1. Зоткин И.Т., Дабижа А.И. (1982). Эволюция метеоритного кратера как процесс случайных перемещений.. Метеоритика, Issue 40, с. 82-90
  2. Gostin V.A., Therriault A.M. (1997). Tookoonooka, a large buried Early Cretaceous impact structure in the Eromanga Basin of southwestern Queensland // Australia. Meteoritics and Planetary Science 32, 593-599.
  3. Preface // Ber. Polarforsch. - No.343. - P. 3-6.
  4. Spray J.G. (2005). Impact Structures listed by Name. Current total number of confirmed impact structures: 172 .
  5. Haines P.W. (2005). Impact cratering and distal ejecta: the Australian record. Aus.Journal of Earth sciences. Vol.52, N.4/5. Aug./Oct. p.481-507
  6. Osinski G.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
  7. BRON K.A., GOSTIN V. (2012). The Tookoonooka marine impact horizon, Australia: Sedimentary and petrologic evidence // Meteoritics & Planetary Science 47, Nr 2, 296-318.

Спутниковая фотография кратера из Google Earth.

Геологическая карта кратера
The clasts consist of impact breccia fragments, as well as devitrified impact melt glass. Breccia samples have also been found during drilling into the central uplift dome; these breccias have a devitrified glassy matrix, with angular clasts.
(Gostin, Therriault, 1997).

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