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Lecture 12: Crystallization & Mineral Reactions Read Chpt 2

Lecture 12: Crystallization & Mineral Reactions Read Chpt 2

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<strong>Lecture</strong> <strong>12</strong>:<br />

<strong>Crystallization</strong> & <strong>Mineral</strong> <strong>Reactions</strong><br />

<strong>Crystallization</strong>: formation of minerals from solutions, melts or vapors;<br />

go from random to more ordered (crystalline state)<br />

What causes crystallization from a solution?<br />

• Change in composition<br />

• Change in temperature<br />

• Change in pressure<br />

<strong>Crystallization</strong> from a melt occurs with two competing tendencies:<br />

1. Thermal vibrations that tend to destroy the nuclei of potential minerals<br />

2. Attractive forces that tend to aggregate atoms into crystal structures<br />

<strong>Read</strong> <strong>Chpt</strong> 2


Crystal Growth: : How do they form??<br />

Nucleation: a “seed” crystal forms (aka(<br />

“nucleus”); ions constantly come<br />

together, but most redissolve. . Why? Atoms at the surface have<br />

unsatistified bonds (incomplete polyhedra). More surface atoms per unit<br />

solid = less stability (high surface energy)<br />

Critical Size: : must be reached to grow a crystal; if seed grows rapidly, it<br />

will reach a point where the surface energy is lowered enough that<br />

crystallite can keep growing and not be redissolved; ; ions stick best at<br />

steps and kinks, where they can satisfy more unsatisfied bonds at once


MINERAL REACTIONS<br />

Igneous <strong>Reactions</strong>:<br />

95% of the earth’s s crust is composed of igneous rocks that form from<br />

magmas<br />

Magmas are principally composed of O, Si, , Al, Fe, Ca, Mg, Na and K<br />

(with accessory H 2 O, CO 2 and volatiles like H 2 S, HCl, , CH 4 , CO)<br />

As magmas cool, minerals begin to precipitate in a distinct order:<br />

‘Bowen’s s Reaction Series’


Bowen wanted to answer the question:<br />

How do different types of igneous rocks form? Can you get basalts and<br />

granites from the same “parent” magma?<br />

So, he did a series of lab experiments:<br />

1. Make artificial magma of ‘basaltic’ composition<br />

2. Cool very slowly to a particular temperature<br />

3. Quickly quench<br />

Results? Two different types of “reaction series”<br />

Continuous Reaction Series: : a solid solution of continuously changing<br />

composition forms<br />

Ex. Plagioclase feldspars (Ca rich => Na rich at lower T)<br />

Discontinuous Reaction Series: reactions occur between melt and<br />

previously precipitated crystals; the old crystals dissolve and new<br />

minerals of different composition and structure form<br />

Ex. Olivine => Pyroxene => Amphibole => Biotite


Bowen’s s idea:<br />

Magmatic Differentiation: a single<br />

single homogeneous magma<br />

produces a variety of chemically distinct igneous rocks because of…<br />

Frractional <strong>Crystallization</strong>: crystals are<br />

crystals are physically separated from<br />

the cooling magma (e.g., by gravity settling or rimming) so that liquid and<br />

crystal cannot react further; ; changes the bulk composition of the magma<br />

(in fact, makes it more SiO 2 -rich, because mafic minerals form first and<br />

settle out)<br />

We will discuss this more in the context of phase diagrams…Bowen was<br />

partially correct, but there are other processes at work as well…


MINERAL REACTIONS<br />

Metamorphic <strong>Reactions</strong>:<br />

Reaction that occur in the solid state<br />

-typically isochemical, , that is, the bulk chemistry is unchanged (except often<br />

a change in H 2 O)<br />

Examples:<br />

Dehydration reactions: higher T, volatile H 2 O is formed and lost<br />

Decarbonation reactions: : carbonate-rich sedimentary rocks lose<br />

CO 2 with increasing T<br />

CaCO 3 (calcite) + SiO 2 (silica) = CaSiO 3 (wollastonite)) + CO 2 (gas)<br />

Metasomatic: : additional elements are gained or lost by circulating fluids


MINERAL REACTIONS<br />

Weathering <strong>Reactions</strong> (Physical vs. . Chemical):<br />

Chemical Weathering: thermodynamically driven alteration of minerals to<br />

form new minerals; changes composition and structure; occurs because of<br />

changes in T, P, composition<br />

Primary <strong>Mineral</strong>s: : Quartz, Olivine, Albite, Enstatite, , Muscovite<br />

tend to weather and form<br />

Secondary <strong>Mineral</strong>s: Kaolinite, , Goethite, Gibbsite, Hematite<br />

“Goldich” Weathering Series: : susceptibility to chemical weathering<br />

Quartz


MINERAL REACTIONS<br />

“Goldich” Weathering Series:<br />

Quartz


So what is the answer?<br />

Differences in structure, bonding determine weathering kinetics<br />

More polymerized structures break apart more slowly (more strong bonds<br />

to break!)<br />

Sometimes the reaction product is not solid phase, e.g. secondary layer<br />

silicates, but rather dissolved SiO 2 , Na + , K + , Ca +2 , Mg +2<br />

Examples:<br />

Al 2 SiO 5 (sillimanite)) + SiO 2 (quartz) + H 2 O => Al 2 Si 2 O 5 (OH) 4 (kaolinite)<br />

3KAlSi 3 O 8 (orthoclase) + 2H + => KAl 3 Si 3 O 10 (OH) 2 (muscovite) + 2K + + 6SiO 2


MINERAL REACTIONS<br />

Ultra High Pressure <strong>Reactions</strong>:<br />

Below the crust at high temperatures and pressures, minerals undergo<br />

transformation reactions into structures more suited to those P,T<br />

conditions<br />

How do we know?<br />

Specimens at the surface, e.g., from kimberlite pipes<br />

Laboratory experiments with diamond anvil cells<br />

* Below 6km, Si probably exists in 6-fold coordination with O, rather than<br />

4-fold<br />

* Increased densities of materials, denser packing of elements<br />

* Perovskite and rutile type structures become important*


Rutile Structure (TiO 2 )<br />

Based on hexagonal closest packing (HCP): ABABABAB layers of HP<br />

Ti atoms fill half of the possible octahedral positions<br />

The cations are always in 6-fold (octahedral) coordination.<br />

The anions are coordinated by 3 cations (trigonal<br />

coordination)<br />

Octahedra link along edges


Perovskite Structure (ABO 3 )<br />

Cubic closest packing (CCP) of oxygen, e.g., ABCABC layers of HP<br />

1/4 of oxygens are replaced by a large A cation<br />

A cation is in <strong>12</strong>-fold coordination with surrounding O<br />

B cation is in 6-fold (octahedral) coordination with O<br />

Octahedra share apices only<br />

Very dense structure

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