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4.2: Magma Composition and Eruption Style

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    As noted in the previous section, the types of magma produced in the various volcanic settings can differ significantly. At divergent boundaries and oceanic mantle plumes, where there is little interaction with crustal materials the magma tends to be consistently mafic. At subduction zones, where the magma ascends through significant thicknesses of crust, interaction between the magma and the crustal rock—some of which is quite felsic—leads to increases in the felsic character of the magma.

    differentiation.png
    Figure \(\PageIndex{1}\) The important processes that lead to changes in the composition of magmas stored within magma chambers within relatively felsic rocks of the crust.

    As illustrated in Figure \(\PageIndex{1}\), several processes can make magma that is stored in a chamber within the crust more felsic than it was to begin with, and can also contribute to development of vertical zonation from more mafic at the bottom to more felsic at the top. Partial melting of country rock and country-rock xenoliths increases the overall felsic character of the magma; first, because the country rocks tends to be more felsic than the magma, and second, because the more felsic components of the country rock melt preferentially. Settling of ferromagnesian crystals from the upper part of the magma, and possible remelting of those crystals in the lower part can both contribute to the vertical zonation from relatively mafic at the bottom to more felsic at the top.

    From the perspective of volcanism there are some important differences between felsic and mafic magmas. First, as we’ve already discussed, felsic magmas tend to be more viscous because they have more silica, and hence more polymerization. Second, felsic magmas tend to have higher levels of volatiles; that is, components that behave as gases during volcanic eruptions. The most abundant volatile in magma is water (H2O), followed typically by carbon dioxide (CO2), and then by sulfur dioxide (SO2).

    volatile-compositions.png
    Figure \(\PageIndex{2}\) Variations in the volatile compositions of magmas as a function of silica content.

    The general relationship between the SiO2 content of magma and the amount of volatiles is shown in Figure \(\PageIndex{2}\). Although there are many exceptions to this trend, mafic magmas typically have 1% to 3% volatiles, intermediate magmas have 3% to 4% volatiles, and felsic magmas have 4% to 7% volatiles.

    Differences in viscosity and volatile levels have significant implications for the nature of volcanic eruptions. When magma is deep beneath the surface and under high pressure from the surrounding rocks, the gases remain dissolved. As magma approaches the surface, the pressure exerted on it decreases. Gas bubbles start to form, and the more gas there is in the magma, the more bubbles form. If the magma is runny enough for gases to rise up through it and escape to surface, the pressure will not become excessive. Assuming that it can break through to the surface, the magma will flow out relatively gently. An eruption that involves a steady non-violent flow of magma is called effusive.

    Exercise 4.2 Under pressure!
    A cork flying off the top of a champange bottle
    Figure \(\PageIndex{3}\)

    A good analogy for a magma chamber in the upper crust is a plastic bottle of pop on the supermarket shelf. Go to a supermarket and pick one up off the shelf (something not too dark). You’ll find that the bottle is hard because it was bottled under pressure, and you should be able to see that there are no gas bubbles inside.

    Buy a small bottle of pop (you don’t have to drink it!) and open it. The bottle will become soft because the pressure is released, and small bubbles will start forming. If you put the lid back on and shake the bottle (best to do this outside!), you’ll enhance the processes of bubble formation, and when you open the lid, the pop will come gushing out, just like an explosive volcanic eruption.

    A pop bottle is a better analogue for a volcano than the old baking soda and vinegar experiment that you did in elementary school, because pop bottles—like volcanoes—come pre-charged with gas pressure. All we need to do is release the confining pressure and the gases come bubbling out, forcing the pop with them.

    If the magma is felsic, and therefore too viscous for gases to escape easily, or if it has a particularly high gas content, it is likely to be under high pressure. Viscous magma doesn’t flow easily, so even if there is a conduit for it to move towards surface, it may not flow out. Under these circumstances pressure will continue to build as more magma moves up from beneath and gases continue to exsolve. Eventually some part of the volcano will break and then all of that pent-up pressure will lead to an explosive eruption.

    Mantle plume and spreading-ridge magmas tend to be consistently mafic, so effusive eruptions are the norm. At subduction zones, the average magma composition is likely to be close to intermediate, but as we’ve seen, magma chambers can become zoned and so compositions ranging from felsic to mafic are possible—even likely. Eruption styles can be correspondingly variable.

    Image Descriptions

    Figure \(\PageIndex{1}\) image description: Four processes that can affect the composition of magma stored in chambers.

    1. Loss of olivine or pyroxene (by crystal settling) makes the upper magma more felsic.
    2. Partial melting of country rock makes the magma more felsic.
    3. Partial or complete melting of xenoliths makes the magma more felsic.
    4. Possible re-melting of olivine or pyroxene can make the lower magma more mafic.

    [Return to Figure \(\PageIndex{1}\)]

    Figure \(\PageIndex{2}\) image description: The following table describes the range of data points adapted from the original scatter plot graph.
    Type of Magma Weight % of gasses (mostly H2O) Weight % of SiO2
    Mafic 1 to 3% 47 to 50%
    Intermediate 3 to 4% 57 to 64%
    Felsic 4 to 7% 69 to 72%

    [Return to Figure \(\PageIndex{2}\)]

    Media Attributions

    • Figure \(\PageIndex{1}\): © Steven Earle. CC BY.
    • Figure \(\PageIndex{2}\): Original image by Schminke, 2004. (Schminke, H-U., 2004, Volcanism, Springer-Verlag, Heidelberg). Modified by Steven Earle.
    • Figure \(\PageIndex{3}\): Champagne uncorking photographed with a high speed air-gap flash © Niels Noordhoek. CC BY-SA.

    This page titled 4.2: Magma Composition and Eruption Style is shared under a CC BY 4.0 license and was authored, remixed, and/or curated by Steven Earle (BCCampus) via source content that was edited to the style and standards of the LibreTexts platform.

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