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  2. Алексеев А.С. и др. (1991). Оценки частоты падения небесных тел на Землю, исследование возможности заблаговременного их обнаружения и изменения траекторий. Отчёт по НИР, АН СССР ВЦ, Новосибирск , 128 с.
  3. Graham, Bevan and Hutchison (1985). Catalogue of Meteorites. 4th Edition
  4. Grieve R.A.F. (1987). Terrestrial impact structures. Ann.Rev.Earth Planet.Sci., Vol.15, p. 245-270
  5. (1988). Astronauts guide to terrestrial impact craters.. Space Shuttle Earth Observation Project, Lunar and Planetary Institute (March 1988).
  6. Hodge, Paul W., (1994). Meteorite craters and impact structures of the Earth. Cambridge University Press , 122 рр.
  7. Osinski Gordon R. (2006). The geological record of meteorite impacts. 40th ESLAB First International Conference on Impact Cratering in the Solar System, 8-12 May 2006., Noordwijk,The Netherlands
  8. Jarmo Moilanen (2009). Impact Structures of the World.
Вихреподобная круговая особенность.

Tin Bider is a multi ring structure approximately 6 km in diameter. The target rocks are alternating sequences of upper Cretaceous clay and limestone. Massive continental sandstone of lower Cretaceous is exposed in the center having been uplifted approximately 500m from normal depth.

Shatter cones were initially reported, but were not officially documented. Subsequent investigation yielded conically striated ventifacts created by wind erosion. PDF's have been identified in some mineral grains, which indicate an impact origin for the structure, as does the stratigraphic evidence.

There is a distinct lack of allochthonous material, which suggests that the structure has been eroded to a depth below that of the original crater floor.

One feature that tends to distinguish Tin Bider from other terrestrial impact structures is the extreme prominence of ductile deformation, where brittle deformation is typical for other impacts.

Global Impact Studies Project


Спутниковая фотография кратера из Google Earth.


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