Plate tectonics is a scientific theory that explains the movements and behaviors of the Earth’s lithosphere, which is composed of the crust and uppermost mantle. The theory proposes that the Earth’s lithosphere is broken into a series of plates that are in constant motion, driven by the heat generated from the Earth’s core. As these plates move, they interact with each other, leading to a wide range of geological phenomena, such as earthquakes, volcanic eruptions, and the formation of mountain ranges.

The theory of plate tectonics was developed in the 1960s and 1970s, based on a combination of geophysical data and observations of the Earth’s surface features. It replaced earlier theories of “continental drift” and “sea-floor spreading” and provided a unifying framework for understanding the Earth’s geological history and the distribution of natural resources.

Some of the key concepts related to plate tectonics include the types of plate boundaries, the processes of subduction and sea-floor spreading, the formation of mountains and oceanic ridges, and the distribution of earthquakes and volcanic activity around the world. Plate tectonics has important implications for our understanding of natural hazards, climate change, and the evolution of life on Earth.

Plate Tectonic Theory

Beyond merely describing current plate motions, Plate Tectonics provides an overarching framework that connects many elements of Earth science. Plate tectonics is a relatively young scientific theory that needed the advancement of observational and computing technology in the 1950s and 1960s to become fully elaborated. Its explanatory gravitas and the weight of observational evidence overcame much initial skepticism over how mobile the Earth’s surface really is, and Plate Tectonics quickly became universally accepted by scientists throughout the world.

Historical development of Plate Tectonics theory

The theory of Plate Tectonics is one of the most fundamental and influential theories in the field of geology. The theory explains the structure of the Earth’s lithosphere and the processes that drive the movement of Earth’s tectonic plates. The development of Plate Tectonics theory is the result of the contributions of many scientists over several centuries. Here are some of the key developments in the historical development of Plate Tectonics theory:

  1. Continental Drift hypothesis by Alfred Wegener (1912): The idea that the continents were once connected and have since drifted apart was first proposed by Alfred Wegener in 1912. Wegener based his hypothesis on the fit of the continents, similarities in rock types and fossils on opposite sides of the Atlantic, and evidence of past glaciation.
  2. Paleomagnetism studies (1950s): In the 1950s, studies of the magnetization of rocks on the ocean floor showed that the oceanic crust had a pattern of magnetic stripes that was symmetrical about mid-ocean ridges. This pattern provided evidence of seafloor spreading and helped to support the idea of continental drift.
  3. Vine-Matthews-Morley hypothesis (1963): In 1963, Fred Vine, Drummond Matthews, and Lawrence Morley proposed a hypothesis that explained the symmetrical magnetic stripes on the seafloor in terms of seafloor spreading. The hypothesis suggested that new oceanic crust was formed at mid-ocean ridges and then moved away from the ridges in opposite directions, creating a pattern of magnetic stripes.
  4. Theory of Plate Tectonics (late 1960s): In the late 1960s, the idea of continental drift and seafloor spreading were combined into the Theory of Plate Tectonics. The theory explains the movement of the Earth’s lithospheric plates, which are made up of the continents and oceanic crust. The plates move in response to forces generated by the mantle convection, and they interact at plate boundaries, which are associated with earthquakes, volcanic activity, and mountain building.
  5. Subsequent refinements: Since the development of Plate Tectonics theory, there have been many refinements and advances in our understanding of plate motion and plate boundaries. These include the recognition of different types of plate boundaries (e.g., divergent, convergent, and transform), the study of hotspots and mantle plumes, and the use of global positioning system (GPS) to track plate motion.

Evidence for the theory

The theory of plate tectonics is supported by a wide range of evidence from various fields of study. Here are some examples:

  1. Paleomagnetism: Rocks contain tiny magnetic minerals that align themselves with the Earth’s magnetic field when they are formed. By measuring the orientation of these minerals, scientists can determine the latitude at which the rock was formed. When rocks from different continents are compared, they show that their magnetic orientations match up as if they were once joined together.
  2. Seafloor spreading: The mid-ocean ridges, where new oceanic crust is formed, are the longest mountain ranges on Earth. As magma rises and solidifies at the ridges, it creates new oceanic crust that moves away from the ridge in opposite directions. By measuring the ages of the rocks on either side of the ridge, scientists have shown that the seafloor is spreading apart.
  3. Earthquakes and volcanoes: Most earthquakes and volcanoes occur at plate boundaries, providing further evidence that the plates are moving.
  4. GPS measurements: Global positioning system (GPS) technology allows scientists to measure the movement of Earth’s plates with great accuracy. These measurements confirm that the plates are indeed moving, and provide information about the rates and directions of plate motion.
  5. Fossil evidence: Fossils of identical organisms have been found on opposite sides of the Atlantic Ocean, indicating that the continents were once joined together.

Overall, the theory of plate tectonics is supported by a large body of evidence from a variety of sources, providing a robust explanation for the movements and interactions of Earth’s lithospheric plates.

Plate Boundaries: Types and Characteristics

Plate boundaries refer to the zones where the plates that make up the Earth’s lithosphere interact. There are three main types of plate boundaries: divergent, convergent, and transform. Each type is characterized by specific features and geological processes.

  1. Divergent Plate Boundaries: These occur where plates move away from each other. Magma rises from the mantle and creates new crust as it cools and solidifies. This process is called seafloor spreading and results in the formation of mid-ocean ridges. Divergent boundaries also occur on land, where they create rift valleys. Examples of divergent boundaries include the Mid-Atlantic Ridge and the East African Rift Zone.
  2. Convergent Plate Boundaries: These occur where plates move towards each other. There are three types of convergent boundaries, depending on the type of plates involved: oceanic-oceanic, oceanic-continental, and continental-continental. At an oceanic-oceanic convergent boundary, one plate subducts (dives beneath) the other, and a deep-sea trench is formed. The subduction also creates a volcanic arc on the overriding plate. Examples of oceanic-oceanic convergent boundaries include the Aleutian Islands and the Mariana Islands. At an oceanic-continental convergent boundary, the denser oceanic plate subducts beneath the less dense continental plate, creating a continental volcanic arc. Examples of oceanic-continental convergent boundaries include the Andes and the Cascades. At a continental-continental convergent boundary, neither plate subducts because they are too buoyant. Instead, they crumple and fold, creating large mountain ranges. Examples of continental-continental convergent boundaries include the Himalayas and the Appalachian Mountains.
  3. Transform Plate Boundaries: These occur where plates slide past each other. They are characterized by strike-slip faults, where the movement is horizontal rather than vertical. Transform boundaries are associated with earthquakes, and the most famous example is the San Andreas Fault in California.

The characteristics of plate boundaries are related to the type of plate interaction and the geological processes that occur at these boundaries. Understanding the types of plate boundaries is crucial for understanding plate tectonics and the geological processes that shape our planet.

Plate boundaries

How plate tectonics works

Plate tectonics is the theory that describes the movement of large segments of the Earth’s lithosphere (crust and uppermost part of the mantle) on top of the weaker asthenosphere. The lithosphere is broken up into a series of plates that move relative to one another at rates of a few centimeters per year. The movement of these plates is driven by forces generated within the Earth’s interior.

The process of plate tectonics involves the following steps:

  1. Creation of new oceanic lithosphere at mid-ocean ridges, where magma rises from the mantle and solidifies to form new crust. This is called seafloor spreading.
  2. Destruction of old oceanic lithosphere at subduction zones, where one plate is forced beneath another into the mantle. This process is accompanied by the release of seismic energy, causing earthquakes.
  3. Movement of plates due to the forces generated at their boundaries, which can be divergent, convergent or transform.
  4. Interactions between the plates, which can cause the formation of mountains, the opening or closing of ocean basins, and the formation of volcanoes.

Overall, the movement of the Earth’s plates is responsible for many of the geological features we observe on our planet.

What are the plates?

Earth’s lithosphere, which is the outermost solid layer of the Earth, is divided into several large and small plates that float on the underlying, ductile asthenosphere. These plates are composed of the Earth’s crust and the uppermost portion of the mantle, and they can move independently of one another. There are about a dozen major plates, which are the Pacific, North American, South American, Eurasian, African, Indo-Australian, Antarctic, and Nazca plates, and several smaller plates.

Plate boundaries

Plate boundaries are the regions where two or more tectonic plates meet. There are three main types of plate boundaries: divergent boundaries, where plates move apart from each other; convergent boundaries, where plates move towards each other and collide; and transform boundaries, where plates slide past each other. These boundaries are characterized by specific geological features and phenomena, such as rift valleys, mid-ocean ridges, subduction zones, and earthquakes. The interactions between plates at their boundaries are responsible for many geological processes, including mountain building, volcanic activity, and the formation of ocean basins.

Divergent Boundaries: Features and Examples

Divergent boundaries are locations where two tectonic plates move away from each other. These boundaries can be found both on land and under the ocean. As the plates move apart, magma rises to the surface and cools to form new crust, which creates a gap or rift between the plates.

Features of Divergent Boundaries:

  • Mid-ocean ridges: Underwater mountain ranges that form at divergent boundaries between oceanic plates. The most extensive and best-known mid-ocean ridge is the Mid-Atlantic Ridge.
  • Rift valleys: Deep valleys that form on land at divergent plate boundaries, such as the East African Rift Valley.
  • Volcanoes: When magma rises to the surface at divergent boundaries, it can form volcanoes, especially in areas where the boundary is under the ocean. These volcanoes are typically shield volcanoes, which are broad and gently sloping.

Examples of Divergent Boundaries:

  • Mid-Atlantic Ridge: The boundary between the North American Plate and the Eurasian Plate.
  • East African Rift Valley: The boundary between the African Plate and the Arabian Plate.
  • Iceland: A volcanic island that sits on the Mid-Atlantic Ridge at the boundary between the North American Plate and the Eurasian Plate.

Convergent Boundaries: Features and Examples

Convergent boundaries are areas where two tectonic plates collide. The characteristics and features of these boundaries depend on the type of plates that are converging, whether they are oceanic or continental plates, and their relative densities. There are three types of convergent boundaries:

  1. Oceanic-continental convergence: In this type of convergence, an oceanic plate subducts beneath a continental plate, forming a deep oceanic trench and a volcanic mountain chain. The subduction of the oceanic plate creates a partial melting of the mantle, which leads to the formation of magma. The magma rises to the surface and creates a volcanic mountain chain on the continental plate. Examples of this type of boundary include the Andes Mountains in South America and the Cascade Range in North America.
  2. Oceanic-oceanic convergence: In this type of convergence, one oceanic plate subducts beneath another oceanic plate, forming a deep oceanic trench and a volcanic island arc. The subduction of the oceanic plate creates a partial melting of the mantle, which leads to the formation of magma. The magma rises to the surface and creates a volcanic island arc. Examples of this type of boundary include the Aleutian Islands in Alaska and the Mariana Islands in the western Pacific.
  3. Continental-continental convergence: In this type of convergence, two continental plates collide, forming a high mountain range. Since both continental plates have similar densities, neither can be subducted. Instead, the plates are pushed upwards, forming a high mountain range with extensive folding and faulting. Examples of this type of boundary include the Himalayas in Asia and the Appalachian Mountains in North America.

At convergent boundaries, earthquakes, volcanic eruptions, and the formation of mountain ranges are common features due to the intense geologic activity that occurs at these locations.

Transform Boundaries: Features and Examples

Transform boundaries are zones where two tectonic plates slide past each other in a horizontal motion. These boundaries are also known as conservative boundaries since there is no net creation or destruction of lithosphere. Here are some of the features and examples of transform boundaries:


  • Transform boundaries are typically characterized by a series of parallel faults or fractures in the lithosphere.
  • The faults associated with transform boundaries can range from a few meters to hundreds of kilometers in length.
  • Transform boundaries can create linear features on the Earth’s surface, such as valleys or ridges.
  • The movement of the plates along transform boundaries can create earthquakes.


  • The San Andreas Fault in California is a well-known example of a transform boundary. It marks the boundary between the North American Plate and the Pacific Plate.
  • The Alpine Fault in New Zealand is another example of a transform boundary, marking the boundary between the Pacific Plate and the Australian Plate.
  • The Dead Sea Transform in the Middle East is a complex system of transform faults that connect the Red Sea Rift to the East Anatolian Fault Zone.

Transform boundaries play an important role in plate tectonics, as they help to accommodate the movement of plates along the Earth’s surface.

Plate Motion and Plate Kinematics

Plate motion refers to the movement of tectonic plates relative to each other. The study of plate motion is called plate kinematics. Plate kinematics involves measuring the direction, rate, and style of movement of tectonic plates.

Plate motion is driven by the movement of magma in the mantle, which causes the plates to move in different directions and at different speeds. The movement of plates can be measured using a variety of techniques, including GPS (Global Positioning System) and satellite imagery.

There are three types of plate boundaries: divergent, convergent, and transform. At divergent boundaries, two plates move away from each other, creating new crust in the process. At convergent boundaries, two plates move towards each other, and the denser oceanic plate is subducted beneath the less dense continental plate. At transform boundaries, two plates slide past each other horizontally.

The direction and speed of plate motion can be affected by a variety of factors, including the density and thickness of the lithosphere, the strength and orientation of the lithospheric plates, and the distribution of mantle convection cells. The study of plate kinematics is essential to understanding the formation and evolution of the Earth’s crust, as well as to predicting and mitigating the effects of earthquakes and volcanic eruptions.

Driving Forces of Plate Tectonics

The driving forces of plate tectonics are the forces that cause the movement of the Earth’s tectonic plates. There are two main types of driving forces:

  1. Ridge push: This force is caused by the upward push of magma at mid-ocean ridges, which creates new oceanic crust. As the new crust forms, it pushes the older crust away from the ridge, causing it to move.
  2. Slab pull: This force is caused by the weight of subducting oceanic lithosphere, which pulls the rest of the plate towards the subduction zone. As the plate is pulled, it can cause deformation, earthquakes, and volcanic activity.

Other possible driving forces of plate tectonics include mantle convection, which is the slow movement of the Earth’s mantle due to heat from the core, and gravitational forces, which can cause lateral movement of plates.

Plate Tectonics and Earthquakes

Plate tectonics and earthquakes are closely related phenomena. Earthquakes occur when two plates interact at their boundaries. Plate boundaries are classified into three types: divergent, convergent, and transform. Earthquakes occur at all three types of boundaries, but the characteristics of the earthquakes differ depending on the boundary type.

At divergent boundaries, earthquakes tend to be shallow and low-magnitude. This is because the plates are moving apart and there is relatively little friction and stress on the rocks. However, as the plates move further apart, the depth of the earthquakes can increase.

At convergent boundaries, earthquakes can be deep and high-magnitude. This is because the plates are colliding, and the rocks are under high stress and pressure. Subduction zones, where one plate is forced beneath another, are particularly prone to large, destructive earthquakes.

Transform boundaries also experience large earthquakes. These boundaries occur where two plates are sliding past each other horizontally. The friction and pressure on the rocks can lead to large earthquakes.

Overall, plate tectonics is the driving force behind most earthquakes on Earth, and understanding the movement and interactions of tectonic plates is crucial for predicting and mitigating earthquake hazards.

Plate Tectonics and Volcanism

Plate tectonics and volcanism are closely related because the majority of Earth’s volcanic activity occurs at plate boundaries. Magma rises from the mantle and is forced upward by tectonic plate movement, creating volcanic eruptions. The type of volcano and eruption style is determined by the composition and viscosity of the magma.

At divergent plate boundaries, magma rises from the mantle to create new crust, forming shield volcanoes that are typically non-explosive. Mid-ocean ridges are examples of this type of volcanic activity.

At convergent plate boundaries, the denser oceanic plate subducts beneath the less dense continental plate, melting the subducted plate to form magma. This type of volcanic activity can result in explosive eruptions and the formation of stratovolcanoes. The Pacific Ring of Fire is a zone of intense volcanic activity that occurs at convergent plate boundaries.

Transform plate boundaries do not typically produce volcanic activity, but they can create volcanic features such as fissure eruptions and volcanic vents.

In summary, plate tectonics plays a significant role in the formation and location of volcanoes, and the type of volcanic activity is determined by the plate boundary type and magma composition.

Plate Tectonics and Mountain Building

Plate tectonics plays a significant role in mountain building or orogeny. Mountains are formed by the deformation and uplift of the Earth’s crust. There are two types of mountain-building processes: 1) convergent boundary mountain building and 2) intraplate mountain building.

  1. Convergent boundary mountain building occurs where two tectonic plates collide and cause uplift and deformation. The most prominent example of this type of mountain building is the Himalayan mountain range. The Indian subcontinent collided with the Eurasian plate, causing the uplift of the Himalayas.
  2. Intraplate mountain building occurs where a tectonic plate moves over a mantle plume. As the plate moves over the plume, magma rises to the surface, creating volcanic islands and a chain of mountains. The Hawaiian Islands are an example of intraplate mountain building.

Plate tectonics also plays a role in the formation of other geological structures, such as rift valleys and oceanic trenches. In rift valleys, the crust is pulled apart by tectonic forces, causing the formation of a valley. Oceanic trenches form at subduction zones, where one tectonic plate is pushed under another and into the mantle. As the plate descends, it bends and forms a deep trench.

Plate Tectonics and the Rock Cycle

Plate tectonics and the rock cycle are closely related processes that shape the Earth’s surface and the composition of its crust. The rock cycle describes the transformation of rocks from one type to another through geologic processes such as weathering, erosion, heat and pressure, and melting and solidification. Plate tectonics plays a significant role in the rock cycle by recycling and changing the Earth’s crust through subduction, collision, and rifting processes.

Subduction zones are areas where one tectonic plate is being forced beneath another, and they are associated with the formation of volcanic arcs and island arcs. As the subducting plate descends into the mantle, it heats up and releases water, which lowers the melting temperature of surrounding rocks and generates magma. This magma rises to the surface and forms volcanoes, which release new minerals and gases into the atmosphere.

Collision zones occur where two tectonic plates converge and uplifts the crust, leading to the formation of mountain ranges. The collision of the Indian and Eurasian plates, for example, created the Himalayan mountain range. This process also causes metamorphism of rocks, as the intense heat and pressure of the collision transforms them into new types of rocks.

Rifting zones are areas where tectonic plates are moving apart, leading to the formation of new ocean basins and mid-ocean ridges. As plates move apart, the crust is thinned, and magma rises to fill the gap, eventually solidifying and forming new crust. This process produces volcanic activity and can lead to the formation of new mineral deposits.

In summary, plate tectonics drives the rock cycle by creating new crust, recycling old crust, and transforming rocks through subduction, collision, and rifting processes.

Plate Tectonics and the Evolution of Life

Plate tectonics have played a significant role in the evolution of life on Earth. It has shaped the planet’s environment and allowed for the development and diversification of life over time. Here are some ways that plate tectonics has influenced the evolution of life:

  1. Formation of continents: Plate tectonics has caused the formation of continents and their movement over time. The separation and collision of continents have created diverse habitats for different types of organisms to evolve.
  2. Climate change: Plate tectonics has influenced climate change by changing the distribution of land and sea and the circulation patterns of the oceans and atmosphere. This has affected the evolution of species by creating new habitats and changing environmental conditions.
  3. Biogeography: The movement of continents has created barriers and pathways for the migration of species, leading to the development of unique ecosystems and biogeographic patterns.
  4. Volcanism: Plate tectonics has led to the formation of volcanoes, which have contributed to the evolution of life by providing new habitats and nutrient-rich soil.

Overall, plate tectonics has been a key factor in shaping the Earth’s environment and creating the conditions necessary for the evolution and diversification of life.

Plate Tectonics and Mineral Resources

Plate tectonics plays a significant role in the formation and distribution of mineral resources. Ore deposits, including precious metals such as gold, silver, and platinum, as well as industrial metals such as copper, zinc, and lead, are often associated with tectonic plate boundaries.

At convergent plate boundaries, subduction zones can generate large-scale mineral deposits, including porphyry copper, epithermal gold, and silver, and massive sulfide deposits. These deposits are formed by hydrothermal fluids that are released from the subducting slab and the overlying mantle wedge, causing mineral precipitation in the surrounding rocks.

In addition, mid-ocean ridges, where new oceanic crust is created, can host deposits of sulfide minerals that are rich in copper, zinc, and other metals. These deposits are formed by hydrothermal vents that release mineral-rich fluids into the surrounding seawater.

Plate tectonics also influences the formation of hydrocarbon deposits, such as oil and gas. These deposits are often found in sedimentary basins that are associated with rift valleys, passive margins, and convergent margins. Organic-rich sedimentary rocks are buried and heated over time, leading to the formation of hydrocarbons.

Overall, plate tectonics is a crucial factor in the formation and distribution of mineral resources, and understanding the geological processes associated with plate boundaries is essential for identifying and exploiting these resources.


Although most of Earth’s volcanic activity is concentrated along or adjacent to plate boundaries, there are some important exceptions in which this activity occurs within plates. Linear chains of islands, thousands of kilometres in length, that occur far from plate boundaries are the most notable examples. These island chains record a typical sequence of decreasing elevation along the chain, from volcanic island to fringing reef to atoll and finally to submerged seamount. An active volcano usually exists at one end of an island chain, with progressively older extinct volcanoes occurring along the rest of the chain. Canadian geophysicist J. Tuzo Wilson and American geophysicist W. Jason Morgan explained such topographic features as the result of hotspots.

The principal tectonic plates that make up Earth’s lithosphere. Also located are several dozen hot spots where plumes of hot mantle material are upwelling beneath the plates.Encyclopædia Britannica, Inc.

earthquake zones; volcanoesThe world’s earthquake zones occur in red bands and largely coincide with the boundaries of Earth’s tectonic plates. Black dots indicate active volcanoes, whereas open dots indicate inactive ones.Encyclopædia Britannica, Inc.

The number of these hotspots is uncertain (estimates range from 20 to 120), but most occur within a plate rather than at a plate boundary. Hotspots are thought to be the surface expression of giant plumes of heat, termed mantle plumes, that ascend from deep within the mantle, possibly from the core-mantle boundary, some 2,900 km (1,800 miles) below the surface. These plumes are thought to be stationary relative to the lithospheric plates that move over them. A volcano builds upon the surface of a plate directly above the plume. As the plate moves on, however, the volcano is separated from its underlying magma source and becomes extinct. Extinct volcanoes are eroded as they cool and subside to form fringing reefs and atolls, and eventually they sink below the surface of the sea to form a seamount. At the same time, a new active volcano forms directly above the mantle plume.

Diagram depicting the process of atoll formation. Atolls are formed from the remnant parts of sinking volcanic islands.Encyclopædia Britannica, Inc.

The best example of this process is preserved in the Hawaiian-Emperor seamount chain. The plume is presently situated beneath Hawaii, and a linear chain of islands, atolls, and seamounts extends 3,500 km (2,200 miles) northwest to Midway and a further 2,500 km (1,500 miles) north-northwest to the Aleutian Trench. The age at which volcanism became extinct along this chain gets progressively older with increasing distance from Hawaii—critical evidence that supports this theory. Hotspot volcanism is not restricted to the ocean basins; it also occurs within continents, as in the case of Yellowstone National Park in western North America.

Measurements suggest that hotspots may move relative to one another, a situation not predicted by the classical model, which describes the movement of lithospheric plates over stationary mantle plumes. This has led to challenges to this classic model. Furthermore, the relationship between hotspots and plumes is hotly debated. Proponents of the classical model maintain that these discrepancies are due to the effects of mantle circulation as the plumes ascend, a process called the mantle wind. Data from alternative models suggest that many plumes are not deep-rooted. Instead, they provide evidence that many mantle plumes occur as linear chains that inject magma into fractures, result from relatively shallow processes such as the localized presence of water-rich mantle, stem from the insulating properties of continental crust (which leads to the buildup of trapped mantle heat and decompression of the crust), or are due to instabilities in the interface between continental and oceanic crust. In addition, some geologists note that many geologic processes that others attribute to the behaviour of mantle plumes may be explained by other forces.

Reference Lists

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