Serra da Cangalha

Coordinates: 8°5′S 46°52′W / 8.083°S 46.867°W / -8.083; -46.867
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Serra da Cangalha
Tocantins
Serra da Cangalha is located in Brazil
Serra da Cangalha

Serra da Cangalha is an

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

References

  1. ^ "Serra da Cangalha". Earth Impact Database. Planetary and Space Science Centre University of New Brunswick Fredericton. Retrieved 2017-10-09.
  2. Bibcode:1992LPI....23..887M
    .
  3. ^ a b R. Almeida Filho; F.R. Moreira; C.H.Beisl (2003). "The Serra da Cangalha astrobleme as revealed by ASTER and SRTM orbital data" (PDF). International Journal of Remote Sensing. 24: 1–6. Archived from the original (PDF) on 2011-07-06. Retrieved 2007-09-24.
  4. doi:10.1016/j.tecto.2013.12.009
    .
  5. ^ a b R. Gregio. "Cratera da Serra da Cangalha". Archived from the original on 2007-09-30. Retrieved 2007-09-24.
  6. ^
    doi:10.1016/j.pepi.2004.08.029
    .
  7. ^ a b 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" (PDF). Lunar and Planetary Science XXXV. Retrieved 2007-09-24.
  8. ^ W. Masero; P.-A. Schnegg; S.L. Fontes. "Magnetotelluric investigation of the Serra da Cangalha impact crater, Northeast Brazil". {{cite journal}}: Cite journal requires |journal= (help)
  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. S2CID 4167202
    .
  11. ISBN 978-3-663-01891-9
    .
  12. 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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