Exhumation (geology)

Last updated

In geology, the term exhumation refers to the process by which a parcel of rock (that was formerly buried), approaches Earth's surface. [1]

Contents

It differs from the related ideas of rock uplift and surface uplift in that it is explicitly measured relative to the surface of the Earth, rather than with reference to some absolute reference frame, such as the Earth's geoid. [1]

Exhumation of buried rocks should be considered as two different categories namely, exhumation by denudation/erosion or exhumation by tectonic processes followed by erosion. In the latter case, rocks (or rock packages) from deeper crustal levels (meter to kilometer depths below the Earth's surface) are brought towards the Earth's surface (i.e.shallower crustal levels) by crustal thickening (see compared also tectonic uplift) and/or extensional tectonics and are subsequently exposed by erosion. Often exhumation involves a complex interaction between crustal thickening, extensional tectonics and erosion.

Notably, there are overlapping characteristics between the different modes of burial and exhumation and distinction and between them relies on a series of parameters such as: [2]

Detailed and integrated geologic modelling, structural geology, geochronology and metamorphic geological disciplines are key to understanding these processes.

Denudation

Exhumation through denudation could be considered as the process of exposing rock packages solely through the removal of their overlying unconsolidated sediments or solid rock layers. Denudation is here considered as a process that removes parts of the Earth's upper crust by physical processes that occur naturally (e.g. glaciers, wind, water, landslides). Through this form of exhumation, something previously buried in sediments, for example a landform, is uncovered and can be exposed.

Exhumation by tectonic processes

Exhumation by tectonic processes refers to any geological mechanism that brings rocks from deeper crustal levels to shallower crustal levels. While erosion or denudation is fundamental in eventually exposing these deeper rocks at the Earth's surface, the geological phenomenon that drive the rocks to shallower crust are still considered exhumation processes. Geological exhumation occurs on a range of scales, from smaller-scale thrusts typically occurring within the shallow crust (less than ca. 10 km deep) [3] which results in exhumation in the order of centimeters to meters scales, to larger-scale features originating at deeper crustal levels along which, exhumation is in the order of hundreds of meters to kilometers.

The geological mechanisms that drive deep crustal exhumation can occur in a variety of tectonic settings but are ultimately driven by the convergence of tectonic plates through subduction. Depending on the type of convergent boundary, exhumation occurs by thrusting in the accretionary wedge, by obduction and/or as a process during the orogenic cycle (i.e. mountain building and collapse cycle).

Obduction

During the subduction of an oceanic plate underneath the continental crust, some fragments of the oceanic crust can be trapped above the continental crust through obduction. The resulting rocks obducted on the continental crust are called ophiolites. [4]   While the exact mechanism behind the formation of ophiolites is still up for debate, [4] those rocks still show an example of rocks being exhumed and exposed at the surface by the tectonic process of obduction and then exposed.

Exhumation of the deep crust during an orogenic cycle.

Exhumation of deep crustal rocks during an orogenic cycle occurs mainly during continental collision or during post-collision extension [2] and is thus, is broadly grouped into the three mechanisms which are used to describe the burial and exhumation of the cycle namely, syn-convergent orogenic wedges, [5] [6] channel flow (also known as ductile extrusion) [7] and post-convergence gravitational collapse.

Syn-convergent orogenic wedge

During the subduction to the collisional phases of the orogenic cycle, a tectonic wedge forms on the prowedge (side of the subducting plate) and commonly the retrowedge (continental side) of the orogen. During the continued convergence, the wedge maintains its shape by maintaining its critical angle of taper [6] [5] by the interaction of thickening through basal accretion or foreland propagation (frontal accretion) and thinning through normal faulting and erosion at the upper part of the wedge. Erosion of the wedge significantly impacts the dynamics within the wedge, which promotes exhumation by thrusting mid-crustal rocks to the hanging wall of the wedge. [8] [9] Characteristics of this mode of exhumation include, evidence for strong non coaxial reverse-shearing, pro-grade metamorphism, cooling ages are progressively younger towards deeper structural levels and that exhumation at higher structural levels is coeval to burial of the structural levels. [2] Tectonics of this kind result in fold and thrust belts or if they are built up over long periods, can form thick-stacked long-hot-orogens, [7] such as the Himalayas.

Channel-flow

Channel flow typically occurs in long-hot orogens when the orogen is sufficiently thick to promote partial melting in the middle-lower part of the orogen to a point where the rocks reach a critically low viscosity enabling them to flow. [7] [10] [11] Subsequently these rocks can decoupled from their base and begin to flow to higher crustal levels along lithostatic pressure gradients that can be caused by melt-induced buoyancy or differences in topography and lateral density contrasts. [12] both of which are affected by erosion. [13] Characteristics of this mode of exhumation include simultaneous normal shearing and reverse shearing along the roof and the base of the channel respectively, high-temperature retrograde metamorphic assemblages, cooing ages should be younger to the front of the channel and P-T-t paths suggesting prolonged burial and synchronous exhumation throughout the channel. [2]

Post-convergent gravitational collapse

Post-convergent gravitational collapse (extension) occurs once the convergence forces can no longer support the gravitational force of the orogen that was built up during collision.[ citation needed ] During collapse, high-grade rocks from the core of the orogen are exhumed through upward flow towards now thinned crustal areas forming domal shaped metamorphic core complexes. [14] [15] Alternatively, or in conjunction with the extension of the center of the orogen, propagation of the rock-mass towards the margin may lead to exhumation along a series of brittle or ductile thrusts and normal faults [11] and ultimately the formation of fold and thrust type belts along the margins of the collapsed orogen. Characteristics of gravitational collapse include outward verging, normal sense shear zones along the margins of the core complexes and exhumation-only type P-T-t paths. [2]

Related Research Articles

Orogeny The formation of mountain ranges

Orogeny is the primary mechanism by which mountains are formed on continents. An orogeny is an event that takes place at a convergent plate margin when plate motion compresses the margin. This leads to both structural deformation and compositional differentiation of the Earth's lithosphere. An orogenic belt or orogen develops as the compressed plate crumples and is uplifted to form one or more mountain ranges; this involves a series of geological processes collectively called orogenesis. A synorogenic process or event is one that occurs during an orogeny.

Convergent boundary Region of active deformation between colliding tectonic plates

A convergent boundary is an area on Earth where two or more lithospheric plates collide. One plate eventually slides beneath the other, a process known as subduction. The subduction zone can be defined by a plane where many earthquakes occur, called the Wadati–Benioff zone. These collisions happen on scales of millions to tens of millions of years and can lead to volcanism, earthquakes, orogenesis, destruction of lithosphere, and deformation. Convergent boundaries occur between oceanic-oceanic lithosphere, oceanic-continental lithosphere, and continental-continental lithosphere. The geologic features related to convergent boundaries vary depending on crust types.

Forearc The region between an oceanic trench and the associated volcanic arc

A forearc is the region between an oceanic trench and the associated volcanic arc. Forearc regions are found at convergent margins, and include any accretionary wedge and forearc basin that may be present. Due to tectonic stresses as one tectonic plate rides over another, forearc regions are sources for great thrust earthquakes.

Tectonic uplift is the geologic uplift of Earth's surface that is attributed to plate tectonics. While isostatic response is important, an increase in the mean elevation of a region can only occur in response to tectonic processes of crustal thickening, changes in the density distribution of the crust and underlying mantle, and flexural support due to the bending of rigid lithosphere.

Geology of the Himalaya Origins and structure of the mountain range

The geology of the Himalayas is a record of the most dramatic and visible creations of the immense mountain range formed by plate tectonic forces and sculpted by weathering and erosion. The Himalayas, which stretch over 2400 km between the Namcha Barwa syntaxis in Tibet and the Nanga Parbat syntaxis in Kashmir, are the result of an ongoing orogeny — the collision of the continental crust of two tectonic plates namely the Indian Plate thrusting into the Eurasian Plate. The Himalaya-Tibet region supplies fresh water for more than one-fifth of the world population, and accounts for a quarter of the global sedimentary budget. Topographically, the belt has many superlatives: the highest rate of uplift, the highest relief, among the highest erosion rates at 2–12 mm/yr, the source of some of the greatest rivers and the highest concentration of glaciers outside of the polar regions. This last feature earned the Himalaya its name, originating from the Sanskrit for "the abode of the snow".

Continental collision Phenomenon in which mountains are produced on the boundaries of converging tectonic plates

In geology, continental collision is a phenomenon of plate tectonics that occurs at convergent boundaries. Continental collision is a variation on the fundamental process of subduction, whereby the subduction zone is destroyed, mountains produced, and two continents sutured together. Continental collision is only known to occur on Earth.

Grenville orogeny

The Grenville orogeny was a long-lived Mesoproterozoic mountain-building event associated with the assembly of the supercontinent Rodinia. Its record is a prominent orogenic belt which spans a significant portion of the North American continent, from Labrador to Mexico, as well as to Scotland.

Anatexis is the partial melting of rocks. Traditionally, anatexis is used specifically to discuss the partial melting of crustal rocks, while the generic term "partial melting" refers to the partial melting of all rocks, in both the crust and mantle.

Décollement

Décollement is a gliding plane between two rock masses, also known as a basal detachment fault. Décollements are a deformational structure, resulting in independent styles of deformation in the rocks above and below the fault. They are associated with both compressional settings and extensional settings.

Erosion and tectonics

The interaction between erosion and tectonics has been a topic of debate since the early 1990s. While the tectonic effects on surface processes such as erosion have long been recognized, the opposite has only recently been addressed. The primary questions surrounding this topic are what types of interactions exist between erosion and tectonics and what are the implications of these interactions. While this is still a matter of debate, one thing is clear, the Earth's landscape is a product of two factors: tectonics, which can create topography and maintain relief through surface and rock uplift, and climate, which mediates the erosional processes that wear away upland areas over time. The interaction of these processes can form, modify, or destroy geomorphic features on the Earth's surface.

A river anticline is a geologic structure that is formed by the focused uplift of rock caused by high erosion rates from large rivers relative to the surrounding areas. An anticline is a fold that is concave down, whose limbs are dipping away from its axis, and whose oldest units are in the middle of the fold. These features form in a number of structural settings. In the case of river anticlines, they form due to high erosion rates, usually in orogenic settings. In a mountain building setting, like that of the Himalaya or the Andes, erosion rates are high and the river anticline's fold axis will trend parallel to a major river. When river anticlines form, they have a zone of uplift between 50-80 kilometers wide along the rivers that form them.

Ultra-high-pressure metamorphism refers to metamorphic processes at pressures high enough to stabilize coesite, the high-pressure polymorph of SiO2. It is important because the processes that form and exhume ultra-high-pressure (UHP) metamorphic rocks may strongly affect plate tectonics, the composition and evolution of Earth's crust. The discovery of UHP metamorphic rocks in 1984 revolutionized our understanding of plate tectonics. Prior to 1984 there was little suspicion that continental rocks could reach such high pressures.

Pre-collisional Himalaya

Pre-collisional Himalaya is the arrangement of the Himalayan rock units before mountain-building processes resulted in the collision of Asia and India. The collision began in the Cenozoic and it is a type locality of a continental-continental collision. The reconstruction of the initial configuration of the rock units and the relationship between them is highly controversial, and major concerns relate to the arrangements of the different rock units in three dimensions. Several models have been advanced to explain the possible arrangements and petrogenesis of the rock units.

Huangling Complex

Huangling Complex represents a group of rock units appear in the middle of Yangtze Block in South China, distributed across Yixingshan, Zigui, Huangling and Yichang counties. The group of rock involves nonconformity that sedimentary rocks overlie the metamorphic basement. It is a 73-km long, asymmetrical dome-shaped anticline with axial plane orientating in north-south direction. It has a steeper west flank and a gentler east flank. Basically, there are three tectonic units from the anticline core to the rim, including Archean to Paleoproterozoic metamorphic basement, Neoproterozoic to Jurassic sedimentary rocks and Cretaceous fluvial deposit sedimentary cover. The northern part of the core is mainly tonalite-trondhjemite-gneiss (TTG) and Cretaceous sedimentary rock, it is called the Archean Kongling Complex. The middle of the core is mainly the Neoproterozoic granitoid. The southern part of the core is the Neoproterozoic potassium granite. Two basins are situated on the western and eastern flanks of the core respectively, including the Zigui basin and Dangyang basin. Both basins are synforms while Zigui basin has a larger extent of folding. Yuanan Graben and Jingmen Graben are found within Dangyang Basin area. Huangling Complex is an important area that helps unravel the tectonic history of South China Craton because it has well-exposed layers of rock units from Archean basement rock to Cretaceous sedimentary rock cover due to the erosion of the anticline.

Scandinavian Caledonides

The Scandinavian Caledonides are the vestiges of an ancient, today deeply eroded orogenic belt formed during the Silurian–Devonian continental collision of Baltica and Laurentia, which is referred to as the Scandian phase of the Caledonian orogeny. The size of the Scandinavian Caledonides at the time of their formation can be compared with the size of the Himalayas. The area east of the Scandinavian Caledonides, including parts of Finland, developed into a foreland basin where old rocks and surfaces were covered by sediments. Today, the Scandinavian Caledonides underlay most of the western and northern Scandinavian Peninsula, whereas other parts of the Caledonides can be traced into West and Central Europe as well as parts of Greenland and eastern North America.

Paleogeography of the India–Asia collision system Geological and geomorphological evolution of India and Asia

The paleogeography of the India–Asia collision system is the reconstructed geological and geomorphological evolution within the collision zone of the Himalayan orogenic belt. The continental collision between the Indian and Eurasian plate is one of the world's most renowned and most studied convergent systems. However, many mechanisms remain controversial. Some of the highly debated issues include the onset timing of continental collision, the time at which the Tibetan plateau reached its present elevation and how tectonic processes interacted with other geological mechanisms. These mechanisms are crucial for the understanding of Mesozoic and Cenezoic tectonic evolution, paleoclimate and paleontology, such as the interaction between the Himalayas orogenic growth and the Asian monsoon system, as well as the dispersal and speciation of fauna. Various hypotheses have been put forward to explain how the paleogeography of the collision system could have developed. Important ideas include the synchronous collision hypothesis, the Lhasa-plano hypothesis and the southward draining of major river systems.

South China Craton

The South China Craton or South China Block is one of the Precambrian continental blocks in China. It is traditionally divided into the Yangtze Block in the NW and the Cathaysia Block in the SE. The Jiangshan–Shaoxing Fault represents the suture boundary between the two sub-blocks. Recent study suggests that the South China Block possibly has one more sub-block which is named the Tolo Terrane. The oldest rocks in the South China Block occur within the Kongling Complex, which yields zircon U–Pb ages of 3.3–2.9 Ga.

The Superior Craton is a stable crustal block covering Quebec, Ontario, and southeast Manitoba in Canada, and northern Minnesota in the United States. It is the biggest craton among those formed during the Archean period. A craton is a large part of the Earth's crust that has been stable and subjected to very little geological changes over a long time. The size of Superior Craton is about 1,572,000 km2. The craton underwent a series of events from 4.3 to 2.57 Ga. These events included the growth, drifting and deformation of both oceanic and continental crusts.

Earth system interactions across mountain belts

Earth system interactions across mountain belts are interactions between processes occurring in the different systems or "spheres" of the Earth, as these influence and respond to each other through time. Earth system interactions involve processes occurring at the atomic to planetary scale which create linear and non-linear feedback(s) involving multiple Earth systems. This complexity makes modelling Earth system interactions difficult because it can be unclear how processes of different scales within the Earth interact to produce larger scale processes which collectively represent the dynamics of the Earth as an intricate interactive adaptive system.

Geology of Himachal Pradesh

The geology of Himachal Pradesh is dominated by Precambrian rocks that were assembled and deformed during the India-Asia collision and the subsequent Himalayan orogeny. The Northern Indian State Himachal Pradesh is located in the Western Himalaya. It has a rugged terrain, with elevation ranging from 320m to 6975m. Rock materials in the region are largely from the Indian craton, and their ages range from the Paleoproterozoic to the present day. It is generally agreed that the Indian craton collided with Asia 50-60 million years ago (Ma). Rock sequences were thrust and folded immensely during the collision. The area has also been shaped by focused orographic precipitation, glaciation and rapid erosion.

References

  1. 1 2 England, Philip; Molnar, Peter (1990-12-01). "Surface uplift, uplift of rocks, and exhumation of rocks". Geology. 18 (12): 1173–1177. Bibcode:1990Geo....18.1173E. doi:10.1130/0091-7613(1990)018<1173:SUUORA>2.3.CO;2. ISSN   0091-7613.
  2. 1 2 3 4 5 Gervais, Félix; Brown, Richard L. (2011). "Testing modes of exhumation in collisional orogens: Synconvergent channel flow in the southeastern Canadian Cordillera". Lithosphere. 3 (1): 55–75. Bibcode:2011Lsphe...3...55G. doi: 10.1130/L98.1 .
  3. Sibson, R H (1986-05-01). "Earthquakes and Rock Deformation in Crustal Fault Zones". Annual Review of Earth and Planetary Sciences. 14 (1): 149–175. Bibcode:1986AREPS..14..149S. doi:10.1146/annurev.ea.14.050186.001053. ISSN   0084-6597.
  4. 1 2 Robinson, Paul T.; Malpas, John; Dilek, Yildirim; Zhou, Mei-fu (2008). "The significance of sheeted dike complexes in ophiolites". GSA Today. 18 (11): 4. doi: 10.1130/GSATG22A.1 . ISSN   1052-5173.
  5. 1 2 Dahlen, F A (1995). "Critical Taper Model of Fold-And-Thrust Belts and Accretionary Wedges". Annual Review of Earth and Planetary Sciences. 18 (1): 55–99. doi:10.1146/annurev.ea.18.050190.000415. ISSN   0084-6597. S2CID   128774151.
  6. 1 2 Platt, J. P. (1986). "Dynamics of orogenic wedges and the uplift of high-pressure metamorphic rocks". Geological Society of America Bulletin. 97 (9): 1037. Bibcode:1986GSAB...97.1037P. doi:10.1130/0016-7606(1986)97<1037:DOOWAT>2.0.CO;2. ISSN   0016-7606.
  7. 1 2 3 Beaumont, C.; Jamieson, R. A.; Nguyen, M. H.; Lee, B. (2001). "Himalayan tectonics explained by extrusion of a low-viscosity crustal channel coupled to focused surface denudation". Nature. 414 (6865): 738–742. Bibcode:2001Natur.414..738B. doi:10.1038/414738a. ISSN   0028-0836. PMID   11742396.
  8. Willett, Sean D. (1999). "Orogeny and orography: The effects of erosion on the structure of mountain belts". Journal of Geophysical Research: Solid Earth. 104 (B12): 28957–28981. Bibcode:1999JGR...10428957W. doi: 10.1029/1999JB900248 . ISSN   2156-2202.
  9. Willett, Sean D. (1999). "Rheological dependence of extension in wedge models of convergent orogens". Tectonophysics. 305 (4): 419–435. Bibcode:1999Tectp.305..419W. doi:10.1016/S0040-1951(99)00034-7.
  10. Grujic, D. (2006). "Channel flow and continental collision tectonics: an overview". Geological Society, London, Special Publications. 268 (1): 25–37. Bibcode:2006GSLSP.268...25G. doi:10.1144/GSL.SP.2006.268.01.02. ISSN   0305-8719.
  11. 1 2 Jamieson, R. A.; Beaumont, C. (2013-11-01). "On the origin of orogens". Geological Society of America Bulletin. 125 (11–12): 1671–1702. Bibcode:2013GSAB..125.1671J. doi:10.1130/B30855.1. ISSN   0016-7606.
  12. Gervais, Félix; Ranalli, Giorgio (2017). "The effects of lateral density gradients, slopes and buoyancy on channel flow: 1D analytical solutions and applications to the SE Canadian Cordillera". Tectonophysics. 712–713: 578–588. Bibcode:2017Tectp.712..578G. doi:10.1016/j.tecto.2017.06.023.
  13. Godin, L.; Grujic, D.; Law, R. D.; Searle, M. P. (2006). "Channel flow, ductile extrusion and exhumation in continental collision zones: an introduction". Geological Society, London, Special Publications. 268 (1): 1–23. Bibcode:2006GSLSP.268....1G. doi:10.1144/gsl.sp.2006.268.01.01. ISSN   0305-8719. S2CID   56520730.
  14. Brun, Jean-Pierre; Sokoutis, Dimitrios; Driessche, Jean Van Den (1994-04-01). "Analogue modeling of detachment fault systems and core complexes". Geology. 22 (4): 319–322. Bibcode:1994Geo....22..319B. doi:10.1130/0091-7613(1994)022<0319:AMODFS>2.3.CO;2. ISSN   0091-7613.
  15. Tirel, Céline; Brun, Jean-Pierre; Burov, Evgueni (2008). "Dynamics and structural development of metamorphic core complexes". Journal of Geophysical Research: Solid Earth. 113 (B4): B04403. Bibcode:2008JGRB..113.4403T. doi: 10.1029/2005JB003694 . ISSN   2156-2202.