Title: Petrology and Ore Deposits Course 10179
1Petrology and Ore DepositsCourse 10179
- Week 2
- Origin of Magmas by Melting of the Mantle and
Crust - Evolution of Magmas Fractional Crystallization
and Contamination - Reflected Light Microscopy
2Ch5 Origin of Magmas by Melting of the Mantle and
Crust
- Virtually all magmas have been generated within
the outermost 250 km of the Earth by melting of
solid mineral assemblages in the crust or mantle - Melting occurs when an assemblage of minerals
(/-fluid) reaches a temperature that produces a
silicate melt eg may be as low as 650?C for
crustal feldspathic sandstones water, or as
high as gt1200?C to melt dry mantle peridotite - Understanding the processes that generate magmas
first requires an analysis of the phase relations
involved in melting - P becomes an important variable when considering
melting, in contrast to crystallization, which
with volcanic rocks generally takes place at or
near the surface where P rarely exceeds 2kbar.
Plutonic generally crystallize within the
uppermost 15-20 km of the lithosphere 5-7kbar.
However, melting occurs over a much greater range
of depths 10- gt100km (3- gt20kbars) - The composition and T of the magmas derived from
melting of the same parental material can vary
significantly at different P
3Melting in Binary Systems
- Equilibrium melting
- Fractional melting
- Batch melting
4Binary Systems with Peritectites - Equilibrium
Melting
5Binary Systems with Peritectites Fractional
Melting
6Binary Systems with Complete Solid Solution
7Melting in Ternary Systems
Eutectic point
8Batch Melting
- We have been looking at two idealised concepts
1) Equilibrium melting, in which all of the
liquid remains in contact and equilibrium with
the solids, and 2) Fractional melting, in which
the liquid is constantly removed and therefore
cannot interact with the residuum - Do these processes actually occur?
- Experimental work has shown that melt cannot be
removed from a system until a critical minimum
volume of melt has been produced ie 30 for
basaltic liquids and much higher for granitic
melts. This indicates that a blend of equilibrium
and fractional melting may be typical in nature,
with equilibrium melting dominating in the early
stages and fractional melting in the latter. - This intermediate behaviour is referred to as
batch melting. Importantly, batch melting can
lead to the formation of a wide variety of melt
compositions as opposed to pure fractional
melting which only produces specific eutectic or
peritectic compositions.
9Ch6 - Evolution of Magmas Fractional
Crystallization and Contamination
- We have now covered the basics of how magmas are
formed by partial melting, we now need to explore
how the composition of magma can be modified
after it has left the place where it originated
and again it relies heavily on phase diagrams! - The processes that govern magma evolution are
fractional crystallization and assimilation-contam
ination.
10Fractional Crystallization
Rhythmic layering
Colloform growth structures
Cross-bedding
11Binary Eutectic and Peritectic Systems
12Layered Gabbroic Intrusions
- Typically olivine tholeiite composition
- Show prominent structural layering, which forms a
quasi-stratigraphy that subdivides layered
intrusives into various olivine- or
pyroxene-rich, ultramafic rocks at the base
plagioclase-rich, mafic, plutonic rocks such as
gabbros, norites anorthosites in the middle
levels and finally highly fractionated felsic
rocks, such as syenites and granophyres at the
top.
13Crystallization Sequence in Layered Intrusions
14Crystallization Sequence in Layered Intrusions
15Ore Microscopy (reflected light)
16Ch 5-6 Revision Questions
- Chapter 5 Review Questions
- 1. Using Figure 5-1, predict what the temperature
for beginning of melting would be for a rock
consisting of 40 anorthite and 60 diopside.
Predict the initial melting temperature for a
rock with 80 anorthite and 20 diopside. - 2. Construct a melting scenario in the system
forsteritesilica (Figure 5-2) for both
equilibrium and fractional melting for a rock
consisting of 75 enstatite and 25 forsterite.
Follow the melting process from inception of
melting to disappearance of the last few
crystals. - Optional
- 3. Construct a melting scenario in the ternary
system diopside-albite-anorthite (Figure 5-5) for
a rock composition between the diopside-plagioclas
e cotectic line and the diopside comer. - 4. In Figure 5-6B, trace the crystallization of a
variety of melts just on either side of the C-D
binary join to prove to yourself that C-D is in
fact a thermal divide that cannot be crossed by
evolving melts. - 5. Why is melting in the ternary system
diopside-forsterite-silica (Figure 5-7) a good
and relatively simple model for melting of the
upper mantle? - Chapter 6
- 1. In your own words, describe how fractional
crystallization differs from equilibrium
crystallization. - 2. How would you use patterns of igneous rock
compositions (specifically, clustering of
compositions for specific rock types such as
ocean floor basalt or intraplate alkali basalt)
to determine whether most magmas undergo
substantial fractionation during ascent? - 3. Using the ternary systems diopside-forsterites
ilica (Figure 6-8) and forsterite-anorthite-silica
(Figure 6-9), try to work out fractional
crystallization sequences that would give rise to
the layering found in layered intrusion (Figure
6-6). Experiment with each diagram to see what
compositions of mixed magmas would result from
the mixing of fractionated melts and batches of
new magma. (Hint You might find some interesting
"zigzag" liquid descent lines.) - Optional
- 4. Is there any sensible way to track the
continuous evolution in the bulk compositions of
fractionated magmas in a layered intrusion when a
"stratigraphic" layering develops as a result of
such physical processes as gravitational
settling? If not, how do we know that
fractionation actually occurred? - 5. Summarize the ways that trace elements and iso
topes can be used to track the processes of magma
contamination and magma mixing.