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Shock metamorphism

From Wikipedia, the free encyclopedia
Shock-wave related deformation and heating of rocks during collisions
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Shock metamorphism orimpact metamorphism describes the effects of shock-wave related deformation and heating duringimpact events.

The formation of similar features duringexplosive volcanism is generally discounted due to the lack ofmetamorphic effects unequivocally associated with explosions and the difficulty in reaching sufficient pressures during such an event.[1]

Effects

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Mineral microstructures

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Planar fractures

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Planar fractures are parallel sets of multiple planar cracks or cleavages inquartz grains; they develop at the lowestpressures characteristic ofshock waves (~5–8 GPa) and a common feature of quartz grains found associated with impact structures. Although the occurrence of planar fractures is relatively common in other deformed rocks, the development of intense, widespread, and closely spaced planar fractures is considered diagnostic of shock metamorphism.[2]

Planar deformation features

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Shocked quartz with two sets of ‘decorated’ planar deformation features inimpact melt rock from theSuvasvesi South impact structure, Finland (thin sectionphotomicrograph, plane polarized light).
Main article:Planar deformation features

Planar deformation features, or PDFs, are optically recognizable microscopic features ingrains ofsilicate minerals (usuallyquartz orfeldspar), consisting of very narrow planes ofglassy material arranged in parallel sets that have distinct orientations with respect to the grain'scrystal structure. PDFs are only produced by extreme shock compressions on the scale of meteor impacts. They are not found involcanic environments.

Brazil twinning in quartz

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This form oftwinning in quartz is relatively common but the occurrence of close-spaced Brazil twins parallel to thebasal plane, (0001), has only been reported from impact structures. Experimental formation of basal-orientated Brazil twins in quartz requires high stresses (about 8GPa) and high strain rates, and it seems probable that such features in natural quartz can also be regarded as unique impact indicators.[2]

High-pressure polymorphs

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The very high pressures associated with impacts can lead to the formation of high-pressurepolymorphs of various minerals. Quartz may occur as either of its two high-pressure forms,coesite andstishovite. Coesite occasionally occurs associated witheclogites formed during very high pressure regional metamorphism but was first discovered in a meteorite crater in 1960.[3] Stishovite, however, is only known from impact structures.

Reidite, the high-pressurescheelite-structure polymorph ofzircon, is known only from impact structures.

Shatter cones developed in fine graineddolomite from theWells Creek crater, USA.

Two of the high-pressurepolymorphs oftitanium dioxide, one with abaddeleyite-like form and the other with aα-PbO2 structure, have been found associated with theNördlinger Ries impact structure.[4][5]

Diamond, the high-pressureallotrope ofcarbon, has been found associated with many impact structures, and bothfullerenes andcarbynes have been reported.[6]

Shatter cones

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Main article:Shatter cone

Shatter cones have a distinctively conical shape that radiates from the top of the cones repeating cone-on-cone, at various scales in the same sample. They are only known to form in rocks beneathmeteoriteimpact craters orunderground nuclear explosions. They are evidence that the rock has been subjected to a shock with pressures in the range of 2-30GPa.[7][8][9]

Occurrence

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The effects described above have been found singly, or more often in combination, associated with every impact structure that has been identified on Earth. The search for such effects therefore forms the basis for identifying possible candidate impact structures, particularly to distinguish them from volcanic features.

See also

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References

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  1. ^A. J. Gratz, A.J., W. J. Nellis, W.J. & Hinsey, N. 1992. Laboratory Simulations of Explosive Volcanism and Implications for the K/T boundary. Abstracts of the Lunar and Planetary Science Conference, volume 23, page 441.
  2. ^abChapter 4, 'Shock-Metamorphic Effects in Rocks and Minerals' of the online book, French, B.M. 1998.Traces of Catastrophe, A handbook of shock-metamorphic effects in terrestrial meteorite impact structures,Lunar and Planetary Institute 120pp.
  3. ^Chao, E. C. T.;Shoemaker, E. M.; Madsen, B. M. (1960). "First Natural Occurrence of Coesite".Science.132 (3421):220–222.Bibcode:1960Sci...132..220C.doi:10.1126/science.132.3421.220.PMID 17748937.S2CID 45197811.
  4. ^El Goresy, A; Chen, M; Dubrovinsky, L; Gillet, P; Graup, G (August 2001). "An ultradense polymorph of rutile with seven-coordinated titanium from the Ries crater".Science.293 (5534):1467–70.doi:10.1126/science.1062342.PMID 11520981.S2CID 24349901.
  5. ^El Goresy, Ahmed (2001). "A natural shock-induced dense polymorph of rutile with α-PbO2 structure in the suevite from the Ries crater in Germany".Earth and Planetary Science Letters.192 (4):485–495.Bibcode:2001E&PSL.192..485E.doi:10.1016/S0012-821X(01)00480-0.
  6. ^Gilmour, I (1999). "Carbon allotropes in impact-produced rocks".Meteoritics & Planetary Science.34: A43.Bibcode:1999M&PSA..34R..43G.
  7. ^French, B.M. (1998).Traces of Catastrophe.Lunar and Planetary Institute. Retrieved2007-05-20.
  8. ^Sagy, A.; Fineberg, J.; Reches, Z. (2004)."Shatter cones: Branched, rapid fractures formed by shock impact".Journal of Geophysical Research.109 (B10): B10209.Bibcode:2004JGRB..10910209S.doi:10.1029/2004JB003016.
  9. ^French, Bevan M. (2005)."Stalking the Wily Shatter Cone: A Critical Guide for Impact-Crater Hunters"(PDF).Impacts in the Field.2 (Winter).Impact Field Studies Group: s 3–10. Archived fromthe original(PDF) on 2011-07-20.

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