Serra Da Cangalha

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Short description: Impact crater in Brazil
Serra da Cangalha
Serra da Cangalha Crater.jpg
Serra da Cangalha crater
Impact crater/structure
ConfidenceConfirmed
Diameter12–13 km (7.5–8.1 mi)
Age<300 Ma
ExposedYes
DrilledYes
Location
LocationParnaíba Basin
Coordinates [ ⚑ ] : 8°5′S 46°52′W / 8.083°S 46.867°W / -8.083; -46.867
CountryBrazil
StateTocantins
Serra da Cangalha is located in Brazil
Serra da Cangalha
Location of the crater in Brazil

Serra da Cangalha is an impact crater in the State of Tocantins, near the border of Maranhão State, in north/northeastern Brazil.[1] The crater is between 12 and 13 kilometres (7.5 and 8.1 mi) in diameter, making it the second-largest known crater in Brazil.[2] Its age is estimated to be about 220 million years (Triassic period).[3] The name means Pack-Saddle Mountains in Portuguese.

Description

The outer perimeter is a circular inward scarp about 12 kilometres (7.5 mi) in diameter on the largely undisturbed Cretaceous and upper Silurian sediments of the Parnaíba basin,[4] breached on the west, north, and south sides by drainage valleys. Within the perimeter there is a series of concentric circular valleys and a central basin, all at roughly the same elevation, separated by ring walls. Shuttle Radar Topography Mission imagery shows a faint ring about 11 kilometres (6.8 mi) in diameter, a second ring of gentle hills about 5 to 6 kilometres (3.1 to 3.7 mi) in diameter, and an inner ring of steeper hills, about 3 kilometres (1.9 mi) in diameter and up to 420 metres (1,380 ft) high, open to the northwest, surrounding a central basin about 2.2 kilometres (1.4 mi) in diameter.[5][6][7]

The impact origin is attested by the presence of impact breccias, quartzite shatter cones and shocked quartz. The meteorite is believed to have struck the surface at a low oblique angle, 25 to 30 degrees on dry land. Radial faults are present inside the crater, and some extend up to 16 km from the center.[7] Disturbed and steeply inclined sediments from the Carboniferous and Devonian periods occur within the crater. A magnetic survey of the structure indicates that deformation within the crater extends to a depth of about 2 kilometres (1.2 mi).[3][5][6][8][9]

History and studies

The identification of the structure as an impact crater was first published in 1973 by R.S. Dietz and B.M. French.[10][11] Shatter cones were reported by Beatty in 1980.[12] Impact breccias, impact melting, and shocked quartz were reported by McHone in his 1986 thesis.[13] A magnetic survey of the structure was published by A.A. Adepelumi and others in 2005.[6]

See also

  • Riachão Ring
  • Santa Marta crater

References

  1. ↑ "Serra da Cangalha". Earth Impact Database. Planetary and Space Science Centre University of New Brunswick Fredericton. http://www.passc.net/EarthImpactDatabase/New website_05-2018/serra-da-cangalha.html. Retrieved 2017-10-09. 
  2. ↑ McHone, J. F.; Dietz, R. S. (1992). "Earth's multiple impact craters and astroblemes (abstract)". Houston: Lunar and Planetary Institute. pp. 887–888. Bibcode: 1992LPI....23..887M. 
  3. ↑ 3.0 3.1 R. Almeida Filho; F.R. Moreira; C.H.Beisl (2003). "The Serra da Cangalha astrobleme as revealed by ASTER and SRTM orbital data". International Journal of Remote Sensing 24: 1–6. http://mtc-m12.sid.inpe.br/col/sid.inpe.br/sergio/2005/06.17.18.34/doc/raimundo4.pdf. Retrieved 2007-09-24. 
  4. ↑ De Castro, David L.; Fuck, Reinhardt A.; Phillips, Jeffrey D.; Vidotti, Roberta M.; Bezerra, Francisco H. R.; Dantas, Elton L. (2014). "Crustal structure beneath the Paleozoic Parnaíba Basin revealed by airborne gravity and magnetic data, Brazil on USGS". Tectonophysics 614: 18. doi:10.1016/j.tecto.2013.12.009. https://pubs.er.usgs.gov/publication/70118240. 
  5. ↑ 5.0 5.1 R. Gregio. "Cratera da Serra da Cangalha". http://rgregio.astrodatabase.net/cratera_serra_cangalha.htm. 
  6. ↑ 6.0 6.1 6.2 Adepelumi, A. A.; Fontes, S.L.; Schnegg, P.A.; Flexor,J.M. (2005). "An integrated magnetotelluric and aeromagnetic investigation of the Serra da Cangalha impact crater, Brazil". Physics of the Earth and Planetary Interiors 150 (1): 159–182. doi:10.1016/j.pepi.2004.08.029. Bibcode: 2005PEPI..150..159A. http://doc.rero.ch/record/5061/files/1_Schnegg_Pierre-Andr___-_An_integrated_magnetotelluric_20050905.pdf. 
  7. ↑ 7.0 7.1 W.U. Reimold; G.R.J. Cooper; R. Romano; D. Cowan; C. Koeberl (2004). "A SRTM Investigation of Serra da Cangalho [sic] Impact Structure, Brazil". http://www.lpi.usra.edu/meetings/lpsc2004/pdf/1232.pdf. Retrieved 2007-09-24. 
  8. ↑ W. Masero; P.-A. Schnegg; S.L. Fontes. Magnetotelluric investigation of the Serra da Cangalha impact crater, Northeast Brazil. 
  9. ↑ Adekunle Adepelumi; Jean M. Flexor; Sergio L. Fontes; Pierre-A. Schnegg. "A magnetotelluric investigation of the Serra da Cangalha impact crater structure, Brazil". 
  10. ↑ Dietz, R.S.; French, B.M. (1973). "Two probable astroblemes in Brazil". Nature 244 (5418): 561–562. doi:10.1038/244561a0. Bibcode: 1973Natur.244..561D. 
  11. ↑ Crósta, A. P. (1987). J. Pohl. ed. "Impact structures in Brazil". Research in Terrestrial Impact Structures (Braunschweig/Wiesbad: Friedrich, Vieweg & Sohn): 30–38. doi:10.1007/978-3-663-01889-6_2. ISBN 978-3-663-01891-9. Bibcode: 1987rtis.conf...30C. 
  12. ↑ Beatty J. K. (1980). "Crater hunting in Brazil". Sky and Telescope 59: 464––467. Bibcode: 1980S&T....59..464B. 
  13. ↑ McHone J. F. (1986). Terrestrial impact structures: Their detection and verification with new examples from Brazil. University of Illinois at Urbana-Champaign, Urbana, Illinois. p. 210. 



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Categories: [Impact craters of Brazil] [Triassic impact craters]

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