Igneous rock
Deep within our planet and exploding onto its surface, molten rock continually reshapes Earth. Igneous rocks, born from the cooling and solidification of this fiery material, are the fundamental building blocks of continents and oceanic crust alike. Understanding them unlocks critical secrets about Earth's dynamic interior and its powerful geological story. Igneous rocks originate from molten rock, either deep within the Earth's crust and mantle or from volcanic eruptions on the surface. Their formation location dictates their texture: slow cooling underground creates large crystals, while rapid surface cooling results in fine-grained or glassy rocks. These fundamental rocks constitute the vast majority of Earth's crust and serve as invaluable records for dating geological events and understanding planetary dynamics.
AI Summary
Deep within our planet and exploding onto its surface, molten rock continually reshapes Earth. Igneous rocks, born from the cooling and solidification of this fiery material, are the fundamental building blocks of continents and oceanic crust alike. Understanding them unlocks critical secrets about Earth's dynamic interior and its powerful geological story.
- Igneous rocks originate from molten rock, either deep within the Earth's crust and mantle or from volcanic eruptions on the surface.
- Their formation location dictates their texture: slow cooling underground creates large crystals, while rapid surface cooling results in fine-grained or glassy rocks.
- These fundamental rocks constitute the vast majority of Earth's crust and serve as invaluable records for dating geological events and understanding planetary dynamics.
The Earth's Fiery Foundations
The word "igneous" comes from the Latin word "igneus," meaning "fiery," and it perfectly describes these rocks. Along with sedimentary and metamorphic rocks, igneous rocks are one of the three main types that form our planet's crust. They are quite literally born of fire, representing Earth's raw, molten beginnings.
At their core, igneous rocks are formed from the cooling and solidification of molten rock. When this molten rock is deep beneath the Earth's surface, contained within the crust or mantle, it's called magma. When it erupts onto the surface, perhaps through a volcano, it's called lava.
This molten rock—magma—originates from the partial melting of existing rocks deep within Earth's mantle or crust. What causes this intense melting? It usually comes down to one or more of three key geological processes: an increase in temperature, a decrease in pressure, or a change in the rock's chemical composition.
Two Worlds of Cooling: Intrusive vs. Extrusive
The journey a molten rock takes largely determines the type of igneous rock it becomes. If it cools and solidifies beneath the surface, hidden away, it forms intrusive igneous rocks. If it erupts and solidifies on the surface, exposed to the elements, it forms extrusive igneous rocks. This distinction is crucial to their appearance and properties.
Intrusive: The Slow-Cooked Giants
Intrusive rocks, also known as plutonic rocks, form deep within the Earth's crust. Here, surrounded by insulating "country rock," magma cools incredibly slowly—sometimes over hundreds of thousands to millions of years. This prolonged cooling allows individual mineral crystals ample time to grow large enough to be easily seen with the naked eye.
These subterranean formations can create impressive geological structures beneath the surface. Gigantic bodies of intrusive rock, called batholiths, form the cores of many major mountain ranges. When erosion strips away the overlying rock over eons, these vast, crystalline cores are finally exposed to the surface.
Intrusive bodies also include more modest features like sills, which are horizontal sheets that intrude between existing rock layers, and dikes, which are vertical sheets that cut across them. These reveal pathways of ancient magma flow.
Common examples of intrusive igneous rocks include: Granite (often forming large continental masses) Gabbro (a primary component of the lower oceanic crust) Diorite
Extrusive: The Fast and Furious
In stark contrast, extrusive igneous rocks, often called volcanic rocks, form when lava erupts onto the Earth's surface. Exposed to the cooler air or water, this molten rock cools very rapidly—sometimes in a matter of seconds or minutes. This speedy solidification means there's little time for large crystals to grow.
Because of their rapid cooling, extrusive rocks often have fine-grained textures, where individual crystals are too small to be seen without a microscope—this is called an aphanitic texture. Some lavas cool so quickly they form natural glass, like obsidian, with no visible crystal structure at all.
Extrusive rocks are not just about dramatic volcanic eruptions on land—known as subaerial eruptions. Much of this activity occurs unseen beneath our oceans. Mid-ocean ridges, for example, are sites of continuous submarine volcanic activity, creating new oceanic crust.
Common examples of extrusive igneous rocks include: Basalt (the most common type, forming vast lava flows and oceanic crust) Andesite (often found in volcanic arcs) Rhyolite (a silica-rich, often explosive lava)
The behavior of lava when it erupts is profoundly influenced by its viscosity—its resistance to flow. This, in turn, depends on its temperature, chemical composition (especially silica content), and the number of crystals already present. Hot, basaltic lavas, low in silica, flow like thick oil, forming long, thin flows with smooth, ropy surfaces known as pahoehoe.
Magmas rich in silica, like rhyolite, are much cooler and can be up to 10,000 times more viscous than basalt. These thick, sticky lavas often trap dissolved gases—primarily water vapor and carbon dioxide—which build up immense pressure. When this pressure is suddenly released, it leads to violent, explosive eruptions, sometimes shattering the rock.
The material violently ejected during these explosive eruptions is called pyroclastic material or tephra. This can range from fine volcanic ash that drifts for miles, forming widespread ash tuff deposits, to larger fragments like lapilli and volcanic bombs, which can create agglomerates or ignimbrites.
\text{Trapped Gases (e.g., H}_2\text{O, CO}_2) + \text{High Viscosity} + \text{Pressure Release} \rightarrow \text{Explosive Eruption}Telling Earth's Story
Igneous rocks are far more than just cooled lava; they are crucial storytellers for geologists. They constitute an astounding 90-95% of the upper 16 kilometers of the Earth's crust by volume, and most of our oceanic crust is built from them, making them fundamental to understanding our planet.
The specific minerals and overall chemistry of igneous rocks provide a direct window into the deep Earth. They reveal the composition of the lower crust or upper mantle where their parent magma originated, and even the intense temperature and pressure conditions present during their formation and ascent.
Perhaps most importantly, igneous rocks can be precisely dated using radiometric dating techniques, which measure the decay of radioactive isotopes within their minerals. This allows scientists to establish absolute ages for geological events, providing a critical timeline that helps calibrate the entire geological time scale of Earth's history.
Different types of igneous rocks are characteristic of specific tectonic environments, acting like fingerprints that help geologists reconstruct ancient plate movements and continental configurations. Beyond their scientific value, some igneous rocks are also rich sources of valuable mineral deposits, including ores of tungsten, tin, uranium, chromium, and platinum.
Deciphering Rock Identity: Classification
Classifying igneous rocks helps us organize, understand, and communicate their origins and properties. One of the most immediate and observable clues to a rock's identity is its texture—the size, shape, and arrangement of its mineral grains. This directly reflects how and where the magma cooled.
Texture: A Window into Cooling History
Rocks with crystals large enough to be seen with the naked eye are called phaneritic—a hallmark of slow-cooling intrusive rocks, like granite. Those with crystals too small to discern, requiring a microscope, are aphanitic, characteristic of rapidly-cooling extrusive rocks like basalt.
Sometimes, you'll find igneous rocks with a mixed texture: larger, distinct crystals, called phenocrysts, embedded within a much finer-grained matrix, known as groundmass. This porphyritic texture tells a tale of two cooling phases—one slow, allowing large crystals to grow, followed by a rapid cooling phase, often occurring during ascent and eruption.
Mineralogical Classification: The Internal Blueprint
Geologists also classify igneous rocks based on their mineral composition, which reflects the chemical makeup of the original magma. For most common igneous rocks, the key minerals are quartz, feldspars (alkali and plagioclase), feldspathoids, olivines, pyroxenes, amphiboles, and micas. Their relative proportions reveal much about the rock's identity.
The IUGS (International Union of Geological Sciences) provides a systematic mineralogical classification scheme. It uses the percentages of Quartz, Alkali Feldspar, Plagioclase, and Feldspathoid minerals (the QAPF components) to place a rock on a specialized diagram, immediately suggesting its precise name.
Key minerals used in mineralogical classification (QAPF): Quartz (Q) Alkali Feldspar (A) Plagioclase (P) Feldspathoid (F)
Chemical Classification: Elemental Fingerprints
For very fine-grained volcanic rocks or glassy ones, identifying individual minerals with a microscope can be challenging or impossible. In these cases, geologists turn to chemical classification, analyzing the rock's elemental composition—especially the percentages of silicon, oxygen, aluminum, sodium, potassium, calcium, iron, and magnesium.
Silica (SiO2) content is the single most important chemical factor in classifying igneous rocks. It forms the basis for broad categories that dictate many of a rock's properties, including its typical color, density, and even how explosively its magma might erupt.
| Composition Mode of occurrence Felsic (>63% SiO2) Intermediate (52% to 63% SiO2) Mafic (45% to 52% SiO2) Ultramafic (<45% SiO2) Intrusive Granite Diorite Gabbro Peridotite Extrusive Rhyolite Andesite Basalt Komatiite
Beyond silica, the total content of alkali metal oxides (Na2O and K2O) is crucial for classifying volcanic rocks. The TAS (Total Alkali versus Silica) diagram uses these two chemical components to precisely categorize most volcanic rocks, guiding geologists to their specific names and helping understand their origin.
Magma Series and Tectonic Settings: Global Connections
Igneous rocks don't just tell us what they are, but where they formed in the grand scheme of plate tectonics. Geologists recognize different "magma series"—like the tholeiitic, calc-alkaline, and alkaline series—each typically associated with specific tectonic environments on Earth.
Tholeiitic magmas, for instance, are characteristic of mid-ocean ridges, where new oceanic crust is constantly being formed by mantle upwelling. Calc-alkaline and alkaline magmas are more common in mature subduction zones, where one plate dives beneath another, melting as it descends, often leading to powerful volcanic arcs. This intricate relationship between rock chemistry and global tectonics highlights how intertwined Earth's systems truly are.
Evolving Ideas: A Brief History of Classification
The scientific classification of igneous rocks has evolved over centuries. Some names, like "basalt" and "granite," date back to ancient times or early naturalists like Georgius Agricola in the 16th century, long before modern geological understanding of their origins.
In the early 20th century, a push for more scientific rigor led American petrologists Cross, Iddings, Pirsson, and Washington to propose a "quantitative" classification based purely on chemical analysis. While their specific system was eventually abandoned for its impracticality in fieldwork, it profoundly influenced future approaches, laying groundwork for modern chemical classifications.
Article
Igneous rock
Geologic provinces of the world (USGS)
Igneous rock (igneous from Latin igneus 'fiery'), or magmatic rock, is one of the three main rock types, the others being sedimentary and metamorphic. Igneous rocks are formed through the cooling and solidification of magma or lava.
The magma can be derived from partial melts of existing rocks in a terrestrial planet's mantle or crust. Typically, the melting is caused by one or more of three processes: an increase in temperature, a decrease in pressure, or a change in composition. Solidification into rock occurs either below the surface as intrusive rocks or on the surface as extrusive rocks. Igneous rock may form with crystallization to form granular, crystalline rocks, or without crystallization to form natural glasses.
Igneous rocks occur in a wide range of geological settings: shields, platforms, orogens, basins, large igneous provinces, extended crust and oceanic crust.
Volcanic eruptions of lava are major sources of igneous rocks. (Mayon volcano in the Philippines, erupting in 2009)
Natural columns of igneous rock separated from each other by columnar joints, in Madeira
Geological significance
Igneous rock
Igneous and metamorphic rocks make up 90–95% of the top 16 kilometres (9.9 mi) of the Earth's crust by volume. Igneous rocks form about 15% of the Earth's current land surface. Most of the Earth's oceanic crust is made of igneous rock.
Igneous rocks are also geologically important because:
• their minerals and global chemistry give information about the composition of the lower crust or upper mantle from which their parent magma was extracted, and the temperature and pressure conditions that allowed this extraction; • their absolute ages can be obtained from various forms of radiometric dating and can be compared to adjacent geological strata, thus permitting calibration of the geological time scale; • their features are usually characteristic of a specific tectonic environment, allowing tectonic reconstructions (see plate tectonics); • in some special circumstances they host important mineral deposits (ores): for example, tungsten, tin, and uranium are commonly associated with granites and diorites, whereas ores of chromium and platinum are commonly associated with gabbros.
Geological setting
Igneous rock
Formation of igneous rock
Igneous rocks can be either intrusive (plutonic and hypabyssal) or extrusive (volcanic).
Intrusive
Basic types of intrusions:
Intrusive igneous rocks make up the majority of igneous rocks and are formed from magma that cools and solidifies within the crust of a planet. Bodies of intrusive rock are known as intrusions and are surrounded by pre-existing rock (called country rock). The country rock is an excellent thermal insulator, so the magma cools slowly, and intrusive rocks are coarse-grained (phaneritic). The mineral grains in such rocks can generally be identified with the naked eye. Intrusions can be classified according to the shape and size of the intrusive body and its relation to the bedding of the country rock into which it intrudes. Typical intrusive bodies are batholiths, stocks, laccoliths, sills and dikes. Common intrusive rocks are granite, gabbro, or diorite.
The central cores of major mountain ranges consist of intrusive igneous rocks. When exposed by erosion, these cores (called batholiths) may occupy huge areas of the Earth's surface.
Intrusive igneous rocks that form at depth within the crust are termed plutonic (or abyssal) rocks and are usually coarse-grained. Intrusive igneous rocks that form near the surface are termed subvolcanic or hypabyssal rocks and they are usually much finer-grained, often resembling volcanic rock. Hypabyssal rocks are less common than plutonic or volcanic rocks and often form dikes, sills, laccoliths, lopoliths, or phacoliths.
Extrusive
Extrusive igneous rock is made from lava released by volcanoes
Sample of basalt (an extrusive igneous rock), found in Massachusetts
Extrusive igneous rock, also known as volcanic rock, is formed by the cooling of molten magma on the earth's surface. The magma, which is brought to the surface through fissures or volcanic eruptions, rapidly solidifies. Hence such rocks are fine-grained (aphanitic) or even glassy. Basalt is the most common extrusive igneous rock and forms lava flows, lava sheets and lava plateaus. Some kinds of basalt solidify to form long polygonal columns. The Giant's Causeway in Antrim, Northern Ireland is an example.
The molten rock, which typically contains suspended crystals and dissolved gases, is called magma. It rises because it is less dense than the rock from which it was extracted. When magma reaches the surface, it is called lava. Eruptions of volcanoes into air are termed subaerial, whereas those occurring underneath the ocean are termed submarine. Black smokers and mid-ocean ridge basalt are examples of submarine volcanic activity.
The volume of extrusive rock erupted annually by volcanoes varies with tectonic setting. Extrusive rock is produced in the following proportions:
• divergent boundary: 73% • convergent boundary (subduction zone): 15% • hotspot: 12%.
The behaviour of lava depends upon its viscosity, which is determined by temperature, composition, and crystal content. High-temperature magma, most of which is basaltic in composition, behaves in a manner similar to thick oil and, as it cools, treacle. Long, thin basalt flows with pahoehoe surfaces are common. Intermediate composition magma, such as andesite, tends to form cinder cones of intermingled ash, tuff and lava, and may have a viscosity similar to thick, cold molasses or even rubber when erupted. Felsic magma, such as rhyolite, is usually erupted at low temperature and is up to 10,000 times as viscous as basalt. Volcanoes with rhyolitic magma commonly erupt explosively, and rhyolitic lava flows are typically of limited extent and have steep margins because the magma is so viscous.
Felsic and intermediate magmas that erupt often do so violently, with explosions driven by the release of dissolved gases—typically water vapour, but also carbon dioxide. Explosively erupted pyroclastic material is called tephra and includes tuff, agglomerate and ignimbrite. Fine volcanic ash is also erupted and forms ash tuff deposits, which can often cover vast areas.
Because volcanic rocks are mostly fine-grained or glassy, it is much more difficult to distinguish between the different types of extrusive igneous rocks than between different types of intrusive igneous rocks. Generally, the mineral constituents of fine-grained extrusive igneous rocks can only be determined by examination of thin sections of the rock under a microscope, so only an approximate classification can usually be made in the field. Although classification by mineral makeup is preferred by the IUGS, this is often impractical, and chemical classification is done instead using the TAS classification.
Classification
Igneous rock
Close-up of granite (an intrusive igneous rock)
Igneous rocks are classified according to mode of occurrence, texture, mineralogy, chemical composition, and the geometry of the igneous body.
The classification of the many types of igneous rocks can provide important information about the conditions under which they formed. Two important variables used for the classification of igneous rocks are particle size, which largely depends on the cooling history, and the mineral composition of the rock. Feldspars, quartz or feldspathoids, olivines, pyroxenes, amphiboles, and micas are all important minerals in the formation of almost all igneous rocks, and they are basic to the classification of these rocks. All other minerals present are regarded as nonessential in almost all igneous rocks and are called accessory minerals. Types of igneous rocks with other essential minerals are very rare, but include carbonatites, which contain essential carbonates.
In a simplified compositional classification, igneous rock types are categorized into felsic or mafic based on the abundance of silicate minerals in the Bowen's Series. Rocks dominated by quartz, plagioclase, alkali feldspar and muscovite are felsic. Mafic rocks are primarily composed of biotite, hornblende, pyroxene and olivine. Generally, felsic rocks are light colored and mafic rocks are darker colored.
For textural classification, igneous rocks that have crystals large enough to be seen by the naked eye are called phaneritic; those with crystals too small to be seen are called aphanitic. Generally speaking, phaneritic implies an intrusive origin or plutonic, indicating slow cooling; aphanitic are extrusive or volcanic, indicating rapid cooling.
An igneous rock with larger, clearly discernible crystals embedded in a finer-grained matrix is termed porphyry. Porphyritic texture develops when the larger crystals, called phenocrysts, grow to considerable size before the main mass of the magma crystallizes as finer-grained, uniform material called groundmass. Grain size in igneous rocks results from cooling time so porphyritic rocks are created when the magma has two distinct phases of cooling.
Igneous rocks are classified on the basis of texture and composition. Texture refers to the size, shape, and arrangement of the mineral grains or crystals of which the rock is composed.
Texture
Gabbro specimen showing phaneritic texture, from Rock Creek Canyon, eastern Sierra Nevada, California
Texture is an important criterion for the naming of volcanic rocks. The texture of volcanic rocks, including the size, shape, orientation, and distribution of mineral grains and the intergrain relationships, will determine whether the rock is termed a tuff, a pyroclastic lava or a simple lava. However, the texture is only a subordinate part of classifying volcanic rocks, as most often there needs to be chemical information gleaned from rocks with extremely fine-grained groundmass or from airfall tuffs, which may be formed from volcanic ash.
Textural criteria are less critical in classifying intrusive rocks where the majority of minerals will be visible to the naked eye or at least using a hand lens, magnifying glass or microscope. Plutonic rocks also tend to be less texturally varied and less prone to showing distinctive structural fabrics. Textural terms can be used to differentiate different intrusive phases of large plutons, for instance porphyritic margins to large intrusive bodies, porphyry stocks and subvolcanic dikes. Mineralogical classification is most often used to classify plutonic rocks. Chemical classifications are preferred to classify volcanic rocks, with phenocryst species used as a prefix, e.g. "olivine-bearing picrite" or "orthoclase-phyric rhyolite".
Mineralogical classification
Basic classification scheme for igneous rocks based on their mineral composition. If the approximate volume fractions of minerals in the rock are known, the rock name and silica content can be read off the diagram. This is not an exact method, because the classification of igneous rocks also depends on other components, yet in most cases it is a good first guess.
QAPF diagram
The IUGS recommends classifying igneous rocks by their mineral composition whenever possible. This is straightforward for coarse-grained intrusive igneous rock, but may require examination of thin sections under a microscope for fine-grained volcanic rock, and may be impossible for glassy volcanic rock. The rock must then be classified chemically.
Mineralogical classification of an intrusive rock begins by determining if the rock is ultramafic, a carbonatite, or a lamprophyre. An ultramafic rock contains more than 90% of iron- and magnesium-rich minerals such as hornblende, pyroxene, or olivine, and such rocks have their own classification scheme. Likewise, rocks containing more than 50% carbonate minerals are classified as carbonatites, while lamprophyres are rare ultrapotassic rocks. Both are further classified based on detailed mineralogy.
In the great majority of cases, the rock has a more typical mineral composition, with significant quartz, feldspars, or feldspathoids. Classification is based on the percentages of quartz, alkali feldspar, plagioclase, and feldspathoid out of the total fraction of the rock composed of these minerals, ignoring all other minerals present. These percentages place the rock somewhere on the QAPF diagram, which often immediately determines the rock type. In a few cases, such as the diorite-gabbro-anorthite field, additional mineralogical criteria must be applied to determine the final classification.
Where the mineralogy of a volcanic rock can be determined, it is classified using the same procedure, but with a modified QAPF diagram whose fields correspond to volcanic rock types.
Chemical classification and petrology
Total alkali versus silica classification scheme (TAS) as proposed in Le Maitre's 2002 Igneous Rocks – A classification and glossary of terms Blue area is roughly where alkaline rocks plot; yellow area is where subalkaline rocks plot.
When it is impractical to classify a volcanic rock by mineralogy, the rock must be classified chemically.
There are relatively few minerals that are important in the formation of common igneous rocks, because the magma from which the minerals crystallize is rich in only certain elements: silicon, oxygen, aluminium, sodium, potassium, calcium, iron, and magnesium. These are the elements that combine to form the silicate minerals, which account for over ninety percent of all igneous rocks. The chemistry of igneous rocks is expressed differently for major and minor elements and for trace elements. Contents of major and minor elements are conventionally expressed as weight percent oxides (e.g., 51% SiO2, and 1.50% TiO2). Abundances of trace elements are conventionally expressed as parts per million by weight (e.g., 420 ppm Ni, and 5.1 ppm Sm). The term "trace element" is typically used for elements present in most rocks at abundances less than 100 ppm or so, but some trace elements may be present in some rocks at abundances exceeding 1,000 ppm. The diversity of rock compositions has been defined by a huge mass of analytical data—over 230,000 rock analyses can be accessed on the web through a site sponsored by the U. S. National Science Foundation (see the External Link to EarthChem).
The single most important component is silica, SiO2, whether occurring as quartz or combined with other oxides as feldspars or other minerals. Both intrusive and volcanic rocks are grouped chemically by total silica content into broad categories.
• Felsic rocks have the highest content of silica, and are predominantly composed of the felsic minerals quartz and feldspar. These rocks (granite, rhyolite) are usually light coloured, and have a relatively low density. • Intermediate rocks have a moderate content of silica, and are predominantly composed of feldspars. These rocks (diorite, andesite) are typically darker in colour than felsic rocks and somewhat more dense. • Mafic rocks have a relatively low silica content and are composed mostly of pyroxenes, olivines and calcic plagioclase. These rocks (basalt, gabbro) are usually dark coloured, and have a higher density than felsic rocks. • Ultramafic rock is very low in silica, with more than 90% of mafic minerals (komatiite, dunite).
This classification is summarized in the following table:
<table><thead><tr><th></th><th>Composition</th></tr></thead><tbody><tr><td>Mode of occurrence</td><td>Felsic (>63% SiO2)</td><td>Intermediate (52% to 63% SiO2)</td><td>Mafic (45% to 52% SiO2)</td><td>Ultramafic (<45% SiO2)</td></tr><tr><td>Intrusive</td><td>Granite</td><td>Diorite</td><td>Gabbro</td><td>Peridotite</td></tr><tr><td>Extrusive</td><td>Rhyolite</td><td>Andesite</td><td>Basalt</td><td>Komatiite</td></tr></tbody></table>
The percentage of alkali metal oxides (Na2O plus K2O) is second only to silica in its importance for chemically classifying volcanic rock. The silica and alkali metal oxide percentages are used to place volcanic rock on the TAS diagram, which is sufficient to immediately classify most volcanic rocks. Rocks in some fields, such as the trachyandesite field, are further classified by the ratio of potassium to sodium (so that potassic trachyandesites are latites and sodic trachyandesites are benmoreites). Some of the more mafic fields are further subdivided or defined by normative mineralogy, in which an idealized mineral composition is calculated for the rock based on its chemical composition. For example, basanite is distinguished from tephrite by having a high normative olivine content.
Other refinements to the basic TAS classification include:
• Ultrapotassic – rocks containing molar K2O/Na2O >3. • Peralkaline – rocks containing molar (K2O + Na2O)/Al2O3 >1. • Peraluminous – rocks containing molar (K2O + Na2O + CaO)/Al2O3 <1.
In older terminology, silica oversaturated rocks were called silicic or acidic where the SiO2 was greater than 66% and the family term quartzolite was applied to the most silicic. A normative feldspathoid classifies a rock as silica-undersaturated; an example is nephelinite.
AFM ternary diagram showing the relative proportions of Na2O + K2O (A for Alkali earth metals), FeO + Fe2O3 (F), and MgO (M) with arrows showing the path of chemical variation in tholeiitic and calc-alkaline series magmas
• The tholeiitic series – basaltic andesites and andesites. • The calc-alkaline series – andesites. • The alkaline series – subgroups of alkaline basalts and the rare, very high potassium-bearing (i.e. shoshonitic) lavas.
The alkaline series is distinguishable from the other two on the TAS diagram, being higher in total alkali oxides for a given silica content, but the tholeiitic and calc-alkaline series occupy approximately the same part of the TAS diagram. They are distinguished by comparing total alkali with iron and magnesium content.
These three magma series occur in a range of plate tectonic settings. Tholeiitic magma series rocks are found, for example, at mid-ocean ridges, back-arc basins, oceanic islands formed by hotspots, island arcs and continental large igneous provinces.
All three series are found in relatively close proximity to each other at subduction zones where their distribution is related to depth and the age of the subduction zone. The tholeiitic magma series is well represented above young subduction zones formed by magma from relatively shallow depth. The calc-alkaline and alkaline series are seen in mature subduction zones, and are related to magma of greater depths. Andesite and basaltic andesite are the most abundant volcanic rock in island arc which is indicative of the calc-alkaline magmas. Some island arcs have distributed volcanic series as can be seen in the Japanese island arc system where the volcanic rocks change from tholeiite—calc-alkaline—alkaline with increasing distance from the trench.
History of classification
Some igneous rock names date to before the modern era of geology. For example, basalt as a description of a particular composition of lava-derived rock dates to Georgius Agricola in 1546 in his work De Natura Fossilium. The word granite goes back at least to the 1640s and is derived either from French granit or Italian granito, meaning simply "granulate rock". The term rhyolite was introduced in 1860 by the German traveler and geologist Ferdinand von Richthofen The naming of new rock types accelerated in the 19th century and peaked in the early 20th century.
Much of the early classification of igneous rocks was based on the geological age and occurrence of the rocks. However, in 1902, the American petrologists Charles Whitman Cross, Joseph P. Iddings, Louis V. Pirsson, and Henry Stephens Washington proposed that all existing classifications of igneous rocks should be discarded and replaced by a "quantitative" classification based on chemical analysis. They showed how vague, and often unscientific, much of the existing terminology was and argued that as the chemical composition of an igneous rock was its most fundamental characteristic, it should be elevated to prime position.
Geological occurrence, structure, mineralogical constitution—the hitherto accepted criteria for the discrimination of rock species—were relegated to the background. The completed rock analysis is first to be interpreted in terms of the rock-forming minerals which might be expected to be formed when the magma crystallizes, e.g., quartz feldspars, olivine, akermannite, Feldspathoids, magnetite, corundum, and so on, and the rocks are divided into groups strictly according to the relative proportion of these minerals to one another. This new classification scheme created a sensation, but was criticized for its lack of utility in fieldwork, and the classification scheme was abandoned by the 1960s. However, the concept of normative mineralogy has endured, and the work of Cross and his coinvestigators inspired a flurry of new classification schemes.
Among these was the classification scheme of M.A. Peacock, which divided igneous rocks into four series: the alkalic, the alkali-calcic, the calc-alkali, and the calcic series. His definition of the alkali series, and the term calc-alkali, continue in use as part of the widely used Irvine-Barager classification, along with W.Q. Kennedy's tholeiitic series.
By 1958, there were some 12 separate classification schemes and at least 1637 rock type names in use. In that year, Albert Streckeisen wrote a review article on igneous rock classification that ultimately led to the formation of the IUGG Subcommission of the Systematics of Igneous Rocks. By 1989 a single system of classification had been agreed upon, which was further revised in 2005. The number of recommended rock names was reduced to 316. These included a number of new names promulgated by the Subcommission.
Origin of magmas
Igneous rock
The Earth's crust averages about 35 kilometres (22 mi) thick under the continents, but averages only some 7–10 kilometres (4.3–6.2 mi) beneath the oceans. The continental crust is composed primarily of sedimentary rocks resting on a crystalline basement formed of a great variety of metamorphic and igneous rocks, including granulite and granite. Oceanic crust is composed primarily of basalt and gabbro. Both continental and oceanic crust rest on peridotite of the mantle.
Rocks may melt in response to a decrease in pressure, to a change in composition (such as an addition of water), to an increase in temperature, or to a combination of these processes.
Other mechanisms, such as melting from a meteorite impact, are less important today, but impacts during the accretion of the Earth led to extensive melting, and the outer several hundred kilometres of our early Earth was probably an ocean of magma. Impacts of large meteorites in the last few hundred million years have been proposed as one mechanism responsible for the extensive basalt magmatism of several large igneous provinces.
Decompression
Decompression melting occurs because of a decrease in pressure.
The solidus temperatures of most rocks (the temperatures below which they are completely solid) increase with increasing pressure in the absence of water. Peridotite at depth in the Earth's mantle may be hotter than its solidus temperature at some shallower level. If such rock rises during the convection of solid mantle, it will cool slightly as it expands in an adiabatic process, but the cooling is only about 0.3 °C per kilometre. Experimental studies of appropriate peridotite samples document that the solidus temperatures increase by 3 °C to 4 °C per kilometre. If the rock rises far enough, it will begin to melt. Melt droplets can coalesce into larger volumes and be intruded upwards. This process of melting from the upward movement of solid mantle is critical in the evolution of the Earth.
Decompression melting creates the ocean crust at mid-ocean ridges. It also causes volcanism in intraplate regions, such as Europe, Africa and the Pacific sea floor. There, it is variously attributed either to the rise of mantle plumes (the "Plume hypothesis") or to intraplate extension (the "Plate hypothesis").
Effects of water and carbon dioxide
The change of rock composition most responsible for the creation of magma is the addition of water. Water lowers the solidus temperature of rocks at a given pressure. For example, at a depth of about 100 kilometres, peridotite begins to melt near 800 °C in the presence of excess water, but near or above about 1,500 °C in the absence of water. Water is driven out of the oceanic lithosphere in subduction zones, and it causes melting in the overlying mantle. Hydrous magmas composed of basalt and andesite are produced directly and indirectly as results of dehydration during the subduction process. Such magmas, and those derived from them, build up island arcs such as those in the Pacific Ring of Fire. These magmas form rocks of the calc-alkaline series, an important part of the continental crust.
The addition of carbon dioxide is relatively a much less important cause of magma formation than the addition of water, but genesis of some silica-undersaturated magmas has been attributed to the dominance of carbon dioxide over water in their mantle source regions. In the presence of carbon dioxide, experiments document that the peridotite solidus temperature decreases by about 200 °C in a narrow pressure interval at pressures corresponding to a depth of about 70 km. At greater depths, carbon dioxide can have more effect: at depths to about 200 km, the temperatures of initial melting of a carbonated peridotite composition were determined to be 450 °C to 600 °C lower than for the same composition with no carbon dioxide. Magmas of rock types such as nephelinite, carbonatite, and kimberlite are among those that may be generated following an influx of carbon dioxide into mantle at depths greater than about 70 km.
Temperature increase
Increase in temperature is the most typical mechanism for formation of magma within continental crust. Such temperature increases can occur because of the upward intrusion of magma from the mantle. Temperatures can also exceed the solidus of a crustal rock in continental crust thickened by compression at a plate boundary. The plate boundary between the Indian and Asian continental masses provides a well-studied example, as the Tibetan Plateau just north of the boundary has crust about 80 kilometres thick, roughly twice the thickness of normal continental crust. Studies of electrical resistivity deduced from magnetotelluric data have detected a layer that appears to contain silicate melt and that stretches for at least 1,000 kilometres within the middle crust along the southern margin of the Tibetan Plateau. Granite and rhyolite are types of igneous rock commonly interpreted as products of the melting of continental crust because of increases in temperature. Temperature increases also may contribute to the melting of lithosphere dragged down in a subduction zone.
Magma evolution
Schematic diagrams showing the principles behind fractional crystallisation in a magma. While cooling, the magma evolves in composition because different minerals crystallize from the melt. 1: olivine crystallizes; 2: olivine and pyroxene crystallize; 3: pyroxene and plagioclase crystallize; 4: plagioclase crystallizes. At the bottom of the magma reservoir, a cumulate rock forms.
Main article: Igneous differentiation
Most magmas are fully melted only for small parts of their histories. More typically, they are mixes of melt and crystals, and sometimes also of gas bubbles. Melt, crystals, and bubbles usually have different densities, and so they can separate as magmas evolve.
As magma cools, minerals typically crystallize from the melt at different temperatures (fractional crystallization). As minerals crystallize, the composition of the residual melt typically changes. If crystals separate from the melt, then the residual melt will differ in composition from the parent magma. For instance, a magma of gabbroic composition can produce a residual melt of granitic composition if early formed crystals are separated from the magma. Gabbro may have a liquidus temperature near 1,200 °C, and the derivative granite-composition melt may have a liquidus temperature as low as about 700 °C. Incompatible elements are concentrated in the last residues of magma during fractional crystallization and in the first melts produced during partial melting: either process can form the magma that crystallizes to pegmatite, a rock type commonly enriched in incompatible elements. Bowen's reaction series is important for understanding the idealised sequence of fractional crystallisation of a magma. Clinopyroxene thermobarometry is used to determine temperature and pressure conditions at which magma differentiation occurred for specific igneous rocks.
Magma composition can be determined by processes other than partial melting and fractional crystallization. For instance, magmas commonly interact with rocks they intrude, both by melting those rocks and by reacting with them. Magmas of different compositions can mix with one another. In rare cases, melts can separate into two immiscible melts of contrasting compositions.
Etymology
Igneous rock
• The word igneous means composed of fire and is derived from the Latin root words of igni-, meaning fire, and -eous meaning composed of. • The term volcanic rock is derived from the Latin root words of Vulcan, the Roman god of fire, and -ic, meaning having some characteristics of. • The term plutonic rock is derived from the Latin root words of Pluto, the Roman god of the underworld, and -ic, meaning having some characteristics of.
Gallery
Igneous rock
• Kanaga volcano in the Aleutian Islands with a 1906 lava flow in the foreground • A "skylight" hole, about 6 m (20 ft) across, in a solidified lava crust reveals molten lava below (flowing towards the top right) in an eruption of Kīlauea in Hawaii • Devils Tower, an eroded laccolith in the Black Hills of Wyoming • A cascade of molten lava flowing into Aloi Crater during the 1969–1971 Mauna Ulu eruption of Kilauea volcano • Columnar jointing in the Alcantara Gorge, Sicily • A laccolith of granite (light-coloured) that was intruded into older sedimentary rocks (dark-coloured) at Cuernos del Paine, Torres del Paine National Park, Chile • An igneous intrusion cut by a pegmatite dike, which in turn is cut by a dolerite dike