Illustrations of the Huttonian Theory of the EarthPlayfair, John
Science
Illustrations of the Huttonian Theory of the Earth
Playfair, John
Geology; Hutton, James, 1726-1797. Theory of the earth
[Footnote 192: Geol. Essays, p. 441.]
The appeal made here to Frisi is singularly unfortunate, as that
philosopher has demonstrated the very contrary of Mr Kirwan's
position, and has proved, that the disturbance given to the diurnal
motion by the causes here referred to may be real, but cannot be
perceptible. Having investigated a formula expressing the law which
all such disturbances must necessarily observe, he concludes, "Hàc
autem formulâ manifestum fiet, ex iis omnibus variationibus quæ in
terrestri superficie observari solent, montium et collium abrasione,
dilapsu corporum ponderosiorum in inferiores telluris sinus, nullam
oriri posse variationem _sensibilem_ diurni motûs. Nam si statuamus
data aliqua annorum periodo terrestrem superficiem ad duos usque pedes
abradi undique, eam vero materiæ quantitatem ad profunditatem pedum
1000 dilabi; erit omne quod inde orietur incrementum velocitatis diurni
motûs 30000/(19638051)^2 = 1/12855068184."[193]
[Footnote 193: Frisii Opera, tom. iii. p. 269.]
Here, it is evident, that Frisi admits those very changes on the
surface which we are contending for, and shows, that their tendency is
to accelerate the earth's diurnal motion, but, by a quantity so small,
that, in a space of time amounting at least to 200 years, the increase
of the diurnal motion would only be such a part of the whole as the
preceding fraction is of unity.[194]
[Footnote 194: The time requisite for taking away by waste and erosion
two feet from the surface of all our continents, and depositing it at
the bottom of the sea, cannot be reckoned less than 200 years. The
fraction 1/12855068184, reduced to parts of a day, is 1/148554 of a
second; so that it would require 200 years to shorten the length of
the day, by the above fraction of a second; and therefore it would
require 148554 times 200 years, or 29710800 years, to diminish it an
entire second. The accumulated effect, however, of all the diminutions
during that period, would amount to much more: and if we had any
perfectly uniform standard to compare the motion of the earth with,
its difference from that standard would increase as the squares of the
time, and the total acceleration would amount to one second in 77080
years. Whatever relation this bears to the age of the globe itself, it
exceeds more than ten times the age of any historical record.
Public-domain text, read in full here on John Shaqi.
Reviews
Reviews
No reviews yet
Be the first to share your thoughts on this work.
Elsewhere in the archive
Join the Discussion
Join the discussion
Sign in to leave a comment or review.
Sign InorCreate an account