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VI.—A Chapter in the History of Meteorites

Published online by Cambridge University Press:  01 May 2009

Walter Flight
Walter Flight
Affiliation:
Of the Department of Mineralogy, British Museum.
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Extract

Shortly after this remarkable shower of meteorites had taken place two very full reports on the occurrence were drawn up by von Haidinger. It is computed that over a very limited area more than a thousand stones, weighing in all from 8 to 10 cwt., must have fallen. The largest found is now preserved in the Vienna Collection; it weighs 293·3 kilog. (5 cwt. 3 qrs. 3 lbs.), and measures 2ft. 4 in. long and 18 in. broad, and penetrated the ground to a depth of 11 ft. For drawings of this enormous block, the largest mass of meteoric rock preserved in any collection, and coloured representations of the meteor which was observed at the time of its descent, the reader is referred to von Haidinger's two memoirs.

Type
Original Articles
Information
Geological Magazine , Volume 2 , Issue 12 , December 1875 , pp. 589 - 608
Copyright
Copyright © Cambridge University Press 1875

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References

page 589 note 2 Kenngott., A.Sitzber. Ak. Wiss. Wien, 1869, lix 873.Google ScholarPhil. Mag., 1869, xxxvii. 424.Google Scholar —Schiaparelli, J. V.. Entwurf einer astronomischen Theorie der Sternschnuppen. 1871.Google Scholar Stettin: Nahmer. Page 267.—von Baumhauer, E. H.Archives Néerlandaises, 1872, vii. 146.Google Scholar —See also von Haidinger, W.. Sitzber. Ak. Wiss. Wien, liv. 200Google Scholar and 513. —Rose, G.. Monatsber. Ak. Wiss. Berlin, lxvii. 203.Google Scholar

page 591 note 1 With traces of manganese protoxide.

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page 595 note 1 Constituents removed with sodium carbonate, but undetermined.

page 595 note 2 With trace of potash.

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page 596 note 1 A. Goiran, A Bertolio, A. Zannetti, and L. Musso. Sopra gli Aeroliti caduti il giorno 29 febbraio 1868 nel territorio di Villanova e Motta dei Conti, Piemonte, circondario di Casale. Con Introduzione del padre Denza. 1868, Torino. See also Bull, meteor, dell' Osserv. del R. Coll. Carlo Alberti in Montcalieri, March to June, 1868. —Denza, F.. Compt. rend., 1868, lxvii. 322.Google Scholar —Jervis, G.. I Tesori Sotterranei dell' Italia. Parte Prima. 1873, Torino: Loescher. Page 153.Google Scholar

page 596 note 2 The trajectory of this stone could be approximately determined since three points in a vertical plane were determined: 1) the point where it grazed the top of a tree, 2) the broken end of the bough of a walnut tree severed by the meteorite, and 3) the point where it entered the ground. Other peasants, who were employed lopping trees near the high road which leads from Casale to Vercelli, at a point about 1200 metres from Villanova, observed a rain of black grains; one man was struck on the hat with a piece of considerable size.

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page 601 note 1 In his paper on the Belgian meteorite, a specific gravity = 3·43 is given.

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