The primary cause of change in the composition of a magma is
cooling, which is an inevitable consequence of the magma being formed and migrating from the site of partial melting into an area of lower stress - generally a cooler volume of the crust. Cooling causes the magma to begin to crystallize minerals from the melt or liquid portion of the magma. Most magmas are a mixture of liquid rock (melt) and crystalline minerals (phenocrysts). Contamination is another cause of magma differentiation. Contamination can be caused by
assimilation of wall rocks, mixing of two or more magmas or even by replenishment of the magma chamber with fresh, hot magma. The whole gamut of mechanisms for differentiation has been referred to as the FARM process, which stands for fractional crystallization, assimilation, replenishment and magma mixing.
Fractional crystallization of igneous rocks Fractional crystallization is the removal and segregation from a melt of mineral precipitates, which changes the composition of the melt. This is one of the most important geochemical and physical processes operating within the Earth's
crust and
mantle. Fractional crystallization in silicate melts (magmas) is a very complex process compared to chemical systems in the laboratory because it is affected by a wide variety of phenomena. Prime amongst these are the composition, temperature, and pressure of a magma during its cooling. The composition of a magma is the primary control on which mineral is crystallized as the melt cools down past the
liquidus. For instance in
mafic and
ultramafic melts, the
MgO and
SiO2 contents determine whether
forsterite olivine is precipitated or whether
enstatite pyroxene is precipitated. Two magmas of similar composition and temperature at different pressure may crystallize different minerals. An example is high-pressure and high-temperature fractional crystallization of granites to produce single-
feldspar granite, and low-pressure low-temperature conditions which produce two-feldspar granites. The
partial pressure of volatile phases in silicate melts is also of prime importance, especially in near-
solidus crystallization of granites.
Assimilation Assimilation can be broadly defined as a process where a mass of magma wholly or partially homogenizes with materials derived from the wall rock of the magma body. Assimilation is a popular mechanism to partly explain the felsification of ultramafic and mafic magmas as they rise through the crust: a hot primitive melt intruding into a cooler,
felsic crust will melt the
crust and mix with the resulting melt. This then alters the composition of the primitive magma. Also, pre-existing mafic host rocks can be assimilated by very hot primitive magmas. Effects of assimilation on the chemistry and evolution of magma bodies are to be expected, and have been clearly proven in many places. In the early 20th century there was a lively discussion on the relative importance of the process in igneous differentiation. More recent research has shown, however, that assimilation has a fundamental role in altering the trace element and isotopic composition of magmas, in formation of some economically important ore deposits, and in causing volcanic eruptions.
Replenishment When a melt undergoes cooling along the liquid line of descent, the results are limited to the production of a homogeneous solid body of intrusive rock, with uniform mineralogy and composition, or a partially differentiated
cumulate mass with layers, compositional zones and so on. This behaviour is fairly predictable and easy enough to prove with geochemical investigations. In such cases, a magma chamber will form a close approximation of the ideal
Bowen's reaction series. However, most magmatic systems are polyphase events, with several pulses of magmatism. In such a case, the liquid line of descent is interrupted by the injection of a fresh batch of hot, undifferentiated magma. This can cause extreme fractional crystallisation because of three main effects: • Additional heat provides additional energy to allow more vigorous convection, allows
resorption of existing mineral phases back into the melt, and can cause a higher-temperature form of a mineral or other higher-temperature minerals to begin precipitating • Fresh magma changes the composition of the melt, changing the chemistry of the phases which are being precipitated. For instance,
plagioclase conforms to the liquid line of descent by forming initial
anorthite which, if removed, changes the equilibrium mineral composition to
oligoclase or
albite. Replenishment of the magma can see this trend reversed, so that more anorthite is precipitated atop cumulate layers of albite. • Fresh magma destabilises minerals which are precipitating as
solid solution series or on a
eutectic; a change in composition and temperature can cause extremely rapid crystallisation of certain mineral phases which are undergoing a eutectic crystallisation phase.
Magma mixing Magma mixing is the process by which two magmas meet, comingle, and form a magma of a composition somewhere between the two end-member magmas. Magma mixing is a common process in volcanic magma chambers, which are open-system chambers where magmas enter the chamber, undergo some form of assimilation, fractional crystallisation and partial melt extraction (via eruption of lava), and are replenished. Magma mixing also tends to occur at deeper levels in the crust and is considered one of the primary mechanisms for forming intermediate rocks such as
monzonite and
andesite. Here, due to heat transfer and increased volatile flux from
subduction, the silicic crust melts to form a felsic magma (essentially granitic in composition). These
granitic melts are known as an
underplate.
Basaltic primary melts formed in the mantle beneath the crust rise and mingle with the underplate magmas, the result being part-way between basalt and
rhyolite; literally an 'intermediate' composition.
Other mechanisms of differentiation Interface entrapment Convection in a large magma chamber is subject to the interplay of forces generated by thermal convection and the resistance offered by friction, viscosity and drag on the magma offered by the walls of the magma chamber. Often near the margins of a magma chamber which is convecting, cooler and more viscous layers form concentrically from the outside in, defined by breaks in viscosity and temperature. This forms
laminar flow, which separates several domains of the magma chamber which can begin to differentiate separately.
Flow banding is the result of a process of fractional crystallization which occurs by convection, if the crystals which are caught in the flow-banded margins are removed from the melt. The friction and
viscosity of the magma causes
phenocrysts and
xenoliths within the magma or lava to slow down near the interface and become trapped in a viscous layer. This can change the composition of the melt in large
intrusions, leading to differentiation.
Partial melt extraction With reference to the definitions, above, a magma chamber will tend to cool down and crystallize minerals according to the liquid line of descent. When this occurs, especially in conjunction with zonation and crystal accumulation, and the melt portion is removed, this can change the composition of a magma chamber. In fact, this is basically fractional crystallization, except in this case we are observing a magma chamber which is the remnant left behind from which a daughter melt has been extracted. If such a magma chamber continues to cool, the minerals it forms and its overall composition will not match a sample liquid line of descent or a parental magma composition. ==Typical behaviours of magma chambers==