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Paranaíba meteorite, Cancan farm, Cassilândia, Mato Grosso do Sul, Brazili
Regional Level Types
Paranaíba meteoriteMeteorite Fall Location
Cancan farmFarm
CassilândiaMunicipality
Mato Grosso do SulState
BrazilCountry

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Latitude & Longitude (WGS84):
19° 7' 60'' South , 51° 40' 0'' West
Latitude & Longitude (decimal):
Meteorite Class:
Meteoritical Society Class:
Köppen climate type:
Nearest Settlements:
PlacePopulationDistance
Cassilândia18,497 (2017)7.4km


Ordinary chondrite—black, brecciated, veined (L6,br; S6)
Fall, 1956; 100 kg

A large meteorite, accompanied by detonations, was seen to fall and was evacuated from a 2m deep pit. A large portion of the meteorite was apparently destroyed by local residents. In hand specimens, the meteorite feature's are quite conspicuous as the predominant light round and angular fragments are cut by dark veins and contain broad black areas. A few chondrules are visible in lighter areas, but are absent from darker areas. The lighter areas constitute a monomict breccia, but very fine-grained and variegated opaques occupy the dark veins and dark regions. Total iron contents (Fe 20.86 wt%) along with olivine (Fa23.57) and low Ca-pyroxene (Fs20.7) compositions are characteristic of the L-chondrite geochemical group. Olivine, the predominant phase, is accompanied by lesser amounts of orthopyroxene and albitic plagioclase along with quite minor amounts of troilite and Fe-Ni metal. Accessory chromite, diopside, merrillite and traces of other sulfides and oxides are also reported. The meteorite's dark areas — containing abundant glass and pervasive droplets of Fe-metal and sulfides — are simply the most obvious indicators of very strong pre-terrestrial shocks (level S6). In numerous instances both olivine and orthopyroxene have been converted to weakly isotropic phases or even to completely isotropic glass.

Ar-40-Ar-39 dating of glassy portions of Paranaiba has indicated that the Paranaiba breccia is a mixture of materials which were involved in different (asteroidal) collisions in past eons before they eventually became neighboring constituents of the same earth-bound meteoroid.

The L (relatively low in total iron) chondrites represent ~45% of properly classified meteorite falls with the L6 type by far the largest subset [~70% of L falls]. Of the 271 meteorite falls classified exactly as an 'L6' chondrite Paranaiba is the 9th most massive (as of June 2016). Five L6 meteorites — including 3 falls — have been recovered from Brazil. The 300 kg Putinga fall of 1937 was even more massive.

The largest extant masses (500—1000 g range) have been kept at the Instituto de Geosciências (São Paulo), Museu Nacional-Universidade (Rio de Janeiro), and the United States National Museum (Washington, DC).

Synonyms: Can-Can, Mato Grosso

Select Mineral List Type

Standard Detailed Gallery Strunz Chemical Elements

Mineral List


7 valid minerals.

Meteorite/Rock Types Recorded

Note: data is currently VERY limited. Please bear with us while we work towards adding this information!

Select Rock List Type

Alphabetical List Tree Diagram

Detailed Mineral List:

Chromite
Formula: Fe2+Cr3+2O4
Reference: Ramdohr, P. (1973). The Opaque Minerals in Stony Meteorites. Elsevier Publishing Company: Amsterdam; London: New York. 245 pages.; Gomes, C.B. & Keil, K. (1980) Brazilian Stony Meteorites: University of New Mexico Press: Albuquerque. 162 Pages.
Diopside
Formula: CaMgSi2O6
Reference: Gomes, C.B. & Keil, K. (1980) Brazilian Stony Meteorites: University of New Mexico Press: Albuquerque. 162 Pages.
'Fayalite-Forsterite Series'
Description: Olivine (Mean:Fa23.7, Range: 22.6–24.8) — Often shocked & recrystallized.
Reference: Gomes, C.B. & Keil, K. (1980) Brazilian Stony Meteorites: University of New Mexico Press: Albuquerque. 162 Pages.; Stöffler D., Keil K. & Scott E. R D. (1991) Shock metamorphism of ordinary chondrites. Geochim. Cosmochim. Acta, 55, 3845–3867. (Sept 1991).
'Glass'
Description: Glass is quite variable in composition.
Reference: Gomes, C.B. & Keil, K. (1980) Brazilian Stony Meteorites: University of New Mexico Press: Albuquerque. 162 Pages.
Ilmenite
Formula: Fe2+TiO3
Reference: Ramdohr, P. (1973). The Opaque Minerals in Stony Meteorites. Elsevier Publishing Company: Amsterdam; London: New York. 245 pages.
Isocubanite
Formula: CuFe2S3
Reference: Ramdohr, P. (1973). The Opaque Minerals in Stony Meteorites. Elsevier Publishing Company: Amsterdam; London: New York. 245 pages.
Mackinawite
Formula: (Fe,Ni)9S8
Reference: Ramdohr, P. (1973). The Opaque Minerals in Stony Meteorites. Elsevier Publishing Company: Amsterdam; London: New York. 245 pages.
'Maskelynite'
Description: Maskelynite composition (An11.3Ab83.1Or5.6) corresponds to oligoclase.
Reference: Gomes, C.B. & Keil, K. (1980) Brazilian Stony Meteorites: University of New Mexico Press: Albuquerque. 162 Pages.
'Meteoritic Iron'
Description: Fe-Ni metal often exists as small droplets or as troilite-metal intergrowths. Phases other than taenite are not reported here.
Reference: Gomes, C.B. & Keil, K. (1980) Brazilian Stony Meteorites: University of New Mexico Press: Albuquerque. 162 Pages.
'Orthopyroxene Subgroup'
Reference: Gomes, C.B. & Keil, K. (1980) Brazilian Stony Meteorites: University of New Mexico Press: Albuquerque. 162 Pages.
Taenite
Formula: (Fe,Ni)
Description: Taenite is the only phase of Fe-Ni metal specifically reported by Ramdohr, 1973.
Reference: Ramdohr, P. (1973). The Opaque Minerals in Stony Meteorites. Elsevier Publishing Company: Amsterdam; London: New York. 245 pages.; Gomes, C.B. & Keil, K. (1980) Brazilian Stony Meteorites: University of New Mexico Press: Albuquerque. 162 Pages.
Troilite
Formula: FeS
Reference: Ramdohr, P. (1973). The Opaque Minerals in Stony Meteorites. Elsevier Publishing Company: Amsterdam; London: New York. 245 pages.; Stöffler D., Keil K. & Scott E. R D. (1991) Shock metamorphism of ordinary chondrites. Geochim. Cosmochim. Acta, 55, 3845–3867. (Sept 1991).

Gallery:

List of minerals arranged by Strunz 10th Edition classification

Group 1 - Elements
Taenite1.AE.10(Fe,Ni)
Group 2 - Sulphides and Sulfosalts
Isocubanite2.CB.55bCuFe2S3
Mackinawite2.CC.25(Fe,Ni)9S8
Troilite2.CC.10FeS
Group 4 - Oxides and Hydroxides
Chromite4.BB.05Fe2+Cr3+2O4
Ilmenite4.CB.05Fe2+TiO3
Group 9 - Silicates
Diopside9.DA.15CaMgSi2O6
Unclassified Minerals, Rocks, etc.
'Fayalite-Forsterite Series'-
'Glass'-
'Maskelynite'-
'Meteoritic Iron'-
'Orthopyroxene Subgroup'-

List of minerals for each chemical element

OOxygen
O ChromiteFe2+Cr23+O4
O IlmeniteFe2+TiO3
O DiopsideCaMgSi2O6
MgMagnesium
Mg DiopsideCaMgSi2O6
SiSilicon
Si DiopsideCaMgSi2O6
SSulfur
S IsocubaniteCuFe2S3
S Mackinawite(Fe,Ni)9S8
S TroiliteFeS
CaCalcium
Ca DiopsideCaMgSi2O6
TiTitanium
Ti IlmeniteFe2+TiO3
CrChromium
Cr ChromiteFe2+Cr23+O4
FeIron
Fe ChromiteFe2+Cr23+O4
Fe IlmeniteFe2+TiO3
Fe IsocubaniteCuFe2S3
Fe Mackinawite(Fe,Ni)9S8
Fe Taenite(Fe,Ni)
Fe TroiliteFeS
NiNickel
Ni Mackinawite(Fe,Ni)9S8
Ni Taenite(Fe,Ni)
CuCopper
Cu IsocubaniteCuFe2S3

References

Sort by

Year (asc) Year (desc) Author (A-Z) Author (Z-A)
Ramdohr, P. (1973). The Opaque Minerals in Stony Meteorites. Elsevier Publishing Company: Amsterdam; London: New York. 245 pages.
Gomes, C.B. & Keil, K. (1980) Brazilian Stony Meteorites: University of New Mexico Press: Albuquerque. 162 pages.
Stöffler D., Keil K. & Scott E. R D. (1991) Shock metamorphism of ordinary chondrites. Geochim. Cosmochim. Acta, 55, 3845–3867. (Sept 1991).
Kunz, J., Falter, M. & Jessberger, E.K. (1997) Shocked meteorites: Argon-40-argon-39 evidence for multiple impacts: Meteoritics & Planetary Science 32(5): 647-670. (Sept 1997).
Zucolotto, M.E., Andrade, W.A. & Klein, V.C. (2000) The meteorite collection of Museu Nacional-Universidade Federal do Rio de Janeiro, Brazil: Meteoritics & Planetary Science 35(S5): pp. A185–A187. (Sept 2000).
Grady, M.M (2000). Catalogue of Meteorites (5/e). Cambridge University Press: Cambridge; New York; Oakleigh; Madrid; Cape Town. 689 pages.

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