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Introduction to Earth Sciences I Topic 4 Mantle Dynamics and Plate Tectonics Lecture 4.5: Subduction & Plate Collision In this lecture, we will cover four topics related to subduction. First, we will briefly discuss subduction zone earthquakes, following on the mention of arc volcanic hazards in the previous lecture. Second, we will introduce ideas about mountain building, resulting from unsuccessful subduction – “collision” – of neighboring continental plates. Third, we will introduce the recrystallization of rocks due to pressure and temperature, known as metamorphism. As it turns out, almost all metamorphic rocks have been recrystallized under conditions unique to subduction zones. Fourth, we will illustrate the concept that the growth of continents has proceeded largely from the amalgamation of arc crust and other small crustal fragments via subduction and collision. Subduction zone earthquakes QuickTime™ and a TIFF (LZW) decompressor are needed to see this picture. We begin this lecture with another view of the Wadati-Benioff zone, the zone of deepening earthquakes that define the top of descending, cold, oceanic plates in subduction zones. Here, in an image created by the Alaska Volcanological Observatory in Fairbanks, you can see the subduction zone beneath the Aleutian islands and south central Alaska deepening northward from the trench (red line). The Aleutian subduction zone has been the site of two of the three largest earthquakes ever recorded. One was the 1964 earthquake near Anchorage, in which more than 70 people died. Subduction zone earthquakes in general are extremely hazardous. Recent techniques for measuring motions of the Earth’s surface, related to the Global Positioning System (GPS) have made it much easier to understand and - in a sense - predict these earthquakes. The following two diagrams - from the web pages of Jeff Freymuller of the University of Alaska in Fairbanks, illustrate ground motion measured via GPS for the Kenai Peninsula south of Anchorage over a period of several years. The top diagram shows cumulative vertical motion, while the lower diagram shows horizontal motion in terms of velocities relative to the stable interior of Alaska. QuickTime™ and a TIFF (LZW) decompressor are needed to see this picture. QuickTime™ and a TIFF (LZW) decompressor are needed to see this picture. Freymuller and his colleagues have shown that these motions are completely consistent with elastic bending of the overthrust plate, which is currently completely coupled to the subducting Pacific plate. Elastic deformation means reversible deformation and, like a steel leaf spring, the more the elastic upper crust is bent, the higher the stresses which act to undo this deformation. Eventually, these elastic stresses will be sufficient to overcome friction on the subduction zone fault system, and another great earthquake will shake the Anchorage area. Freymuller et al. estimate that the 1964 Anchorage quake completely released stored elastic stress built up over hundreds of years, so - if the frictional properties of the subduction faults haven’t changed too much - it might be a while before the next one. Not all of the Aleutian subduction system is locked like it is in the Anchorage area. The following map, which is greatly reduced for reproduction here, is available online from the Alaska Volcano Observatory. Among other things, it shows the rupture areas of the largest earthquakes in pink. These include most of the Aleutian subduction zone, except for the notorious Shumagin gap. Since there haven’t been any great earthquakes recorded in this gap, if the subduction zone faults are locked, a big one may be immanent. However, GPS measurements have shown that this part of the subduction system is not locked. The overthrust plate is not undergoing measurable elastic deformation, and instead seems to be stably and quietly sliding over the subducting Pacific plate in this region. The inference is that the Shumagin gap is not a high hazard area ... it actually seems to be a low hazard area. QuickTime™ and a TIFF (LZW) decompressor are needed to see this picture. Subduction zone earthquakes, like other earthquakes, are generally interpreted in terms of elastic deformation followed by frictional failure along brittle faults, as we have done in the previous paragraphs. This is because viscous deformation, at higher temperatures and greater depths, is generally irreversible. Once deformed, the shape of things is permanently changed and won’t “bounce back”. The following diagram summarizes some important differences between elastic and brittle behavior, on the one hand, and viscous deformation on the other. QuickTime™ and a TIFF (LZW) decompressor are needed to see this picture. As noted in the figure above, elastic/brittle deformation generally occurs in relatively cold rocks, and/or as a result of relatively rapid movement, while viscous deformation occurs at higher temperatures and/or in response to slower movements. Brittle deformation - the permanent component of elastic/brittle behavior - is highly localized along thin fractures, whereas conventionally it is supposed that viscous deformation is much more broadly distributed. There is a dramatic decrease in the number of earthquakes along Wadati-Benioff zones below a depth of 50 to 70 km, and this is interpreted in terms of a transition from brittle to ductile deformation along the subduction fault system. However, some observations don’t fit this explanation very well. Again, we reproduce here the tomographic image of the NE Japan subduction zone from Zhao et al., 1992. Now we wish to focus on the extensive occurrence of earthquakes at greater than 70 km depth. They may be rare compared to shallower quakes, but they certainly do occur. Also, in this data set, one can clearly see a double seismic zone, with a dipping plane of earthquakes about 50 km below the top of the subducting oceanic plate. The rocks here started out quite a bit hotter than the top of the subducting crust. A first-order estimate for the temperature at 50 km in an old oceanic plate would be about 700°C, and this can only be increased by conductive heating during subduction into the hotter mantle. All the earthquakes in this diagram below 70 km depth are usually called “intermediate depth earthquakes” (because there are even deeper ones). Some scientists have proposed a role for subducted H2O in causing intermediate depth earthquakes. Release of H2O bound in minerals, during chemical reactions driven by conductive heating of the subducting plate, could cause “dehydration embrittlement”. Never mind what this is, in detail. This might be an OK explanation for intermediate depth earthquakes along the top of the subducting plate, but how about the lower seismic zone? What evidence is there for penetration of H2O to 50 km depth in oceanic plates? An alternative may be that there are ductile mechanisms for earthquakes. Recently, scientists have begun to revisit an idea for periodic viscous heating along ductile shear zones, first proposed by Jack Whitehead in the 1970’s. Simply speaking, it might work as follows. Deformation is confined to narrow shear zones, which are pre-existing zones with very small crystals, because the strength of rocks is strongly dependent on grain size. Maybe the zones of small crystals originally form by crushing of crystals along brittle faults during earthquakes. Anyway, we know they exist, because we can find them in ophiolite mantle sections and other exposures of rocks from great depth. The strength, or viscosity of rocks depends on temperature as well as grain size. As stresses build up along a plate boundary, viscous deformation begins in the shear zone. Frictional heating begins to lower the viscosity, so the same stress leads to faster viscous deformation, which in turn heats the rock still more, in a feedback loop which ultimately results in release of all the stored stress in a rapid, viscous earthquake. With stress released, deformation and frictional heating stop, and the shear zone may cool conductively, getting ready for another cycle of instability. This could explain intermediate depth earthquakes, without a role for H2O or brittle failure. Continental collision We now turn to the topic of mountain building. The world’s highest mountain ranges are the HimalayaKarakorum mountains in Asia, the Alps and Caucasus in Europe, the Andes in South America, and the Alaska Range – St. Elias Mountains in North America. By far the largest of these is the Himalaya-Karakorum chain, including the high plateau of Tibet. This is produced by northward movement of the Indian continental plate into Eurasia. The following link leads to an animation of the motion of India relative to Eurasia and Africa, reconstructed on the basis of oceanic and continental paleomagnetic data: http://earth.leeds.ac.uk/dynamicearth/himalayas/india/anim ation.htm As you can see, the data show that India migrated northward until it collided with Eurasia, while the intervening ocean basin was consumed along a subduction zone along the south margin of Eurasia. This second animation shows a somewhat more speculative crosssectional history of the collision: http://earth.leeds.ac.uk/dynamicearth/himalayas/deformatio n/collide/index.htm As noted before, the continental crust is composed of lowdensity rocks rich in silicon, aluminum, sodium and potassium. Because it has such a low density, it is difficult or impossible to subduct large proportions of continental crust. Thus, scientists infer that the subducting oceanic plate north of India broke off, and was consumed into the mantle, while the continental crust in the Indian and Eurasian plates simply pushed together – thickening and rising as a result of compression. The resulting thickening of the continental crust on both sides of the original line of collision – called a “suture zone” – caused the mountains to rise. As noted earlier in the course, the elevation of a particular plate is largely controlled by its density. Like a block of wood in a pool of water, the crust floats on the viscously deforming mantle, and the height with which it floats depends on the density relative to the mantle and the thickness of the crust. QuickTime™ and a TIFF (LZW) decompressor are needed to see this picture. http://earth.leeds.ac.uk/dynamicearth/ For crust with different density and the same thickness, the less dense plate floats higher. For crust with the same density and different thickness, the thicker plate floats higher. http://earth.leeds.ac.uk/dynamicearth/ http://earth.leeds.ac.uk/dynamicearth/ QuickTime™ and a TIFF (LZW) decompressor are needed to see this picture. http://earth.leeds.ac.uk/dynamicearth/ The increased thickness of the crust due to the continental collision between India and Eurasia led to the formation of high mountains on both sides of the suture zone. Compression in the lower crust, due to plate collision, essentially folds and pushes low-density continental material upward and outward. Thus, compression in the deep interior of the Himalayas and other large mountains is accompanied by extension and outward growth of the mountain range near the surface. The following picture illustrates some of the complex features resulting from this process. Please don’t worry about or try to memorize the many technical terms used in this diagram. As mountains grow, erosion of the highest ridges becomes very rapid, due to the ordinary action of rainfall and wind, but also to additional mechanisms that are rare in more subdued terrain, such as glacial erosion, avalanches and landslides. Here is another schematic cross-section illustrating the effects of erosion as well as folding, uplift, and lateral extension of the mountain range due to collision. In this cross-section, all of the faults illustrated are still reverse, or thrust faults. However, sometimes the extension of the steep mountain range even produces extensional, normal faults. This can best be visualized as the result of piling up too much material in the middle of a mountain range with steep sides. The steep sides undergo “gravitational collapse” and the interior of the range extends outward. The previous three diagrams come from an excellent web site on mountain building, http://www.uwm.edu/Course/geosci697-tectonic/ Continental collisions don’t just cause compression and thickening of the crust. They also cause lateral motions. A famous paper by Tapponier & Molnar in J. Geophys. Res. proposed that the Chinese crust is being propelled eastward into the South China Sea (accommodated by subduction further east) as a result of the collision of India and Eurasia: Tapponier realized that the pattern of faults and crustal thickness in east Asia resembled deformation experiments in plastic materials, and went on to do a series of experiments with wooden blocks and putty that produced striking images of faults and deformation patterns similar to that seen in east Asia: This idea may have seemed pretty speculative to geoscientists in the 1980’s when it was first proposed, but has recently received dramatic confirmation from GPS measurements. The following diagram comes from a paper in J. Geophys. Res. this year: In this diagram, the velocities of the crust measured with a large number of GPS instruments are shown with arrows, and the ellipses indicate the uncertainty of the measurement. Colors indicate elevation, with green being low and tan being the highest. Large arrows along the front of the Himalayan mountains record continued collision of India into Eurasia. Smaller arrows to the north and east provide dramatic confirmation of Tapponier & Molnar’s hypothesis that China is moving eastward, driven by the plate collision to the south. Another example of this type of lateral “extrusion” is in northern Turkey, where a block is being pushed westward by collision between the Arabian and Eurasian plates, with much of the resulting, lateral motion between northern Turkey and Eurasia accommodated on the North Anatolian strike-slip fault. Unfortunately, this large fault is seismically active and passes through areas with high population density, leading to disasters such as the 1999 earthquake that killed more than 50,000 people. http://earth.leeds.ac.uk/dynamicearth/ This concludes our section on mountain building via continental collision, except to note that many older mountain ranges formed in the same way. Thus, the Urals in Asia and the Appalachians in North America are erosional remnants of Himalayan-style collisions that occurred hundreds of millions of years ago. Metamorphism Metamorphism occurs when changes in pressure and temperature cause recrystallization of rocks. So for example minerals which are stable – “happy” – at low temperature and pressure, like clays, break down as they are heated, giving rise to new minerals which are stable at higher temperature, such as micas. In turn, micas break down with the formation of garnet and feldspar and other minerals. Most of these changes also involve release of “volatiles”, like H2O and CO2, which are abundantly bound in the molecular structure of the low temperature minerals but are much less abundant in the high temperature minerals. We don’t have time to go into the details of this process. A good web page that illustrates some general concepts is http://www.ig.uit.no/~kaarek/geology_intro/metamorphism .swf What we do wish to emphasize here is that most metamorphism recorded by rocks that are exposed on the Earth’s surface occurred at depth in subduction zones and arcs. Part of the reason for this is that the minerals in rocks tend to record the highest temperature that the rock has experienced. The reason for this is that, as alluded to above, changes in minerals during heating evolve H2O and CO2 as gases and fluids, which then leave the rock. Because the H2O and CO2 are gone, it is hard for the low temperature minerals to form again as the rock cools and decompresses later in its history. So, the high temperature mineral assemblages are often preserved. And, for most crustal rocks, the highest temperature and pressure conditions they can reach are attained beneath subductionrelated volcanic arcs. To elaborate on this a little further, we need to illustrate typical geotherms for different tectonic settings. We found that most textbooks don’t do this very well, so we have made our own summary diagram: Continental interiors are old and cold. Nothing much has happened to them for millions or even billions of years, and meanwhile they have been losing heat by conduction to the Earth’s surface. We can estimate the temperature at a given depth beneath the continental interiors by looking at mineral compositions in blocks of mantle material from near the base of the plate (xenoliths) transported in explosive volcanic eruptions. Because the mineral compositions are sensitive to temperature and pressure, we can measure their compositions and estimate the conditions at which they formed. Also cold are subduction zones, because cold oceanic crust is being rapidly transported into the Earth’s interior, with little time to be conductively heated by the surrounding, hotter mantle. We’ve shown several figures – of thermal models for subduction zones, and seismic data – illustrating that this is true. As noted in the previous lecture, there is ample evidence that the crust beneath arcs is very hot at a given depth, compared to most other tectonic settings. This is so, apparently, because of upwelling of hot mantle material to replace cold material pulled from the base of the overthrust plate during subduction. Arcs are hotter than old oceanic plates, which generally are about 100 km thick and have undergone extensive cooling, losing heat to the oceans by conduction and hydrothermal convection. The hottest geotherms are for oceanic spreading centers, where hot mantle material rises almost to the seafloor, to replace colder material that is diverging due to plate spreading. Sometimes, continental plates undergo partial or complete rifting as a result of tectonic extension. This is happening in the “Basin and Range” province of Arizona, Nevada and Oregon now. Under these circumstances, the geotherm may approach arc or even oceanic spreading center temperatures. However, because old continental rocks have in many cases already undergone metamorphism, with loss of H2O and CO2, it is likely that continental rifting does not cause important metamorphic changes in the crust. Why go into all this? In order to illustrate that metamorphic rocks are mostly recrystallized in arcs. The following figure shows a summary of the pressure and temperature conditions recorded by metamorphic rocks worldwide, from Prof. John Winter’s web site and textbook. The labeled blue and purple lines, and the grey fields, show metamorphic conditions recorded by rocks from many different places. On this diagram are superimposed the geotherms we constructed and presented in the previous figure. Here, we are only looking at the shallowest, coldest parts of those curves. What you can see is that the great majority of metamorphic rocks (purple lines, grey fields) record such high temperatures at a given depth that they must have been recrystallized beneath an arc. In a few regions, there are belts of “high pressure, low temperature” metamorphic rocks (HP, shown with blue lines on the previous diagram), and even “ultra-high pressure” rocks (UHP, lying at higher pressures than in the previous diagram). These generally have very young radiometric ages, and still contain many hydrous minerals, so we know that they are not old, dehydrated rocks from continental interiors. Instead, they are rocks that were recrystallized during subduction, and that’s why they record such low temperatures at high pressure. If HP and UHP rocks began to subduct, how come they are now exposed on the surface for geologists to sample and study? It’s not certain, but scientists note that most of the UHP rocks are low density (meta) sediments and blocks of continental crust. Perhaps, they started to subduct, presumably while attached to an old, cold oceanic plate. But as they got hotter, their attachment to the old, dense material grew weaker, and eventually they “floated” buoyantly back to the surface. This scenario seems particularly likely in continental collision zones, and indeed UHP rocks are found close to the suture zones in the Himalaya, as well as along more ancient suture zones in the Alps and western Norway. Thus, while metamorphic rocks record both high and low temperatures at a given depth, they both were recrystallized in subduction-related tectonic settings, arcs for the higher temperature examples, and in the subducting plate itself for the lower temperature rocks. This is reflected in the fact that HP and UHP rocks are often found in “paired metamorphic belts”, together with higher temperature metamorphic rocks. QuickTime™ and a TIFF (LZW) decompressor are needed to see this picture. The diagram above illustrates two famous examples of paired metamorphic belts, from SW Japan associated with ongoing subduction, and in California associated with subduction that ended 50 million years ago. These paired belts appear to reflect the juxtaposition of very low heat flow and very high heat flow in the overthrust plate of subduction zones, as illustrated in the previous lecture. Continental accretion Finally, we wish to briefly mention that the process of collision and mountain building has probably played an important role in forming the continental crust. Collisional mountain belts are complicated, and often include many small fragments of young arc crust and metamorphosed, young sediments between larger, older continental blocks. Again, without going into detail, we use the diagram above to illustrate this. In this schematic mountain range (modeled on the southern Appalachians), there are several “suture zones” representing ocean basins that were consumed during collision. Between these sutures lie small fragments of buoyant crust that did not subduct. Some of these fragments are the remnants of arcs, others are fragments of older continents, perhaps broken off by rifting, and still others are metamorphosed piles of sediments, similar to those that accumulate in deep sea trenches today where rapid erosion and river transport leads to landslides into the steep, deep trenches. The following figure illustrates the tremendously complex geology of western North America, in which each small block outlined in black is a different fragment, whose geologic history prior to collision with North America along subduction zones was different from the history of all the surrounding fragments. Bit by bit, they are added to the margins of continents, and eventually some become incorporated in the continental interiors after big collision events. The next two illustrations show how this kind of accretionary tectonics has affected the eastern part of North America. In dark grey are fragments of the African continent, plus metamorphic and intrusive rocks that formed during a collision between Africa and North America. These were left behind QuickTime™ and a TIFF (LZW) decompressor when Africa rifted away from are needed to see this picture. North America, about 150 million years ago in this region, during formation of the modern Atlantic Ocean. The light grey rocks are sediments and arc rocks that were added to the North American margin during small collision events, and then caught in the big collision between Africa and North America. The resulting structure is shown in this schematic cross-section: QuickTime™ and a TIFF (Uncompressed) decompressor are needed to see this picture. The pink rocks used to belong to the African plate. The green rocks are ophiolites (remember them, fragments of oceanic crust thrust onto continental margins?). The grey rocks are metamorphosed rocks and sediments. And the red, yellow and orange rocks are sediments that were derived from the high mountains along the zone of continental collision, and accumulated to the west on the stable interior of the North American plate. You have to go north to see the fragments of old African crust, but the belt of metamorphosed arc rocks and sediments continues through the New York area, and can be seen as the Manhattan schist and Fordham gneiss in outcrops throughout the area, most famously in Central Park. If you go there – as some of you did during one of the lab sessions in this course – you will see sediments formed by submarine landslides, that were later metamorphosed and folded during the collisional events. This concludes the section on mantle convection and plate tectonics. We started off with simple principles of convection, and ended with the daunting complexity of continental tectonics and growth. Some things are easy to understand and well established, like the causes and structures of thermal convection, the evidence for seafloor spreading and subduction, the driving forces for plate tectonics due to hot new oceanic crust at spreading centers and cold, old subducting oceanic crust, the basic causes of melting beneath mid-ocean ridges and arcs, the causes of brittle subduction zone earthquakes, and the basic nature of metamorphism. Some things are less easy to understand, and are topics of ongoing scientific research. Some of these include the morphology of melt transport networks in the mantle, the cause(s) of intermediate depth earthquakes, and the fundamental principles that govern deformation during continental tectonics. We hope some of you will contribute to understanding these topics, or at least keep an educated eye on the newspapers to understand future developments.