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Clastic rock
Clastic rock
from Wikipedia
A thin section of a clast (sand grain), derived from a basalt scoria. Vesicles (air bubbles) can be seen throughout the clast. Plane-polarized light above, cross-polarized light below. Scale box is 0.25 mm.

Clastic rocks are composed of fragments, or clasts, of pre-existing minerals and rock. A clast is a fragment of geological detritus,[1] chunks, and smaller grains of rock broken off other rocks by physical weathering.[2] Geologists use the term clastic to refer to sedimentary rocks and particles in sediment transport, whether in suspension or as bed load, and in sediment deposits.

Sedimentary clastic rocks

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Claystone from Montana

Clastic sedimentary rocks are rocks composed predominantly of broken pieces or clasts of older weathered and eroded rocks. Clastic sediments or sedimentary rocks are classified based on grain size, clast and cementing material (matrix) composition, and texture. The classification factors are often useful in determining a sample's environment of deposition. An example of clastic environment would be a river system in which the full range of grains being transported by the moving water consist of pieces eroded from solid rock upstream.

Grain size varies from clay in shales and claystones; through silt in siltstones; sand in sandstones; and gravel, cobble, to boulder sized fragments in conglomerates and breccias. The Krumbein phi (φ) scale numerically orders these terms in a logarithmic size scale.

Siliciclastic sedimentary rocks

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Siliciclastic rocks are clastic noncarbonate rocks that are composed almost exclusively of silicon, either as forms of quartz or as silicates.

Composition

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The composition of siliciclastic sedimentary rocks includes the chemical and mineralogical components of the framework as well as the cementing material that make up these rocks. Boggs divides them into four categories; major minerals, accessory minerals, rock fragments, and chemical sediments.[3]

Major minerals can be categorized into subdivisions based on their resistance to chemical decomposition. Those that possess a great resistance to decomposition are categorized as stable, while those that do not are considered less stable. The most common stable mineral in siliciclastic sedimentary rocks is quartz (SiO2).[3] Quartz makes up approximately 65 percent of framework grains present in sandstones and about 30 percent of minerals in the average shale. Less stable minerals present in this type of rocks are feldspars, including both potassium and plagioclase feldspars.[3] Feldspars comprise a considerably lesser portion of framework grains and minerals. They only make up about 15 percent of framework grains in sandstones and 5% of minerals in shales. Clay mineral groups are mostly present in mudrocks (comprising more than 60% of the minerals) but can be found in other siliciclastic sedimentary rocks at considerably lower levels.[3]

Accessory minerals are associated with those whose presence in the rock are not directly important to the classification of the specimen. These generally occur in smaller amounts in comparison to the quartz, and feldspars. Furthermore, those that do occur are generally heavy minerals or coarse grained micas (both muscovite and biotite).[3]

Rock fragments also occur in the composition of siliciclastic sedimentary rocks and are responsible for about 10–15 percent of the composition of sandstone. They generally make up most of the gravel size particles in conglomerates but contribute only a very small amount to the composition of mudrocks. Though they sometimes are, rock fragments are not always sedimentary in origin. They can also be metamorphic or igneous.[3]

Chemical cements vary in abundance but are predominantly found in sandstones. The two major types are silicate based and carbonate based. The majority of silica cements are composed of quartz, but can include chert, opal, feldspars and zeolites.[3]

Composition includes the chemical and mineralogic make-up of the single or varied fragments and the cementing material (matrix) holding the clasts together as a rock. These differences are most commonly used in the framework grains of sandstones. Sandstones rich in quartz are called quartz arenites, those rich in feldspar are called arkoses, and those rich in lithics are called lithic sandstones.

Classification

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Siliciclastic sedimentary rocks are composed of mainly silicate particles derived from the weathering of older rocks and pyroclastic volcanism. While grain size, clast and cementing material (matrix) composition, and texture are important factors when regarding composition, siliciclastic sedimentary rocks are classified according to grain size into three major categories: conglomerates, sandstones, and mudrocks. The term clay is used to classify particles smaller than .0039 millimeters. However, the term can also be used to refer to a family of sheet silicate minerals.[3] Silt refers to particles that have a diameter between .062 and .0039 millimeters. The term mud is used when clay and silt particles are mixed in the sediment; mudrock is the name of the rock created with these sediments. Furthermore, particles that reach diameters between .062 and 2 millimeters fall into the category of sand. When sand is cemented together and lithified it becomes known as sandstone. Any particle that is larger than two millimeters is considered gravel. This category includes pebbles, cobbles and boulders. Like sandstone, when gravels are lithified they are considered conglomerates.[3]

Conglomerates and breccias
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Conglomerate
Breccia. Notice the angular nature of the large clasts

Conglomerates are coarse grained rocks dominantly composed of gravel sized particles that are typically held together by a finer grained matrix.[4] These rocks are often subdivided into conglomerates and breccias. The major characteristic that divides these two categories is the amount of rounding. The gravel sized particles that make up conglomerates are well rounded while in breccias they are angular. Conglomerates are common in stratigraphic successions of most, if not all, ages but only make up one percent or less, by weight, of the total sedimentary rock mass.[3] In terms of origin and depositional mechanisms they are very similar to sandstones. As a result, the two categories often contain the same sedimentary structures.[3]

Sandstones
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Sandstone from Lower Antelope Canyon

Sandstones are medium-grained rocks composed of rounded or angular fragments of sand size, that often but not always have a cement uniting them together. These sand-size particles are often quartz but there are a few common categories and a wide variety of classification schemes that classify sandstones based on composition. Classification schemes vary widely, but most geologists have adopted the Dott scheme,[5][better source needed] which uses the relative abundance of quartz, feldspar, and lithic framework grains and the abundance of muddy matrix between these larger grains.

Mudrocks
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Rocks that are classified as mudrocks are very fine grained. Silt and clay represent at least 50% of the material that mudrocks are composed of. Classification schemes for mudrocks tend to vary, but most are based on the grain size of the major constituents. In mudrocks, these are generally silt, and clay.[6]

According to Blatt, Middleton and Murray [7] mudrocks that are composed mainly of silt particles are classified as siltstones. In turn, rocks that possess clay as the majority particle are called claystones. In geology, a mixture of both silt and clay is called mud. Rocks that possess large amounts of both clay and silt are called mudstones. In some cases the term shale is also used to refer to mudrocks and is still widely accepted by most. However, others have used the term shale to further divide mudrocks based on the percentage of clay constituents. The plate-like shape of clay allows its particles to stack up one on top of another, creating laminae or beds. The more clay present in a given specimen, the more laminated a rock is. Shale, in this case, is reserved for mudrocks that are laminated, while mudstone refers those that are not.

Diagenesis of siliciclastic sedimentary rocks

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Siliciclastic rocks initially form as loosely packed sediment deposits including gravels, sands, and muds. The process of turning loose sediment into hard sedimentary rocks is called lithification. During the process of lithification, sediments undergo physical, chemical and mineralogical changes before becoming rock. The primary physical process in lithification is compaction. As sediment transport and deposition continues, new sediments are deposited atop previously deposited beds, burying them. Burial continues and the weight of overlying sediments causes an increase in temperature and pressure. This increase in temperature and pressure causes loose grained sediments become tightly packed, reducing porosity, essentially squeezing water out of the sediment. Porosity is further reduced by the precipitation of minerals into the remaining pore spaces.[3] The final stage in the process is diagenesis and will be discussed in detail below.

Cementation

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Cementation is the diagenetic process by which coarse clastic sediments become lithified or consolidated into hard, compact rocks, usually through the deposition or precipitation of minerals in the spaces between the individual grains of sediment.[4] Cementation can occur simultaneously with deposition or at another time. Furthermore, once a sediment is deposited, it becomes subject to cementation through the various stages of diagenesis discussed below.

Shallow burial (eogenesis)

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Eogenesis refers to the early stages of diagenesis. This can take place at very shallow depths, ranging from a few meters to tens of meters below the surface. The changes that occur during this diagenetic phase mainly relate to the reworking of the sediments. Compaction and grain repacking, bioturbation, as well as mineralogical changes all occur at varying degrees.[3] Due to the shallow depths, sediments undergo only minor compaction and grain rearrangement during this stage. Organisms rework sediment near the depositional interface by burrowing, crawling, and in some cases sediment ingestion. This process can destroy sedimentary structures that were present upon deposition of the sediment. Structures such as lamination will give way to new structures associated with the activity of organisms. Despite being close to the surface, eogenesis does provide conditions for important mineralogical changes to occur. This mainly involves the precipitation of new minerals.

Mineralogical changes during eogenesis
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Mineralogical changes that occur during eogenesis are dependent on the environment in which that sediment has been deposited. For example, the formation of pyrite is characteristic of reducing conditions in marine environments.[3] Pyrite can form as cement, or replace organic materials, such as wood fragments. Other important reactions include the formation of chlorite, glauconite, illite and iron oxide (if oxygenated pore water is present). The precipitation of potassium feldspar, quartz overgrowths, and carbonate cements also occurs under marine conditions. In non marine environments oxidizing conditions are almost always prevalent, meaning iron oxides are commonly produced along with kaolin group clay minerals. The precipitation of quartz and calcite cements may also occur in non marine conditions.

Deep burial (mesogenesis)

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Compaction
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As sediments are buried deeper, load pressures become greater resulting in tight grain packing and bed thinning. This causes increased pressure between grains thus increasing the solubility of grains. As a result, the partial dissolution of silicate grains occurs. This is called pressure solutions. Chemically speaking, increases in temperature can also cause chemical reaction rates to increase. This increases the solubility of most common minerals (aside from evaporites).[3] Furthermore, beds thin and porosity decreases allowing cementation to occur by the precipitation of silica or carbonate cements into remaining pore space.

In this process minerals crystallize from watery solutions that percolate through the pores between grain of sediment. The cement that is produced may or may not have the same chemical composition as the sediment. In sandstones, framework grains are often cemented by silica or carbonate. The extent of cementation is dependent on the composition of the sediment. For example, in lithic sandstones, cementation is less extensive because pore space between framework grains is filled with a muddy matrix that leaves little space for precipitation to occur. This is often the case for mudrocks as well. As a result of compaction, the clayey sediments comprising mudrocks are relatively impermeable.

Dissolution
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Dissolution of framework silicate grains and previously formed carbonate cement may occur during deep burial. Conditions that encourage this are essentially opposite of those required for cementation. Rock fragments and silicate minerals of low stability, such as plagioclase feldspar, pyroxenes, and amphiboles, may dissolve as a result of increasing burial temperatures and the presence of organic acids in pore waters. The dissolution of frame work grains and cements increases porosity particularly in sandstones.[3]

Mineral replacement
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This refers to the process whereby one mineral is dissolved and a new mineral fills the space via precipitation. Replacement can be partial or complete. Complete replacement destroys the identity of the original minerals or rock fragments giving a biased view of the original mineralogy of the rock.[3] Porosity can also be affected by this process. For example, clay minerals tend to fill up pore space and thereby reducing porosity.

Telogenesis

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In the process of burial, it is possible that siliciclastic deposits may subsequently be uplifted as a result of a mountain building event or erosion.[3] When uplift occurs, it exposes buried deposits to a radically new environment. Because the process brings material to or closer to the surface, sediments that undergo uplift are subjected to lower temperatures and pressures as well as slightly acidic rain water. Under these conditions, framework grains and cement are again subjected to dissolution and in turn increasing porosity. On the other hand, telogenesis can also change framework grains to clays, thus reducing porosity. These changes are dependent on the specific conditions that the rock is exposed as well as the composition of the rock and pore waters. Specific pore waters, can cause the further precipitation of carbonate or silica cements. This process can also encourage the process of oxidation on a variety of iron bearing minerals.

Sedimentary breccias

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Sedimentary breccias are a type of clastic sedimentary rock which are composed of angular to subangular, randomly oriented clasts of other sedimentary rocks. They may form either:

  1. In submarine debris flows, avalanches, mud flow or mass flow in an aqueous medium. Technically, turbidites are a form of debris flow deposit and are a fine-grained peripheral deposit to a sedimentary breccia flow.
  2. As angular, poorly sorted, very immature fragments of rocks in a finer grained groundmass which are produced by mass wasting. These are, in essence, lithified colluvium. Thick sequences of sedimentary (colluvial) breccias are generally formed next to fault scarps in grabens.

In the field, it may at times be difficult to distinguish between a debris flow sedimentary breccia and a colluvial breccia, especially if one is working entirely from drilling information. Sedimentary breccias are an integral host rock for many sedimentary exhalative deposits.

Igneous clastic rocks

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Basalt breccia, green groundmass is composed of epidote

Clastic igneous rocks include pyroclastic volcanic rocks such as tuff, agglomerate and intrusive breccias, as well as some marginal eutaxitic and taxitic intrusive morphologies. Igneous clastic rocks are broken by flow, injection or explosive disruption of solid or semi-solid igneous rocks or lavas.

Igneous clastic rocks can be divided into two classes:

  1. Broken, fragmental rocks produced by intrusive processes, usually associated with plutons or porphyry stocks
  2. Broken, fragmental rocks associated with volcanic eruptions, both of lava and pyroclastic type

Metamorphic clastic rocks

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Clastic metamorphic rocks include breccias formed in faults, as well as some protomylonite and pseudotachylite. Occasionally, metamorphic rocks can be brecciated via hydrothermal fluids, forming a hydrofracture breccia.

Hydrothermal clastic rocks

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Hydrothermal clastic rocks are generally restricted to those formed by hydrofracture, the process by which hydrothermal circulation cracks and brecciates the wall rocks and fills them in with veins. This is particularly prominent in epithermal ore deposits and is associated with alteration zones around many intrusive rocks, especially granites. Many skarn and greisen deposits are associated with hydrothermal breccias.

Impact breccias

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A fairly rare form of clastic rock may form during meteorite impact. This is composed primarily of ejecta; clasts of country rock, melted rock fragments, tektites (glass ejected from the impact crater) and exotic fragments, including fragments derived from the impactor itself.

Identifying a clastic rock as an impact breccia requires recognising shatter cones, tektites, spherulites, and the morphology of an impact crater, as well as potentially recognizing particular chemical and trace element signatures, especially osmiridium.

See also

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References

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Revisions and contributorsEdit on WikipediaRead on Wikipedia
from Grokipedia
Clastic rocks, also known as clastic sedimentary rocks, are a major category of sedimentary rocks formed from fragments of pre-existing rocks and minerals, termed clasts, that range in size from microscopic particles to boulders and are derived through mechanical weathering, , transportation, deposition, compaction, and cementation. These rocks constitute approximately 85-90% of all sedimentary rocks and are distinguished by their detrital texture, where discrete grains are bound together by natural cements such as silica, , or iron oxides. Unlike chemical or biochemical sedimentary rocks, clastic rocks originate primarily from physical breakdown processes rather than precipitation from solutions or biological activity. The formation of clastic rocks begins with the of source rocks, which produces clasts through physical (mechanical) and chemical processes, followed by transportation by agents like , , or that sort and round the particles based on , , and density. Upon deposition in basins such as rivers, lakes, or oceans, the sediments undergo , including compaction under the weight of overlying layers and cementation, which transforms loose into solid rock. This process preserves information about past environments, as and composition reflect the energy of the transporting medium and the proximity to the source area. Clastic rocks are classified primarily by grain size and composition, with the Wentworth scale defining categories from clay (<1/256 mm) to boulders (>256 mm). Fine-grained examples include and , formed from and clay; medium-grained sandstones consist of sand-sized , , or rock fragments; and coarse-grained conglomerates and breccias feature rounded or angular , respectively. Compositional classification uses the QFL diagram, analyzing proportions of (Q), (F), and lithic fragments (L) to infer and maturity, with quartz-rich rocks indicating extensive and transport. Clastic rocks play a crucial role in Earth's geological record, hosting fossils that document ancient and environments, serving as aquifers and reservoirs due to their and permeability, and providing insights into tectonic history through studies. Sedimentary rocks, of which clastic rocks form the majority, cover about 75% of the Earth's land surface and are essential for understanding evolution and resource exploration.

Overview

Definition and Formation

Clastic rocks are sedimentary rocks composed of fragments, known as clasts, derived from the mechanical breakdown of pre-existing rocks or minerals, which are subsequently transported, deposited, and lithified into solid rock. These rocks form through clastic , a process distinct from chemical or biogenic accumulation, as the clasts retain their original and texture from the source material to a significant degree. The formation of clastic rocks begins with weathering, where physical processes like frost action and thermal expansion, or chemical processes such as hydrolysis and oxidation, break down bedrock into loose fragments or ions. Erosion then removes these materials through agents including water, wind, ice, and gravity, initiating their transport. During transportation, clasts are sorted by size and shape—larger, denser particles settle first—while abrasion rounds angular fragments depending on distance traveled and medium velocity. Deposition occurs when the transporting energy diminishes, such as in river deltas, beaches, or deep ocean basins, allowing clasts to accumulate in layers. Finally, lithification transforms the sediment into rock through compaction, which expels water and reduces pore space, and cementation, where minerals like silica or calcite precipitate to bind the clasts. Clasts in clastic rocks originate from the of igneous, metamorphic, or sedimentary protoliths, with tectonic settings playing a crucial role by uplifting and exposing these source rocks to surface processes. For instance, in orogenic belts like mountain ranges, tectonic uplift accelerates , supplying abundant grains from weathered or other durable minerals. While bioclastic deposits, such as shell fragments, can contribute to certain clastic rocks, the primary focus here is on detrital clasts from lithic sources. classification, such as distinguishing from clay, further aids in interpreting these depositional environments, as detailed elsewhere.

Key Characteristics

Clastic rocks exhibit a fragmental texture composed of discrete mineral grains or rock fragments (clasts) that are mechanically transported, deposited, and subsequently cemented, distinguishing them from crystalline non-clastic rocks formed by precipitation or consolidation without discrete particles. This fragmental nature results in clast-supported fabrics, where larger grains touch each other with minimal matrix, or matrix-supported fabrics, where finer particles fill spaces between coarser clasts, influencing overall rock stability and fluid flow properties. Key textural attributes include sorting, which ranges from poor (mixed grain sizes, typical of high-energy, short-transport deposits like alluvial fans) to well-sorted (uniform sizes, as in aeolian dunes or beaches), reflecting the energy and duration of transport processes. Rounding varies from angular (indicating minimal transport, e.g., in breccias near source areas) to rounded (due to abrasion during prolonged transport by water or wind), while grain shape—often subangular to subspherical—further evolves with distance from the source, affecting packing density and porosity. Structural elements in clastic rocks primarily arise from depositional dynamics and include , manifest as horizontal layers defined by variations in grain size, color, or composition, which record episodic sediment accumulation. Cross-stratification appears as inclined internal layers within beds, formed by migrating bedforms such as dunes or ripples under unidirectional currents, serving as paleocurrent indicators. Grading, where fines upward (normal grading) or coarsens (inverse), signals rapid deposition from waning flows, such as in turbidites, and reflects fluctuating depositional energy. Porosity and permeability are governed by grain packing, sorting, and cementation, with well-sorted, rounded grains promoting higher intergranular pore space (up to 30-40% in uncemented sands) and better connectivity for fluid migration compared to poorly sorted equivalents. Distinguishing traits of clastic rocks include their detrital, non-crystalline matrix, often cemented by minerals like , , or iron oxides, in contrast to the interlocking crystals of igneous or metamorphic rocks. typically ranges from 2.2 to 2.8 g/cm³ for common clastics like sandstones, varying with composition (e.g., quartz-dominated at ~2.65 g/cm³) and compaction, while finer-grained mudrocks may approach 2.7 g/cm³ due to tighter packing. Mechanical strength is heterogeneous, with coarser, well-cemented clastics exhibiting higher compressive resistance than matrix-rich, fine-grained varieties, influenced by texture and diagenetic bonding. Diagnostic tests for identifying clastic rocks begin with hand-sample observations, where visible clasts, (using scales like Wentworth's, from clay <0.004 mm to boulders >256 mm), rounding, and like are assessed directly. For detailed analysis, thin-section microscopy under polarized light reveals grain boundaries, mineral identities (e.g., vs. ), matrix composition, and cement types, confirming the fragmental origin and distinguishing clastics from crystalline rocks.

Sedimentary Clastic Rocks

Composition of Siliciclastic Rocks

Siliciclastic rocks are primarily composed of detrital grains derived from the mechanical and of pre-existing rocks, with , , and lithic fragments forming the dominant framework grains. is the most stable and abundant framework grain, often comprising 65% or more of the total grains in mature sandstones due to its resistance to chemical . Feldspars, including K-feldspar (such as and ) and , range from 0% to over 25% of framework grains, reflecting less stable sources like granitic terrains, and are prone to alteration during transport or burial. Lithic fragments, or rock fragments from sedimentary, igneous, or metamorphic protoliths, vary widely in abundance (0-75%), acting as indicators of proximal or volcanic sources, with chert and fragments behaving similarly to in terms of durability. The matrix in siliciclastic rocks consists of fine-grained detrital material, primarily clay minerals such as and , which often form through the alteration of and lithic grains during . These clays typically constitute less than 30% of the rock volume in well-sorted arenites but can exceed 15% in matrix-rich varieties, filling interstices and influencing . Cements, precipitated during burial, include silica (as quartz overgrowths) and , which bind the framework and matrix, with silica being prevalent in -rich rocks. Chemically, siliciclastic rocks are dominated by SiO₂, which ranges from over 95% in quartz arenites to 50-70% in more aluminous varieties like graywackes, with Al₂O₃ and minor oxides (e.g., Fe₂O₃, K₂O) reflecting the of the grains and matrix. Provenance of siliciclastic rocks is interpreted using the QFL ternary diagram, which plots the relative proportions of quartz (Q), feldspar (F), and lithics (L) to infer source terranes; for instance, high quartz content (>90%) indicates derivation from stable cratonic interiors with intense recycling. Compositional variations define key subtypes: quartz arenites are nearly monomineralic (>90% quartz) with minimal matrix, signifying long transport and sorting; arkoses are feldspar-rich (>25% F) with subordinate quartz and lithics, pointing to rapid erosion of granitic sources; and graywackes feature abundant lithics (<75% Q) and matrix, derived from tectonically active margins. Accessory heavy minerals, such as zircon, occur in trace amounts (<1%) and enable geochronological dating of provenance. These components collectively determine the rock's stability, with quartz enhancing durability while feldspars and clays reduce it through susceptibility to further alteration.

Classification of Siliciclastic Rocks

Siliciclastic rocks are primarily classified based on grain size, which provides insights into depositional processes and energy conditions. The standard grain size scale for these sediments is the Udden-Wentworth classification, adapted from Wentworth's original geometric progression for clastic materials. This scale delineates categories from coarse gravel to fine clay, enabling consistent description across sedimentary contexts. The Wentworth scale for siliciclastic sediments is summarized in the following table:
CategorySubcategoryGrain Diameter (mm)
GravelBoulder>256
Cobble64–256
4–64
Granule2–4
Very coarse1–2
Coarse0.5–1
Medium0.25–0.5
Fine0.125–0.25
Very fine0.0625–0.125
-0.0039–0.0625
Clay-<0.0039
Rock types are named according to dominant grain size fractions, with gravel-sized (>2 mm) deposits forming conglomerates (rounded clasts) or breccias (angular clasts), sand-sized (0.0625–2 mm) forming sandstones, and finer fractions (<0.0625 mm) yielding siltstones or mudstones/shales. Textural maturity further refines this by assessing sorting and roundness, progressing from immature (poorly sorted, angular grains with matrix) through submature and mature stages to supermature (well-sorted, rounded grains with minimal matrix), reflecting prolonged transport and weathering. Compositional classification integrates mineralogy via schemes like Dott's QFL ternary diagram, which plots quartz (Q), feldspar (F), and lithic fragments (L) to categorize sandstones as quartzose (high Q, stable, recycled), arkosic (feldspar-rich, near-source), or lithic (rock fragment-dominated, volcanic/tectonic ). These categories distinguish arenites (matrix <15%) from wackes (matrix >15%), aiding analysis. and texture also inform environmental interpretations; for instance, coarse, rounded conglomerates often indicate high-energy fluvial or alluvial settings, while fine, well-laminated shales suggest low-energy marine or lacustrine environments. Modern classifications incorporate techniques to quantify sorting and roundness more objectively, using automated analysis of thin sections or photos to enhance precision in heterogeneous samples. Additionally, seismic integrates these textural attributes with geophysical data for prediction, identifying sequence boundaries and variations in subsurface siliciclastic units.

Diagenesis of Siliciclastic Rocks

Diagenesis refers to the suite of physical, chemical, and biological processes that transform siliciclastic sediments into rocks after deposition, primarily through , fluid interactions, and uplift, without reaching metamorphic conditions. These processes significantly alter the initial composition of siliciclastic rocks, which are dominated by , , and rock fragments, leading to changes in , permeability, and mechanical properties. In siliciclastic systems, is divided into three main stages—eogenesis, mesogenesis, and telogenesis—each governed by distinct depth, temperature, and fluid conditions. Eogenesis occurs in shallow burial depths of less than 1 km, where temperatures range from 10–70°C and pore waters are influenced by depositional or meteoric environments. Key processes include mechanical compaction, which reduces initial from 40–60% through grain rearrangement, and early cementation by minerals such as , , or iron oxides, often forming up to 40% of the rock volume. Dissolution may also begin here, particularly of unstable grains like volcanic fragments, while microbial activity plays a role in promoting authigenic clay formation (e.g., ) and early precipitation, as evidenced by bacterial mediation in near-surface reactions. Recent studies highlight how microbial communities in eogenesis enhance biostabilization and influence initial preservation in tidal and fluvial settings. Mesogenesis takes place during deeper burial (1–5 km), with temperatures of 70–150°C and increasing pressure, transitioning to connate or evolved basinal fluids. Dominant processes are chemical compaction via pressure solution at grain contacts, which further reduces porosity to 10–20%, and albitization of plagioclase feldspars, converting them to more stable albite through sodium-rich fluid interactions. Cementation intensifies with quartz overgrowths on detrital grains (requiring >70–80°C) and authigenesis of clays like illite or chlorite, which can coat grains and inhibit further cementation while reducing permeability. Feldspar dissolution also contributes to secondary porosity creation, though often counteracted by ongoing cementation. Telogenesis occurs upon uplift and exposure to near-surface conditions, typically involving meteoric waters that are oxidizing and CO₂-saturated, leading to acidic dissolution of earlier cements and grains. This stage enhances secondary through and removal, potentially increasing permeability in exhumed , while may oxidize iron-bearing phases. Unlike earlier stages, telogenesis is limited in depth (meters to tens of meters) but can significantly modify reservoir quality. Influencing factors across stages include and , which drive reaction kinetics; fluid chemistry, contrasting meteoric (low , acidic) with connate waters (high , reducing); and initial sediment composition, where quartz-rich sands resist alteration more than - or lithic-rich ones. evolution in siliciclastic rocks follows models of with depth, expressed as φ = φ₀ e^{-cz} (where φ is , φ₀ is initial , c is a rate constant, and z is depth), reflecting progressive compaction and cementation, though secondary can deviate from this trend. Recent research post-2020 emphasizes external influences on , such as CO₂ sequestration in siliciclastic reservoirs, where injected CO₂ promotes dissolution, enhancing secondary but risking mechanical instability through weakened grain frameworks. These insights underscore the dynamic nature of diagenetic evolution in response to modern geoengineering applications.

Sedimentary Breccias

Sedimentary breccias are coarse-grained clastic sedimentary rocks composed predominantly of angular clasts larger than 2 mm in , embedded in a finer-grained matrix of , , or clay, and characterized by poor sorting. These rocks form through the fragmentation and rapid deposition of pre-existing materials, preserving the angularity of clasts due to minimal and abrasion. Subtypes include fault breccias, which develop along tectonic faults from the grinding and fracturing of during movement; collapse breccias, resulting from the dissolution and gravitational of soluble rocks in or cave systems, often producing vuggy textures; and intraformational breccias, formed by the reworking of unlithified or semi-lithified sediments, such as mud cracks or intraclasts within the same depositional layer. Formation occurs in high-energy depositional environments where physical breakage dominates over processes, such as alluvial fans at the base of steep slopes, where flash floods deposit debris with little sorting; reef margins, where wave action shatters corals and shells; or submarine flows, involving that generates angular fragments. The angular clasts indicate short transport distances, often less than a few kilometers, preventing significant abrasion by water or wind. Unlike finer siliciclastics, is typically absent or chaotic due to the high-energy, episodic nature of deposition. Key characteristics include a heterogeneous texture with clast-supported or matrix-supported fabrics, where the matrix often comprises 20-50% of the rock volume and may undergo diagenetic cementation similar to other siliciclastics. Sedimentary breccias differ from conglomerates primarily in clast shape—angular versus rounded—reflecting higher and shorter compared to the fluvial or settings that round . Their internal heterogeneity, with interconnected pores and fractures, makes them significant in reservoirs, acting as traps where permeability contrasts seal oil and gas accumulations, as seen in buildups. Representative examples include the Wapsipinicon Breccias in , featuring reef-rock and island-rock types from coral debris accumulation.

Non-Sedimentary Clastic Rocks

Igneous Clastic Rocks

Igneous clastic rocks, specifically pyroclastic rocks, are fragmental deposits formed directly from explosive volcanic eruptions, consisting of —airborne volcanic that solidify upon deposition. These rocks arise from the fragmentation of during violent eruptions, contrasting with sedimentary clastics by their primary igneous origin without significant or wind transport. Common types include , formed from ash-sized particles (<2 mm); lapilli tuff, incorporating lapilli (2–64 mm); and ignimbrite, a welded resulting from hot ash flows. Pyroclastic rocks are classified based on fragment size and depositional style, with blocks (>64 mm) and bombs (rounded >64 mm) also present in coarser variants. Formation begins with rapid decompression and gas expansion within ascending , shattering it into pyroclasts during explosive events. These fragments are then transported via pyroclastic flows—dense, ground-hugging avalanches of hot gas, ash, and —or surges, which are dilute, turbulent currents, or simply fallout from eruption columns. Upon landing, hot deposits (>600°C) may undergo welding, where glass particles soften and fuse under load, leading to compaction and fiamme structures in . Cooling induces , converting to phases, while extreme heat in some ignimbrites promotes rheomorphic flow—ductile deformation resembling lava—resulting in and lineation. Compositionally, pyroclastic rocks comprise glass shards (vitric components from quenched ), crystals such as and (derived from the magma's cargo), and lithic fragments (accidental rock pieces from the conduit or vent). Classification often uses the relative abundance of these components—vitric, , and lithic—alongside fragment size and degree, ranging from non-welded (loose ) to densely welded or rheomorphic (highly deformed). In to intermediate compositions, and dominate crystals, while rhyolitic variants emphasize and sanidine. Notable examples include the ash-fall deposits burying Pompeii during the AD 79 eruption of , comprising layered from surge and fallout phases. Ignimbrites like those from the illustrate welded pyroclastic flows covering vast areas. Submarine volcaniclastic rocks, often overlooked in terrestrial-focused studies, form through explosive eruptions or resedimentation of subaerial ejecta, as revealed by Ocean Drilling Program cores showing ash layers and debris flows near volcanic arcs.

Metamorphic Clastic Rocks

Metamorphic clastic rocks, such as mylonites, cataclasites, and , form in fault zones where pre-existing rock fragments or grains are intensely deformed into a fine-grained, often foliated matrix under high strain conditions. Mylonites are defined as cohesive, foliated fault rocks characterized by dynamic recrystallization and a fine-grained matrix typically comprising 50-90% of the rock volume, with clasts appearing as strained porphyroclasts or lithic fragments. Cataclasites, in contrast, are cohesive, granular rocks produced by brittle fragmentation, featuring angular clasts of varying sizes embedded in a matrix of crushed material, typically lacking strong . Protomylonites represent an early stage, with 10-50% matrix but retaining more coarser, less recrystallized grains from the , marking the onset of significant ductile strain localization. These rocks derive from initial clasts of sedimentary or igneous origin that undergo solid-state transformation during tectonic activity. The formation of these rocks occurs primarily through tectonic deformation in fault zones, involving either ductile or brittle mechanisms that reduce grain size and develop porphyroclasts—resistant grains or fragments surrounded by finer matrix material. Mylonites develop via ductile processes, such as dynamic recrystallization, where minerals like quartz and feldspar flow and reorganize under elevated temperatures and pressures, typically at depths greater than 10 km, leading to pronounced foliation and lineation. Cataclasites form through brittle grinding and comminution during seismic or aseismic slip, often overprinting mylonites as fault zones are exhumed to shallower crustal levels, resulting in angular clasts and a cataclastic texture without extensive recrystallization. Grain size reduction is a key process in both, driven by cataclasis in brittle regimes and dislocation creep in ductile ones, with porphyroclasts forming as stronger minerals, such as feldspar, resist deformation while the surrounding matrix fines. Key characteristics include distinctive fabrics and mineralogical alterations that reflect deformation intensity and sense of shear. S-C fabrics, consisting of schistosity (S) planes subparallel to the shear zone boundary and shear (C) planes at a low angle to the foliation, are common in mylonites and indicate non-coaxial strain, with the angle between S and C planes decreasing with increasing shear strain. Augen structures, or eye-shaped porphyroclasts with tails of recrystallized matrix, develop in moderately strained mylonites, particularly in granitic protoliths, providing kinematic indicators of shear direction. Mineral changes, such as the transformation of quartz into myrmekitic intergrowths with plagioclase, occur during deformation, where alkali feldspar breakdown produces fine-grained plagioclase-quartz aggregates that weaken the rock and localize strain. Classification follows the Sibson scheme, which distinguishes fault rocks by deformation style and matrix proportion: for foliated (ductile) types, protomylonites (10-50% matrix), mylonites (50-90% matrix), and ultramylonites (>90% matrix); for non-foliated (brittle) cataclasites, a similar progression applies with protocataclasites (10-50% matrix), cataclasites (50-90% matrix), and ultracataclasites (>90% matrix). Prominent examples include mylonites from the zone in , where ductile shear zones at depth exhibit fine-grained quartz-feldspar matrices with porphyroclastic fabrics, transitioning upward to cataclasites in seismic slip zones. Recent studies highlight how these mylonites in the San Andreas accommodate long-term plate motion through distributed ductile strain, with overprinted cataclasites recording episodic seismic events and strain localization in principal slip zones. Such features underscore the role of metamorphic clastic rocks in facilitating fault evolution from ductile to brittle regimes during tectonic exhumation.

Hydrothermal Clastic Rocks

Hydrothermal clastic rocks, primarily manifested as hydrothermal breccias, form through the fracturing of host rocks induced by elevated fluid pressures within hydrothermal systems, resulting in angular rock fragments (clasts) suspended in a mineralized matrix. These breccias arise in mineralized environments where overpressurized fluids, often derived from magmatic sources, exploit pre-existing fractures or create new ones, leading to brittle failure and clast generation. Unlike sedimentary clastics, the transport distance is minimal, preserving the angularity and proximity of fragments to their source. The formation of hydrothermal breccias typically involves mechanisms such as fluid boiling, , or seismic pumping, which generate sudden pressure drops and explosive fracturing in systems. In these processes, hydrothermal fluids infiltrate and weaken the host rock, culminating in hydraulic fracturing that dislodges clasts; subsequent fluid flow suspends and deposits these fragments, often with limited sorting due to the rapid, localized nature of the event. The matrix and cementation occur via of minerals like , sulfides (e.g., , ), and carbonates from the cooling fluids, binding the clasts in place. This results in a clastic texture where the matrix is dominantly hydrothermal in origin, distinguishing these rocks from purely mechanical breccias. Key types of hydrothermal clastic rocks include magmatic-hydrothermal breccias, commonly associated with porphyry copper deposits, and those formed by seawater-basalt interactions in ophiolite sequences linked to volcanogenic massive sulfide (VMS) systems. Magmatic-hydrothermal breccias develop in shallow crustal settings where volatile-rich magmas devolatilize, driving fluid overpressure and brecciation pipes or veins; for instance, in the Copper Creek district, , these breccias host high-grade Cu-Mo-Ag mineralization within angular wall-rock clasts cemented by quartz and . In VMS environments, such as the Semenov-3 hydrothermal field in the , breccias form from the and resedimentation of sulfide mounds by vigorous hydrothermal venting, incorporating fragments in a sulfide-rich matrix. Characteristic features of these rocks include jigsaw-fit clasts, where fragments interlock as if minimally displaced, and milled textures from repeated fluid-induced grinding, often evident in porphyry systems. In magmatic-hydrothermal examples, clasts are typically angular to subangular, reflecting the host lithologies like or , with pipes extending hundreds of meters vertically. VMS-related breccias exhibit chaotic fabrics with sulfide clasts and , formed under conditions where seawater mixing promotes rapid precipitation. These textures highlight the role of in clast support and matrix infill. Economically, hydrothermal clastic rocks are significant hosts for deposits, particularly and , as the brecciation enhances permeability for fluid focusing and mineralization. In porphyry systems like Randu Kuning, , these breccias contain stockwork veins of Cu-Au sulfides, contributing substantially to global production. Similarly, VMS breccias in ophiolites, such as those in ancient seafloor settings, enrich , , and concentrations, with modern analogs informing exploration for seafloor resources. Their association with high-grade zones underscores their value in genesis models.

Impact Breccias

Impact breccias are clastic rocks formed exclusively by hypervelocity impacts on planetary surfaces, consisting of fragmented target rocks ejected and redeposited during crater formation. These breccias include two primary types: , a polymict breccia with clastic matrix containing shocked and lithic clasts alongside impact melt particles or glassy bodies (typically 5-15 vol%), and lithic breccia, which lacks melt components and comprises only rock and fragments in a clastic matrix. The clasts are derived from the disrupted target lithologies, often mixed with varying amounts of impact-generated melt that quenches into upon cooling. Formation begins with the propagation of shock waves exceeding 5 GPa from the hypervelocity impact, which induce intense fracturing, , and localized of target rocks within the transient . During the excavation stage, these materials are ejected ballistically or flow outward, forming fallback breccias inside the and layers beyond; subsequent crater modification involves , mixing clasts with molten components that solidify into a glassy matrix as temperatures drop. This process distinguishes impact breccias from other clastic rocks by the unique shock pressures involved, often reaching 10-100 GPa, far beyond typical geological mechanisms. Characteristic features include shatter cones, striated conical fractures formed at 2-6 GPa in subcrater rocks, and planar deformation features (PDFs) in and grains, manifesting as sets of parallel lamellae at 10-30 GPa. High-pressure polymorphs such as and stishovite, stable forms of silica under 2-10 GPa and >10 GPa respectively, occur as inclusions or veins in clasts, serving as definitive impact indicators. hinges on melt content: clastic (lithic) breccias with <5% melt, suevites with 5-50% melt fragments, and melt breccias with >50% matrix melt transitioning to impact melt rocks. Prominent examples include the suevite at Ries Crater, Germany (15 Ma, 24 km diameter), where polymict breccias with shocked quartz and coesite overlie the Bunte Breccia ejecta layer, illustrating fallback and ejecta deposition. At Chicxulub Crater, Mexico (66 Ma, ~200 km diameter), drill cores reveal ~130 m of polymict suevite with altered impact melt clasts and shocked basement fragments, deposited rapidly post-impact. Recent planetary science from the Perseverance rover in Jezero Crater, Mars, identifies analogous breccia outcrops on the rim, featuring fragmented pale pebbles indicative of ancient impact disruption and cementation, enhancing understanding of extraterrestrial clastic processes.

References

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