Buffon's Natural History. Volume 10 (of 10): Containing a Theory of the Earth, a General History of Man, of the Brute Creation, and of Vegetables, Minerals, &c. &cBuffon, Georges Louis Leclerc, comte de
History
Buffon's Natural History. Volume 10 (of 10): Containing a Theory of the Earth, a General History of Man, of the Brute Creation, and of Vegetables, Minerals, &c. &c
Buffon, Georges Louis Leclerc, comte de
Natural history
easily distinguished at a mile distance, when the rays of the sun shine
on him, and by suppressing the intermediate light which surrounds us,
and darkening our sight, we should see him at least ten times farther;
that is to say, ten miles. Ships, therefore, being much larger, would
be seen as far as the curvature of the earth would permit, without any
other instrument than the naked eye.
[H] Aristotle is, I believe, the first that ever mentioned this
observation.
But a concave mirror, of a great diameter, and of any focus, placed at
the end of a long black tube, would have nearly the same effect as our
great objective glasses of the same diameter and form would have during
the night, and it was probably one of these concave mirrors of polished
steel that was established at the port of Alexandria[I]. If this steel
mirror did really exist, we cannot refuse to the ancients the glory
of the first invention, for this mirror can only be effective by as
much as the light reflected by its surface was collected by another
concave mirror placed at its focus, and in this consists the essence
of the telescope and the merit of its construction. Nevertheless this
does not deprive the great Newton of any glory, who first renewed the
almost-forgotten invention. As the rays of light are by their nature
differently refrangible, he was inclined to think there were no means
of correcting this effect, or, if he had perceived those means, he
judged them so difficult that he chose rather to turn his views another
way, and produce, by means of the reflection of the rays, the great
effects which he could not obtain by their refraction; he, therefore,
constructed his telescope, the reflection of which is infinitely
superior to those that were in common use. The best telescopes are
always dark in comparison of the acromatic, and this obscurity does not
proceed only from the defect of the polish, or the colour of the metal
of mirrors, but from the nature even of light, the rays of which being
differently refrangible are also differently reflexible, although in
much less unequal degrees.
[I] From time immemorial the Chinese, and particularly the Japanese,
have possessed the art of working in steel both in large and small
bodies; and hence I have thought that the words _e ferro sinico_ in the
preceding quotation should be understood as applying to polished steel.
It still remains, therefore, to bring the telescope to perfection, and
to find the manner of compensating this different reflexibility, as we
have discovered that of compensating the different refrangibility.
Public-domain text, read in full here on John Shaqi.
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