The Works of George Berkeley. Vol. 1 of 4: Philosophical Works, 1705-21Berkeley, George
Philosophy
The Works of George Berkeley. Vol. 1 of 4: Philosophical Works, 1705-21
Berkeley, George
Philosophy -- Early works to 1800
75. Many attempts have been made by learned men to account for this
appearance(362). Gassendus(363), Des Cartes(364), Hobbes(365), and several
others have employed their thoughts on that subject; but how fruitless and
unsatisfactory their endeavours have been is sufficiently shewn in the
_Philosophical Transactions_(366) (Numb. 187, p. 314), where you may see
their several opinions at large set forth and confuted, not without some
surprise at the gross blunders that ingenious men have been forced into by
endeavouring to reconcile this appearance with the ordinary principles of
optics(367). Since the writing of which there hath been published in the
_Transactions_ (Numb. 187, p. 323) another paper relating to the same
affair, by the celebrated Dr. Wallis, wherein he attempts to account for
that phenomenon; which, though it seems not to contain anything new, or
different from what had been said before by others, I shall nevertheless
consider in this place.
76. His opinion, in short, is this:—We judge not of the magnitude of an
object by the optic angle alone, but by the optic angle in conjunction
with the distance. Hence, though the angle remain the same, or even become
less, yet, if withal the distance seem to have been increased, the object
shall appear greater. Now, one way whereby we estimate the distance of
anything is by the number and extent of the intermediate objects. When
therefore the moon is seen in the horizon, the variety of fields, houses,
&c. together with the large prospect of the wide extended land or sea that
lies between the eye and the utmost limb of the horizon, suggest unto the
mind the idea of greater distance, and consequently magnify the
appearance. And this, according to Dr. Wallis, is the true account of the
extraordinary largeness attributed by the mind to the horizontal moon, at
a time when the angle subtended by its diameter is not one jot greater
than it used to be.
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