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The Tenham (Queensland) meteoritic shower of 1879 (With Plates XIV-XVII.)

Published online by Cambridge University Press:  14 March 2018

L. J. Spencer*
Affiliation:
British Museum

Extract

Very little reformation can now be gathered about a remarkable shower of meteoric stones that fell many years ago in a remote district in south-west Queensland. Only a few scraps of information have appeared in print, and these are largely contradictory. However, some very tangible evidence arrived unexpectedly at the British Museum in 1935 in the form of a remarkable collection of 102 complete meteoric stones with a total weight of 107¾lb. This material had been in the possession of Mr. Benjamin Dunstan, formerly Government Geologist of Queensland, who had been collecting information of the fall with a view to writing up an account for publication. This unfortunately he never did, and much of the information is now lost. The specimens were offered to the British Museum by his widow, but they came along quite casually as an appendix to a collection of fossils.

Type
Research Article
Copyright
Copyright © The Mineralogical Society of Great Britain and Ireland 1937

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References

page 437 note 1 Dunstan, Benjamin (1864-1933). Obituary notices in Queensland Government Mining Journal, 1933, vol. 34, p. 276 Google Scholar, with portrait; Min. Mag., 1936, vol. 24, p. 284.

page 439 note 1 Anderson, C., A catalogue and bibliography of Australian meteorites. Rec. Australian Museum, 1913, vol. 10, pp. 53-76.CrossRefGoogle Scholar

page 446 note 1 Prior, G. T., Min. Mag., 1916, vol. 18, p. 7.Google Scholar

page 446 note 2 Prior, G. T., Catalogue of Meteorites, British Museum, 1923, p. 189.Google Scholar

page 447 note 1 Prior, G. T., Min. Mag., 1916, vol. 18 Google Scholar, plates I and II.

page 447 note 2 Wülfing, E. A., Die Meteoriten in Sammlungen. Tübingen, 1897, p. 287.Google Scholar

page 448 note 1 The numerous smaller masses of iron found scattered around the Henbury craters and around the single crater at Canyon Diablo, Arizona, resulted from the breaking up of the larger mass by the gaseous explosion that formed the crater.

page 448 note 2 Spencer, L. J., Min. Mag., 1932, vol. 23, p. 7.Google Scholar

page 448 note 3 Ibid., 1935, vol. 24, p. 16.

page 449 note 1 Min. Abstr., 1933, vol. 5, p. 300.

page 450 note 1 Fletcher, L., Min. Mag., 1889, vol. 8, p. 226 Google Scholar ; Farrington, O. C., Meteorites, 1915, p. 46.Google Scholar

page 450 note 2 Silberrad, C. A., Min. Mag., 1932, vol. 23, p. 299.CrossRefGoogle Scholar

page 450 note 3 Spencer, L. J.,Min. Mag., 1933, vol. 23, p. 399 Google Scholar; Meteorite craters as topographical features on the earth's surface. Geogr. Journ., 1933, vol. 81, pp. 227-248 ; and Ann. Rep. Smithsonian Inst., 1935, for 1933, pp. 307-325.