplets in Fe-rich<br />

tholeiitic basalts<br />

Sulfide-silicate immiscibility in massive sulfide<br />

deposits<br />

Carbonatite-nephelinite<br />

nephelinite systems


Magma Mixing<br />

<br />

End member mixing in a suite <strong>of</strong> rocks,<br />

e.g., basalt and rhyolite magmas<br />

<br />

Variation on composition diagrams<br />

should lie on a straight line between the<br />

two most extreme parental compositions


Comingled Basalt-Rhyolite<br />

Mt. McLoughlin, , Oregon<br />

Figure <strong>11</strong>-8 From Winter (2001) An Introduction to<br />

Igneous and Metamorphic Petrology. Prentice Hall<br />

Basalt pillows accumulating at<br />

the bottom <strong>of</strong> granitic magma<br />

chamber<br />

Vinalhaven Island, Maine


Assimilation<br />

<br />

<br />

Incorporation <strong>of</strong> wall rocks, xenoliths<br />

Assimilation by melting is limited by<br />

the heat available in the magma


Zone melting<br />

<br />

Crystallizing igneous material at the<br />

base equivalent to the amount melted<br />

at the top<br />

Transfer heat by convection<br />

Most likely to occur in large mafic<br />

magmas deep in the crust where<br />

country rocks close to liquidus T


In Situ Differentiation Processes<br />

<br />

<br />

In-situ: crystals don’t sink/move<br />

Typically involves<br />

Diffusion<br />

Convective separation <strong>of</strong> liquid and crystals


The Soret Effect<br />

<br />

<br />

Thermal diffusion = Soret effect<br />

Heavy elements/molecules migrate toward the colder end<br />

and lighter ones to the hotter end <strong>of</strong> the gradient


Thermogravitational diffusion<br />

Stable and persistent stagnant boundary layers occur near the<br />

top and sides <strong>of</strong> magma chambers<br />

Figure <strong>11</strong>-<strong>11</strong>. Schematic section through a rhyolitic magma chamber undergoing convection-aided in-situ differentiation.<br />

After Hildreth (1979). Geol. Soc. Amer. Special Paper, 180, 43-75.


Langmuir Model<br />

<br />

<br />

Thermal gradient at wall and cap produces variation in %<br />

crystallization<br />

Compositional convection produces evolved magmas from<br />

boundary layer to cap<br />

Figure <strong>11</strong>-12<br />

12 Formation <strong>of</strong> boundary layers along<br />

the walls and top <strong>of</strong> a magma chamber. From<br />

Winter (2001) An Introduction to Igneous and<br />

Metamorphic Petrology. Prentice Hall


Detecting and assessing assimilation<br />

Isotopes are generally the best<br />

Continental crust becomes progressively enriched in<br />

87 Sr/ 86 Sr and depleted in 143 Nd/ 144 Nd<br />

Figure 9-13. 9<br />

Estimated<br />

Rb and Sr isotopic<br />

evolution <strong>of</strong> the Earth’s<br />

upper mantle, assuming<br />

a large-scale melting<br />

event producing<br />

granitic-type type continental<br />

rocks at 3.0 Ga b.p After<br />

Wilson (1989). Igneous<br />

Petrogenesis. Unwin<br />

Hyman/Kluwer<br />

Kluwer.


Tectonic-Igneous Associations<br />

<br />

<br />

Associations on a larger scale than the<br />

petrogenetic provinces<br />

Attempt to address global patterns <strong>of</strong> igneous<br />

activity by grouping provinces based upon<br />

similarities in occurrence and genesis


Tectonic-Igneous Associations<br />

Mid-Ocean Ridge Volcanism<br />

Ocean Intra-plate (Island) volcanism<br />

Continental Plateau Basalts<br />

Subduction-related volcanism and plutonism<br />

Island Arcs<br />

Continental Arcs<br />

Granites<br />

Mostly alkaline igneous processes <strong>of</strong> stable<br />

craton interiors<br />

Anorthosite Massifs

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