Share to: share facebook share twitter share wa share telegram print page

 

Slab suction

Slab suction is one of the four main forces that drive plate tectonics. It creates a force that pulls down plates as they are subducting and speeds up their movement, creating larger amounts of displacement.

It is because of these forces, slab pull, ridge push, mantle convection, and slab suction that the Earth's crust is able to move and orient itself in various arrangements. This is how throughout the Earth's history there has been the ability to create super continents where all of the land mass has converged into one (for example, Pangaea).

Slab suction occurs when a subducting slab drives flow in the lower mantle by exerting additional force down in the direction of the mantle's convection currents. This flow then exerts shear tractions on the base of nearby plates. This driving force is important when the slabs (or portions thereof) are not strongly attached to the rest of their respective tectonic plate. They cause both the subducting and overriding plate to move in the direction of the subduction zone.[1]

This force occurs between two colliding plates where one is subducting beneath the other. As one plate subducts, it sets up convection currents in the upper mantle that exert a net trenchward pull, and acts to suck both the plates together.[2]

Slab suction is weaker than slab pull, which is the strongest of the driving forces. When measuring the forces of these two mechanisms, slab pull in subducting plate boundaries for upper mantle slabs is 1.9 × 10^21 N.[clarification needed] In comparison slab suction in the upper and lower mantle totaled 1.6 × 10^21 N.[3]

Slab suction in coordination with slab pull are used to analyze the speeds of plates work.[clarification needed] When you combine the slab pull of the upper mantle slabs with the slab suction of lower mantle slabs you get a model showing that subducting plates move four times faster than non subducting plates. Computing the slab suction force can give us predictions of the plate velocities by using viscous flow driven by the slabs and adding it to the shear tractions the flow exerts of the base of the plates.[4] Due to the flow in the lower mantle causing slab suction, changes in viscosity will have a much different effect than how it would apply to the upper mantle. In the lower mantle if you have a decrease in viscosity the flow will become much more rapid and increase the effect of slab suction and if viscosity in the lower mantle increases the effects of slab suction will decrease.

Associated with the slab suction force is the idea of trench roll-back. As a slab of oceanic crust subducts into the mantle, the hinge of the plate (the point where the plate begins to subduct) tends to regress away from the trench. This occurs because there is effectively no force to hold the hinge in one location.[5]

References

  1. ^ Conrad, C. P.; Lithgow-Bertelloni, C (2002). "How Mantle Slabs Drive Plate Tectonics". Science. 298 (5591): 207–209. Bibcode:2002Sci...298..207C. doi:10.1126/science.1074161. PMID 12364804
  2. ^ Wilson, M. (1993-10-01). "Plate-moving mechanisms: constraints and controversies". Journal of the Geological Society. 150 (5): 923–926. Bibcode:1993JGSoc.150..923W. doi:10.1144/gsjgs.150.5.0923. ISSN 0016-7649. S2CID 131474181.
  3. ^ Conrad, C. P.; Lithgow-Bertelloni, C (2002). "How Mantle Slabs Drive Plate Tectonics". Science. 298 (5591): 207–209. Bibcode:2002Sci...298..207C. doi:10.1126/science.1074161. PMID 12364804
  4. ^ Conrad, Clinton P.; Lithgow-Bertelloni, Carolina (2004). "The temporal evolution of plate driving forces: Importance of "slab suction" versus "slab pull" during the Cenozoic". Journal of Geophysical Research: Solid Earth. 109 (B10). doi:10.1029/2004JB002991. hdl:2027.42/95131. ISSN 2156-2202.
  5. ^ Wilson, M. (1993-10-01). "Plate-moving mechanisms: constraints and controversies". Journal of the Geological Society. 150 (5): 923–926. Bibcode:1993JGSoc.150..923W. doi:10.1144/gsjgs.150.5.0923. ISSN 0016-7649. S2CID 131474181.
Kembali kehalaman sebelumnya


Index: pl ar de en es fr it arz nl ja pt ceb sv uk vi war zh ru af ast az bg zh-min-nan bn be ca cs cy da et el eo eu fa gl ko hi hr id he ka la lv lt hu mk ms min no nn ce uz kk ro simple sk sl sr sh fi ta tt th tg azb tr ur zh-yue hy my ace als am an hyw ban bjn map-bms ba be-tarask bcl bpy bar bs br cv nv eml hif fo fy ga gd gu hak ha hsb io ig ilo ia ie os is jv kn ht ku ckb ky mrj lb lij li lmo mai mg ml zh-classical mr xmf mzn cdo mn nap new ne frr oc mhr or as pa pnb ps pms nds crh qu sa sah sco sq scn si sd szl su sw tl shn te bug vec vo wa wuu yi yo diq bat-smg zu lad kbd ang smn ab roa-rup frp arc gn av ay bh bi bo bxr cbk-zam co za dag ary se pdc dv dsb myv ext fur gv gag inh ki glk gan guw xal haw rw kbp pam csb kw km kv koi kg gom ks gcr lo lbe ltg lez nia ln jbo lg mt mi tw mwl mdf mnw nqo fj nah na nds-nl nrm nov om pi pag pap pfl pcd krc kaa ksh rm rue sm sat sc trv stq nso sn cu so srn kab roa-tara tet tpi to chr tum tk tyv udm ug vep fiu-vro vls wo xh zea ty ak bm ch ny ee ff got iu ik kl mad cr pih ami pwn pnt dz rmy rn sg st tn ss ti din chy ts kcg ve 
Prefix: a b c d e f g h i j k l m n o p q r s t u v w x y z 0 1 2 3 4 5 6 7 8 9