Earth:Asthenosphere

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Short description: Highly viscous, mechanically weak, and ductile region of Earth's mantle
The asthenosphere shown at a subduction boundary

The asthenosphere (from grc ἀσθενός (asthenós) 'without strength') is the mechanically weak[1] and ductile region of the upper mantle of Earth. It lies below the lithosphere, at a depth between ~80 and 200 km (50 and 120 mi) below the surface, and extends as deep as 700 km (430 mi). However, the lower boundary of the asthenosphere is not well defined.

The asthenosphere is almost solid, but a slight amount of melting (less than 0.1% of the rock) contributes to its mechanical weakness. More extensive decompression melting of the asthenosphere takes place where it wells upwards, and this is the most important source of magma on Earth. It is the source of mid-ocean ridge basalt (MORB) and of some magmas that erupted above subduction zones or in regions of continental rifting.

Characteristics

The asthenosphere in relation to the other layers of Earth's structure

The asthenosphere is a part of the upper mantle just below the lithosphere that is involved in plate tectonic movement and isostatic adjustments. It is composed of peridotite, a rock containing mostly the minerals olivine and pyroxene.[2] The lithosphere-asthenosphere boundary is conventionally taken at the 1,300 °C (2,370 °F) isotherm. Below this temperature (closer to the surface) the mantle behaves rigidly; above this temperature (deeper below the surface) it acts in a ductile fashion.[3] The asthenosphere is where the mantle rock most closely approaches its melting point, and a small amount of melt is likely to present in this layer.[4]

Seismic waves pass relatively slowly through the asthenosphere[5] compared to the overlying lithospheric mantle. Thus, it has been called the low-velocity zone (LVZ), although the two are not strictly the same;[6][7] the lower boundary of the LVZ lies at a depth of 180 to 220 kilometers (110 to 140 mi),[8] whereas the base of the asthenosphere lies at a depth of about 700 kilometers (430 mi).[9] The LVZ also has a high seismic attenuation (seismic waves moving through the asthenosphere lose energy) and significant anisotropy (shear waves polarized vertically have a lower velocity than shear waves polarized horizontally).[10] The discovery of the LVZ alerted seismologists to the existence of the asthenosphere and gave some information about its physical properties, as the speed of seismic waves decreases with decreasing rigidity. This decrease in seismic wave velocity from the lithosphere to the asthenosphere could be caused by the presence of a very small percentage of melt in the asthenosphere, though since the asthenosphere transmits S waves, it cannot be fully melted.[4]

In the oceanic mantle, the transition from the lithosphere to the asthenosphere (the LAB) is shallower than for the continental mantle (about 60 km in some old oceanic regions) with a sharp and large velocity drop (5–10%).[11] At the mid-ocean ridges, the LAB rises to within a few kilometers of the ocean floor.

The upper part of the asthenosphere is believed to be the zone upon which the great rigid and brittle lithospheric plates of the Earth's crust move about. Due to the temperature and pressure conditions in the asthenosphere, rock becomes ductile, moving at rates of deformation measured in cm/yr over lineal distances eventually measuring thousands of kilometers. In this way, it flows like a convection current, radiating heat outward from the Earth's interior. Above the asthenosphere, at the same rate of deformation, rock behaves elastically and, being brittle, can break, causing faults. The rigid lithosphere is thought to "float" or move about on the slowly flowing asthenosphere, enabling isostatic equilibrium[12] and allowing the movement of tectonic plates.[13][14]

Boundaries

The asthenosphere extends from an upper boundary at approximately Lua error: not enough memory. below the surface[15][7] to a lower boundary at a depth of approximately Lua error: Internal error: The interpreter exited with status 1..Lua error: Internal error: The interpreter exited with status 1.Lua error: Internal error: The interpreter exited with status 1.

Lithosphere-asthenosphere boundary

The lithosphere-asthenosphere boundary (LAB[15][7]) is relatively sharp and likely coincides with the onset of partial melting or a change in composition or anisotropy.[16] Various definitions of the boundary reflect various aspects of the boundary region. In addition to the mechanical boundary defined by seismic data, which reflects the transition from the rigid lithosphere to ductile asthenosphere, these include a thermal boundary layer, above which heat is transported by thermal conduction and below which heat transfer is mainly convective; a rheological boundary, where the viscosity drops below about 1021 Pa-s; and a chemical boundary layer, above which the mantle rock is depleted in volatiles and enriched in magnesium relative to the rock below.[17]

Lower boundary of asthenosphere

The lower boundary of the asthenosphere is less well-defined, but has been placed at the base of the upper mantle.[18] This boundary is neither seismically sharp nor well understoodLua error: Internal error: The interpreter exited with status 1.Lua error: Internal error: The interpreter exited with status 1. but is approximately coincident with the complex 670 km discontinuity.[19] This discontinuity is generally linked to the transition from mantle rock containing ringwoodite to mantle rock containing bridgmanite and periclase.[20]

Origin

The mechanical properties of the asthenosphere are widely attributed to the partial melting of the rock.Lua error: Internal error: The interpreter exited with status 1.Lua error: Internal error: The interpreter exited with status 1. It is likely that a small amount of melt is present through much of the asthenosphere, where it is stabilized by the traces of volatiles (water and carbon dioxide) present in the mantle rock.Lua error: Internal error: The interpreter exited with status 1.Lua error: Internal error: The interpreter exited with status 1. However, the likely amount of melt, not more than about 0.1% of the rock, seems inadequate to fully explain the existence of the asthenosphere. This is not enough melt to fully wet grain boundaries in the rock, and the effects of melt on the mechanical properties of the rock are not expected to be significant if the grain boundaries are not fully wetted. The sharp lithosphere-asthenosphere boundary is also difficult to explain by partial melting alone.Lua error: Internal error: The interpreter exited with status 1.Lua error: Internal error: The interpreter exited with status 1. It is possible that melt accumulates at the top of the asthenosphere, where it is trapped by the impermeable rock of the lithosphere.Lua error: Internal error: The interpreter exited with status 1.Lua error: Internal error: The interpreter exited with status 1. Another possibility is that the asthenosphere is a zone of minimum water solubility in mantle minerals so that more water is available to form greater quantities of melt.[21] Another possible mechanism for producing mechanical weakness is grain boundary sliding, where grains slide slightly past each other under stress, lubricated by the traces of volatiles present.Lua error: Internal error: The interpreter exited with status 1.Lua error: Internal error: The interpreter exited with status 1.

Numerical models of mantle convection in which the viscosity is dependent both on temperature and strain rate reliably produce an oceanic asthenosphere, suggesting that strain-rate weakening is a significant contributing mechanism.[22]

Magma generation

Decompression melting of asthenospheric rock creeping towards the surface is the most important source of magma on Earth. Most of this erupts at mid-ocean ridges to form the distinctive mid-ocean ridge basalt (MORB) of the ocean crust.[23][24][25] Magmas are also generated by decompressional melting of the asthenosphere above subduction zones[26] and in areas of continental rifting.[27][28]

Decompression melting in upwelling asthenosphere likely begins at a depth as great as Lua error: Internal error: The interpreter exited with status 1., where the small amounts of volatiles in the mantle rock (about 100 ppm of water and 60 ppm of carbon dioxide) assist in melting not more than about 0.1% of the rock. At a depth of about Lua error: Internal error: The interpreter exited with status 1., dry melting conditions are reached and melting increases substantially. This dehydrates the remaining solid rock and is likely the origin of the chemically depleted lithosphere.Lua error: Internal error: The interpreter exited with status 1.Lua error: Internal error: The interpreter exited with status 1.Lua error: Internal error: The interpreter exited with status 1.Lua error: Internal error: The interpreter exited with status 1.

See also

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References

  1. ↑ Barrell, J. (1914). "The strength of the crust, Part VI. Relations of isostatic movements to a sphere of weakness – the asthenosphere". The Journal of Geology 22 (7): 655–83. doi:10.1086/622181. Bibcode: 1914JG.....22..655B. 
  2. ↑ Hirschmann 2010.
  3. ↑ Self, Steve; Rampino, Mike (2012). "The Crust and Lithosphere". Geological Society of London. http://www.geolsoc.org.uk/Education-and-Careers/Resources/Papers-and-Reports/Flood-basalts-mantle-plumes-and-mass-extinctions/The-Crust-and-Lithosphere. 
  4. ↑ 4.0 4.1 Kearey, Klepeis & Vine 2009, p. 49.
  5. ↑ Forsyth, Donald W. (1975). "The early structural evolution and anisotropy of the oceanic upper mantle". Geophysical Journal International 43 (1): 103–162. doi:10.1111/j.1365-246X.1975.tb00630.x. Bibcode: 1975GeoJ...43..103F. 
  6. ↑ Kearey, P., ed (1993). The Encyclopedia of the Solid Earth Sciences. Oxford: Blackwell Science. ISBN 978-1-4443-1388-8. OCLC 655917296. https://www.worldcat.org/oclc/655917296. 
  7. ↑ 7.0 7.1 7.2 Eppelbaum, Lev V.; Kutasov, I. M.; Pilchin, Arkady (2013). Applied Geothermics. Berlin. ISBN 978-3-642-34023-9. OCLC 879327163. https://www.worldcat.org/oclc/879327163. 
  8. ↑ Condie, Kent C. (1997). Plate Tectonics and Crustal Evolution. Butterworth-Heinemann. p. 123. ISBN 978-0-7506-3386-4. https://books.google.com/books?id=HZrA6OQzsvgC&pg=PA123. Retrieved 21 May 2010. 
  9. ↑ Kearey, Klepeis & Vine 2009, p. 51.
  10. ↑ Karato 2012.
  11. ↑ Rychert, Catherine A.; Shearer, Peter M. (2011). "Imaging the lithosphere-asthenosphere boundary beneath the Pacific using SS waveform modeling". Journal of Geophysical Research: Solid Earth 116 (B7): B07307. doi:10.1029/2010JB008070. Bibcode: 2011JGRB..116.7307R. 
  12. ↑ Kearey, Klepeis & Vine 2009, pp. 48–49.
  13. ↑ Hendrix, Mark; Thompson, Graham R.; Turk, Jonathan (2015). Earth (2nd ed.). Stamford, CT. ISBN 978-1-285-44226-6. OCLC 864788835. https://www.worldcat.org/oclc/864788835. 
  14. ↑ Garrison, Tom; Ellis, Robert (2017). Essentials of Oceanography (8th ed.). Pacific Grove. ISBN 978-1-337-51538-2. OCLC 1100670264. https://www.worldcat.org/oclc/1100670264. 
  15. ↑ 15.0 15.1 Gupta, Harsh K., ed (2011). Encyclopedia of Solid Earth Geophysics. Dordrecht: Springer. ISBN 978-90-481-8702-7. OCLC 745002805. https://www.worldcat.org/oclc/745002805. 
  16. ↑ Rychert, Catherine A.; Shearer, Peter M. (24 April 2009). "A Global View of the Lithosphere-Asthenosphere Boundary". Science 324 (5926): 495–498. doi:10.1126/science.1169754. PMID 19390041. Bibcode: 2009Sci...324..495R. 
  17. ↑ Artemieva, Irina (2011). The Lithosphere. pp. 6, 12. doi:10.1017/CBO9780511975417. ISBN 978-0-511-97541-7. 
  18. ↑ Anderson, Don L. (1995). "Lithosphere, asthenosphere, and perisphere" (in en). Reviews of Geophysics 33 (1): 125. doi:10.1029/94RG02785. ISSN 8755-1209. Bibcode: 1995RvGeo..33..125A. https://authors.library.caltech.edu/34732/. 
  19. ↑ Fowler, C. M. R.; Fowler, Connie May (2005). The Solid Earth: An Introduction to Global Geophysics. Cambridge University Press. ISBN 978-0521893077. 
  20. ↑ Ito, E; Takahashi, E (1989). "Postspinel transformations in the system Mg2SiO4-Fe2SiO4 and some geophysical implications". Journal of Geophysical Research: Solid Earth 94 (B8): 10637–10646. doi:10.1029/jb094ib08p10637. Bibcode: 1989JGR....9410637I. 
  21. ↑ Mierdel, Katrin; Keppler, Hans; Smyth, Joseph R.; Langenhorst, Falko (19 January 2007). "Water Solubility in Aluminous Orthopyroxene and the Origin of Earth's Asthenosphere". Science 315 (5810): 364–368. doi:10.1126/science.1135422. PMID 17234945. Bibcode: 2007Sci...315..364M. 
  22. ↑ Becker, Thorsten W. (November 2006). "On the effect of temperature and strain-rate dependent viscosity on global mantle flow, net rotation, and plate-driving forces". Geophysical Journal International 167 (2): 943–957. doi:10.1111/j.1365-246X.2006.03172.x. Bibcode: 2006GeoJI.167..943B. 
  23. ↑ Connolly, James A. D.; Schmidt, Max W.; Solferino, Giulio; Bagdassarov, Nikolai (November 2009). "Permeability of asthenospheric mantle and melt extraction rates at mid-ocean ridges". Nature 462 (7270): 209–212. doi:10.1038/nature08517. PMID 19907492. Bibcode: 2009Natur.462..209C. 
  24. ↑ Olive, Jean-Arthur; Dublanchet, Pierre (November 2020). "Controls on the magmatic fraction of extension at mid-ocean ridges". Earth and Planetary Science Letters 549: 116541. doi:10.1016/j.epsl.2020.116541. Bibcode: 2020E&PSL.54916541O. 
  25. ↑ Hofmann, A. W. (1997). "Mantle geochemistry: the message from oceanic volcanism". Nature 385 (6613): 219–228. doi:10.1038/385219a0. Bibcode: 1997Natur.385..219H. https://www.researchgate.net/publication/246759701. 
  26. ↑ Conder, James A.; Wiens, Douglas A.; Morris, Julie (August 2002). "On the decompression melting structure at volcanic arcs and back-arc spreading centers: ARC AND BACK-ARC MELTING". Geophysical Research Letters 29 (15): 17–1–17-4. doi:10.1029/2002GL015390. 
  27. ↑ Keen, C.E.; Courtney, R.C.; Dehler, S.A.; Williamson, M.-C. (February 1994). "Decompression melting at rifted margins: comparison of model predictions with the distribution of igneous rocks on the eastern Canadian margin". Earth and Planetary Science Letters 121 (3–4): 403–416. doi:10.1016/0012-821X(94)90080-9. Bibcode: 1994E&PSL.121..403K. 
  28. ↑ Sternai, Pietro (December 2020). "Surface processes forcing on extensional rock melting". Scientific Reports 10 (1): 7711. doi:10.1038/s41598-020-63920-w. PMID 32382159. Bibcode: 2020NatSR..10.7711S. 

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Bibliography

External links

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