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
Now if we would enquire how long it would require for a globe as large
as the earth to cool, we should find, after the preceding experiments,
that instead of 50,000 years, which Newton assigns for the earth to
cool to the present temperature, it would take 42,964 years, 221 days,
to cool only to the point where it would cease to burn, and 86,667
years and 132 days, to cool to the present temperature.
It might only be supposed, that the refrigeration of the earth should
be considerably increased, because we imagine that refrigeration
is performed by the contact of the air, and that there is a great
difference between the time of refrigeration in the air and in
vacuo; and supposing that the earth and air cool in the same time in
vacuo, this surplus of time should be reckoned. But, in fact, this
difference of time is very inconsiderable, for though the density of
the medium, in which a body cools, makes something on the duration of
the refrigeration, yet this effect is much less than might be imagined,
since in mercury, which is eleven thousand times denser than air, it
is only requisite to plunge bodies into it about nine times as often
as is required to produce the same refrigeration in air. The principal
cause of refrigeration is not, therefore, the contact of the ambient
medium, but the expansive force which animates the parts of heat and
fire, which drives them out of the bodies wherein they reside, and
impels them directly from the centre to the circumference.
By comparing the time employed in the preceding experiments to heat
the iron globes, with that requisite to cool them, we find that they
may be heated till they become white in one sixth part and a half of
the time they take to cool, so as to be held in the hand, and about
one fifteenth and a half of that to cool to actual temperature, so
that there is a great error in the estimate which Newton made on the
heat communicated by the sun to the comet of 1680, for that comet
having been exposed to the violent heat of the sun but a short time,
could receive it only in proportion thereto, and not only in so great
a degree as that author supposes. Indeed, in the passage alluded to,
he considers the heat of red-hot iron much less than in fact it is,
and he himself states it to be, in a Memoir, entitled, _The Scale of
Heat_, published in the Philosophical Transactions of 1701, which was
many years after the publication of his _principles_. We see in that
excellent Memoir, which includes the germ of all the ideas on which
thermometers have since been constructed; that Newton, after very exact
experiments, makes the heat of boiling water to be three times greater
than that of the sun in the height of summer; that of melted tin,
six times greater; that of melted lead, eight times; that of melted
regulus, twelve times; and that of a common culinary fire, sixteen or
seventeen times; hence we may conclude, that the heat of iron, when
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