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Octahedrite
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{{Short description|Structural class of iron meteorites}} {{Use American English|date=January 2019}} {{Use mdy dates|date=January 2019}} {{Infobox meteorite subdivision |Subdivision = Structural class |Name = Octahedrite |Alternative_names = |Image = TolucaMeteorite.jpg |Image_caption = Octahedrite from [[Toluca]] |Image_alt_text = |Compositional_type = Iron |Type = |Class = |Clan = |Group = <!-- list/link all subgroups of this group as a {{flatlist}} |Subgroups = {{flatlist| * }} --> |Parent_body = |Composition = |Petrologic_type = |Number_of_specimens = |TKW = <!-- {{Convert||kg}} --> |Image2 = Meteoric iron phase diagram taenite kamacite octaehedrite.svg |Image2_caption = A phase diagram showing the link between structural and chemical classification. |Image2_alt_text = }} '''Octahedrites''' are the most common [[Iron meteorite#Structural classification|structural class]] of [[iron meteorite]]s. The structures occur because the [[meteoric iron]] has a certain [[nickel]] concentration that leads to the [[exsolution]] of [[kamacite]] out of [[taenite]] while cooling. ==Structure== {{see also|Widmanstätten pattern#Lamellæ formation mechanism|Widmanstätten pattern#Shape and orientation}} Octahedrites derive their name from the crystal structure paralleling an [[octahedron]]. Opposite faces are parallel so, although an octahedron has 8 faces, there are only 4 sets of [[kamacite]] plates. Due to a long cooling time in the interior of the parent [[asteroid]]s, these alloys have crystallized into intermixed millimeter-sized bands (from about 0.2 mm to 5 cm).<ref name=CdE2009>{{cite journal |title=Iron meteorites: Crystallization, thermal history, parent bodies, and origin |journal=Chemie der Erde – Geochemistry |volume=69 |issue=4 |pages=293–325 |doi=10.1016/j.chemer.2009.01.002 |year=2009 |last1=Goldstein|first1=J.I |last2=Scott|first2=E.R.D |last3=Chabot|first3=N.L |bibcode=2009ChEG...69..293G }}</ref> When polished and acid etched the classic [[Widmanstätten pattern]]s of intersecting lines of lamellar kamacite, are visible. In gaps between the kamacite and taenite lamellae, a fine-grained mixture called [[plessite]] is often found. An iron nickel phosphide, [[schreibersite]], is present in most nickel-iron meteorites, as well as an iron-nickel-[[cobalt]] [[carbide]], [[cohenite]]. [[Graphite]] and [[troilite]] occur in rounded nodules up to several cm in size.<ref name=him1975>Vagn F. Buchwald: Handbook of Iron Meteorites. University of California Press, 1975.</ref> ==Subgroups== [[File:ZacatecasMeteoriteGDL cropped.JPG|thumb|280px|The Zacatecas Meteorite found in 1782 in Zacatecas Mexico, weighing 780kg.]] {{see also|Iron meteorite#Structural classification}} Octahedrites can be grouped by the dimensions of kamacite lamellae in the [[Widmanstätten pattern]], which are related to the [[nickel]] content:<ref>James H. Shirley,Rhodes Whitmore Fairbridge, ''Encyclopedia of planetary sciences'', Springer, 1997. {{ISBN|978-0-412-06951-2}}</ref> * Coarsest octahedrites, lamellae width >3.3 mm, 5–9% Ni, symbol Ogg * Coarse octahedrites, lamellae 1.3–3.3 mm, 6.5–8.5% Ni, symbol Og * Medium octahedrites, lamellae 0.5–1.3 mm, 7–13% Ni, symbol Om * Fine octahedrites, lamellae 0.2–0.5 mm, 7.5–13% Ni, symbol Of * Finest octahedrites, lamellae <0.2 mm, 17–18% Ni, symbol Off * Plessitic octahedrites, kamacite spindles, a transitional structure between octahedrites and [[ataxite]]s,<ref>Geochimica et Cosmochimica Acta, Volume 45, Ed. 9–12</ref> 9–18% Ni, symbol Opl ==Mineral== Octahedrite is an obsolete synonym for [[anatase]], one of the three known [[titanium]] dioxide [[mineral]]s.{{cn|date=September 2023}} ==See also== * [[Glossary of meteoritics]] ==References== {{Reflist}} ==External links== *[http://webmineral.com/data/Kamacite.shtml Webmineral] *[http://www.amonline.net.au/geoscience/meteors/types.htm Meteorites Australia] {{Meteorites}}
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