Buenos Ayres and the Provinces of the Rio de La Plata: Their Present State, Trade, and DebtParish, Woodbine, Sir
History
Buenos Ayres and the Provinces of the Rio de La Plata: Their Present State, Trade, and Debt
Parish, Woodbine, Sir
Argentina -- Description and travel; Argentina -- History
It seems, however, to have been assumed here that this iron, as a
matter of course, is meteoric, because it contains those admixtures of
nickel and cobalt which accompany other known meteoric productions.
It appears to me that the hypothesis is not very satisfactorily or
conclusively made out.
The mass I sent home weighs about 1400 pounds, and, making allowance
for what may have been taken from it at Buenos Ayres, may probably when
it arrived there have been not much less than a ton weight. Now De
Celis estimates the mass he examined to have been about fifteen tons
weight, and of much larger dimensions: either this therefore is only a
fragment of what he particularly described, or it is another which has
been found in the same part of the country, and if so, is corroborative
of the Indian accounts of there being more in the vicinity. This was
the opinion of Dr. Redhead, who, in writing to me on the subject, says,
"The native iron found in Santiago is not a single mass, as has been
said; there are several, and the most recent accounts describe them
as huge trunks with deep roots (I use the expression of the natives),
supposed to communicate with each other."[60]
Dr. Redhead's observation was caused by a discussion which arose here
upon some other specimens of native iron, which he had forwarded to me,
from the desert of Atacama, in Peru, and which were described by the
late Mr. Allan in the Transactions of the Royal Society of Edinburgh
for 1828. They were analysed by Dr. Turner, who found them to contain--
Iron . 93.4
Nickel ... 6.618
Cobalt . 0.535
-------
100.553
a result which he considered decisive concerning their origin, because,
he says, it differs from any compound hitherto described in the earth,
and corresponds exactly both in appearance and composition with other
meteoric iron.
But these opinions differ entirely from the belief of those who
procured the specimens.
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