Academy Newspaper Thursday 15th December 1870
The Aerolitic Shower at Hessle.
This meteoric fall, the first recorded to have taken place
in Sweden, occurred at 12.20 p.m. on Ist January, 1869, in the neighbourhood of
Hessle, three Swedish miles from Upsala.
Prof. Nordenskjold, who announced the shower last year, has
now issued (Poggendorff’s Annalen, No. 10, 1870) a detailed account of the
physical and chemical characters of the stones, and the phenomena attending
their descent. They were strewn over a line of country lying 30° E. of S.
towards 30° W. of N.
Some fell within a few yards of peasants leaving church,
another fell close to a fisherman on the Malar Bay Larsta-Viken, dug a hole 3
to 4 inches deep in the ice, and rebounded; when picked up, it was still warm.
The noise accompanying the fall, which was heard in Stockholm, is described as
resembling some very heavy thunderclaps, followed by a rattle like the passing
of waggons at a gallop, and ending with first a note like an organ tone and
then a hissing sound, the whole lasting some minutes.
The sky was cloudy,
and though apparently unseen at Hessle itself, a luminous meteor was noticed by
observers at a distance. The stones vary greatly in size, some weighing nearly
2 lbs., the smallest (and the little ones were numerous) only 0'07 gramme.
Though of sufficiently loose structure to break in pieces
when thrown with the hand against the floor or frozen ground, it is remarkable
that nearly all the specimens are intact, and that some of the stones weighing
2 lbs. which struck the ice of the Larsta-Viken, failed to penetrate it, though
its thickness on that day did not exceed a few inches. These facts support the
statements of eyewitnesses as to their remarkably small downward velocity.
These meteorites present no unusual aspect, and resemble in
particular those of Aussun and Clarac, Haute-Garonne, which fell on the 9th
December 1858. Their exterior is black; within they are bright grey, and
sufficiently porous to cling to the tongue, whence it is concluded that their
mass has not undergone fusion, as would be required by the theory of Laplace.
Chemical analysis proved them to be composed
of about 20 per cent. of nickeliferous iron (chamoisite, Fe,Ni); some
schreibersite, and rather less than 1 per cent. of what was probably chromite;
a variable amount of iron monosulphide (troilite) ; a trace of carbon, probably
in the form of a hydrocarbon; traces of salts soluble in water; about 10 per
cent. of labradorite or anorthite; 37 per cent. of olivine; and 23 per cent. of
shepardite. These silicates, it should be remarked, were not isolated for
examination, but are assumed to be present from calculations based on the
results of an analysis of the mass. The
researches of Prof. Maskelyne and Dr. Laurence Smith have shown the
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