IGNEOUS ROCKS READING, A SUPPLEMENT TO THE LAB MANUAL

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IGNEOUS ROCKS READING, A SUPPLEMENT TO THE LAB MANUAL I Introduction: Igneous rocks are rocks that solidify from molten rock. When molten rock is underground we call it magma whereas when it is above ground we call it lava, even though it is the same stuff. Geologists classify igneous rocks because the different types indicate different tectonic settings, different volcanic plumbing systems, different sources for magma, and many other things. Two main characteristics are used to classify igneous rocks: 1) texture (the size of the mineral grains in the rock; and 2) composition (often determined by what the actual minerals are). Most geologists first determine the texture and then the composition, and with these two bits of information fit the rock into an established igneous-rock classification scheme (of which there are many). There are hundreds of different igneous rock names. Fortunately, many of these are quite rare and often restricted to only a few places on Earth, so most geologists ignore worrying about identifying them. Identifying common igneous rocks therefore becomes much more of a tractable problem, especially because you can do it using only 7 of the 8 most common minerals (that you learned to identify last week, right?). Identifying these minerals in a rock, combined with assessing the rock s texture, makes it possible to do a very decent job of classifying probably 90% of all igneous rocks. The 7 minerals that you need to be able to identify in order to classify igneous rocks are quartz, potassium feldspar (sometimes called alkali feldspar), plagioclase feldspar, mica, amphibole, pyroxene, and olivine. The hints from last week for identifying these minerals is attached to the end of this lab handout. The two textures that are used for classification are called phaneritic and aphanitic. A third texture, porphyritic, is kind of a hybrid between aphanitic and phaneritic. Porphyritic texture isn t used in most rock-name classification schemes, but it is important to identify because if present, it tells you something about the history of the igneous rock. II Texture: Texture is basically a measure of how big the crystals in an igneous rock are, and is important because it gives an indication of how quickly or slowly the rock solidified. This in turn, tells you whether or not it solidified partially or wholly below the surface or whether it solidified on the surface. The basic rule is that the slower the magma or lava solidifies, the larger and more interlocked the mineral grains will be. We call rocks that solidified underground plutonic or intrusive and those that solidified above ground volcanic or extrusive. Note that there are a few exceptions to the fine-grained = extrusive and coarse-grained = intrusive rules, so it is important to not automatically equate texture with solidification location. Rocks are good insulators so if a magma solidifies underground, it will cool very slowly. This slow cooling allows individual mineral grains go grow to large sizes. The texture that results is called phaneritic texture, and is defined as a rock where all the grains are large enough for you to see with your naked eyes. This is why rocks that solidify underground and thus exhibit phaneritic texture are called plutonic rocks or intrusive rocks. Typically, the mineral grains in plutonic rocks have irregular shapes because as they grow, they eventually start to bump into their neighbors and therefore can t assume their ideal shapes. Instead, they form irregular, interlocking shapes. The interlocking of all these individual minerals is what gives many plutonic rocks (such as granite)

2 their strength. Remember, plutonic (or intrusive) is the rock type, phaneritic is the texture that plutonic (or intrusive) rocks exhibit. The exception to this situation (which is common in Hawai i, actually) is thin dikes, which cool very rapidly. They are intrusive (because dikes intrude pre-existing rock), but because they are so thin, they cool quickly, and are extremely fine-grained. If a rock cools above ground without the benefit of insulating surrounding rocks, it will solidify rapidly, meaning that there is little time for crystals to grow. Instead of a few large crystals there will be many more, small crystals. This is aphanitic texture, and is defined as a rock where any or all of the mineral grains are too small to be seen with the naked eye. Rocks that solidify on the surface and thus exhibit aphanitic texture are called volcanic rocks or extrusive rocks. Volcanic (or extrusive) is the rock type, aphanitic is the texture that volcanic (or extrusive) rocks exhibit. A special class of aphanitic rocks cools so fast that there isn t enough time for any crystals to grow. Instead, what is formed is natural glass, such as obsidian. We will talk about obsidian later. The exception to this situation is very thick lava flows that may take weeks to months to solidify. They are extrusive (because they erupted on the surface), but because they are thick, the central parts cool slowly, and they can be reasonably coarse-grained, although never as coarse grained as a typical granite. The third texture, porphyritic, is kind of a hybrid between phaneritic and aphanitic. A porphyritic volcanic rock is one where one set of mineral grains is much larger than all the others. These larger grains are called phenocrysts. In the case of a porphyritic intrusive rock, there will be large, well-formed phenocrysts in a matrix of smaller (but still visible), interlocking grains. In the case of a porphyritic volcanic rock, there will be large, well-formed phenocrysts in a finegrained matrix in which the individual crystals are too small to see. Porphyritic texture tells you that the igneous rock underwent two stages of cooling, first slow, then fast. The larger grains formed and grew during the early, slow cooling, for example while magma sits in a volcanic magma chamber. The finer-grained matrix formed during later, but more rapid cooling, for example after the magma erupted onto the surface. From these brief descriptions you can see that much of an igneous rock s history can be determined merely from an assessment of its texture. Of course in nature there is infinite variability, so there are always going to be rocks that fall on the boundary between the textures defined here. A rock with grains that you can barely see might be a fine-grained plutonic (intrusive) rock or a coarse-grained volcanic (extrusive) rock. In those cases a geologist needs to look for other evidence to determine whether the rock is plutonic or volcanic. III Chemical Composition: Chemical composition is the other major criterion that geologists use to classify igneous rocks. There are numerous schemes that have been devised to do this classification, some of which are simple and others of which are exceedingly complex. Here, we ll deal with two of the simple classifications. The simplest classification divides igneous rocks into three groups, felsic (also called silicic), intermediate, and mafic (also called basic). The word felsic comes from feldspar and silica in combination, and refers to rocks that consist mainly of potassium feldspar and quartz. Potassium feldspar and quartz are light-colored (usually), so felsic rocks tend to be light-colored. Common examples include rocks such as granite (plutonic) and rhyolite (volcanic).

3 The word mafic comes from magnesium and iron in combination. Most magnesium- and iron-bearing minerals (olivines, pyroxenes, amphiboles) tend to be dark, so mafic rocks are usually quite dark as well. The most common plutonic example is gabbro, and the most common volcanic example is basalt. Intermediate rocks, as you might guess, are rocks that fall somewhere between felsic and mafic. Table 3.2 of your lab book lists only one set of intermediate rocks (andesite and diorite), but they deserve better because they are quite common. Most of the Andean volcanoes erupt andesite, and in fact that s where the name andesite comes from in the first place! Table 3.2 includes andesite but doesn t include some equally common and important rock types. For example, Pinatubo and Mt. St. Helens erupt dacite most of the time. Dacite is a volcanic composition that lies between rhyolite and andesite. Additionally, much of the so-called granite that makes up the Sierra Nevada mountains in the Western USA (including Half Dome and El Capitan in Yosemite) aren t actually granite. Instead, these mountains are granodiorite, a plutonic composition that, as its name implies, lies between granite and diorite. The table below shows a more complete scheme for igneous rock classification. Notice that for each composition there is a volcanic and an intrusive rock. Cooling History Felsic Intermediate Mafic Volcanic Rhyolite Dacite Andesite Basalt Plutonic Granite Granodiorite Diorite Gabbro The only way to really place a particular igneous rock into it s correct classification is to run chemical analyses on it. This involves grinding the rock into powder and subjecting it to a battery of chemical tests. This is not what most geologists do in the field, obviously, and not what we will do in this lab. Classification by Mineralogy: Instead, we will classify the igneous rocks based on what minerals are present. Although not as definitive as using chemical analyses, using mineralogy works most of the time because the specific minerals that form are a direct reflection of the chemical composition of the magma. The top row of Table 3.2 in your lab book lists minerals and their percentages in different igneous rocks. Unfortunately, as noted above, it ignores some important intermediate rock types. Figure 1 shows the full complement of rock types (below) and the typical minerals found in each (above). So, for example, if you find an extrusive rock with lots of K-spar, some quartz, some plagioclase feldspar, some muscovite, and some biotite, you can be pretty sure that it s a rhyolite. Likewise, if you find an intrusive rock with lots of plagioclase feldspar, some amphibole, and some pyroxene, it is probably a diorite.

4 Figure 1. Good rock-classification scheme (from Exploring Earth by Davidson, Reed, and Davis). So, in order to classify an igneous rock, you first decide whether it has a phaneritic or aphanitic texture. Next, you look at the minerals that are in the rock and their abundance. Then, using Figure 1, you give the rock a name. This is not super-easy, and many geologists have trouble getting rocks right all the time. One of the most difficult parts is estimating the percentages of different minerals (assuming you have identified them correctly). Most people tend to over-estimate abundances. Figures 2 and 3 are diagrams that show what actual abundances look like.

5 Figure 2. Diagrams for estimating mineral abundances: mafic minerals Figure 3. Diagrams for estimating mineral abundances: felsic minerals

If you want to see a really comprehensive rock-id scheme, check out Figure 4 (don t worry, you won t have to use it). 6 Figure 4. Rock classification scheme based on the abundances of quartz, K-spar, plagioclase feldspar, and a family of minerals called feldspathoids (from Rocks and Minerals by Detrich and Skinner). Note that the shading shows the relative abundances of each type. IV Glassy Rocks: Obsidian Obsidian is a type of natural glass. Some geologists consider glass to technically be a liquid because its molecular structure is completely random. Thus, instead of a regular, repeating structure, as you expect for a true mineral, there is no pattern at all. Natural glass forms when lava or magma cools so quickly that the atoms and molecules don t have enough time to organize themselves into the right locations to form minerals. Instead, they are quenched in their random, liquid positions. Natural glass is closest in texture to aphanitic rocks, and can be porphyritic if there are phenocrysts in a matrix of glass. Natural glass can be any composition (see below), but the term obsidian is reserved for high-silica compositions. Obsidian is typically very dark in color. Pumice Pumice is also natural glass, but it is full of bubbles. These bubbles form in the magma as it rises and the pressure confining it decreases. The bubbles form in the same way that bubbles form in a bottle of beer (or soda if you re under 21) when you take off the cap. There are molecules of

7 gas floating around in the magma. In most magmas they are molecules of CO 2, SO 2, and H 2 O. When the magma is under high pressure, these molecules don t attach to each other, and instead they are just floating around. They are said to be dissolved in the magma. In a bottle of carbonated beverage, the gas molecules are CO 2, and as long as the cap is on, the pressure in the bottle is high, and the CO 2 molecules are dissolved in the beverage. When the pressure on a magma is decreased, usually by the fact that the magma is moving upward in a conduit so that there is less and less material pressing down on it, the gas molecules start to become able to glom together into little regions of pure gas. We call these little regions of pure gas bubbles. This process is called exsolution - the gas is said to have exsolved. If there is initially a lot dissolved gas, and it exsolves rapidly, you will end up with a lot of bubbles. If they can t float up through, and escape out of, the magma, they will get trapped in it when it solidifies. A solidified bubble is called a vesicle. Pumice is an extreme form of this natural, glassy, foam. By definition, the vesicles in pumice are not connected. This means that pumice doesn t get waterlogged and can therefore float. There is often an intimate mixing of pumice and obsidian, meaning that the gas in some parts of a magma was able to exsolve, whereas that in other parts wasn t. Pumice is commonly light in color. Scoria and Reticulite Two other types of very bubbly rocks are scoria and reticulite. Both of these typically form in eruptions of mafic lava (see below), when there are high lava fountains. Scoria is sometimes called cinder, and it is what lots of people buy to mix in with potting soil for their gardens. It can be as high as 75% vesicles, but this isn t high enough to overcome the relatively high density of typical mafic lava compositions, so scoria doesn t float. Another type of very bubbly natural glass, also associated with high lava fountains of mafic lava, is called reticulite, and it can be as much as 95% vesicles! In fact, the only thing holding reticulate together is the thin septa between bubbles. Reticulite is pretty spectacular when viewed with a hand lens. The vesicles in reticulite are interconnected so if you put a piece of it in water it will eventually become waterlogged and sink. Reticulite is very fragile, so please handle it with care. Pele s Hair Early western geologists were fascinated by thin strands of basalt-composition glass that they found lying around on Kīlauea. They (not Hawaiians) named this material Pele s hair. Pele s hair consists of thin, flexible strands of glass that is usually golden to green-brown in color. It forms in high lava fountains when a piece of molten lava is pulled apart as it flies through the air. A thin filament gets pulled out between the two pieces, and it eventually breaks as they separate. The pieces of lava (scoria, usually) fall directly to the ground whereas the Pele s hair may be carried many kilometers by the wind before it lands. Pele s hair can also form when a stream of lava issues from a break in a tube. If the tube is flowing full, the surface of the lava will be dragged by the ceiling, and parts of it will be pulled into long strands of Pele s hair.

8 V Ultramafic Rocks: Ultramafic rocks are usually easy to identify because they commonly consist of only 1 or two minerals (olivine and pyroxene). Both these minerals are quite dense, so ultramafic rocks are also quite dense. Although there are lots of ultramafic rock names, you can get by with only 3: Mineral assemblage Ultramafic rock name >90% olivine Dunite olivine+pyroxene peridotite >90% pyroxene Pyroxenite Most ultramafic rocks are coarse-grained, but they didn t crystallize out of a magma the same way that real igneous rocks do, so most geologists would probably question considering them as phaneritic. Dunites, for example, often consist of olivines that formed in a magma chamber and sank to the bottom where they collected and got stuck together. Even though the olivines crystallized out of a magma, there was never a magma that consisted of pure molten olivine. There are no fine-grained equivalents of ultramafic rocks any more, because magmas of this ultramafic composition don t exist. However, back in the Archean (~3 billion years ago), lavas of this composition were erupted on Earth. They are called komatiites. Although ultramafic rocks are very rare in the Earth s upper crust, they probably make up almost all of the mantle. How do we even know what s down there? The main way is through xenoliths foreign rocks, that are brought up in some volcanic eruptions. The ultramafic rocks in Rock Set 5 were all brought up by eruptions at Hawaiian volcanoes.