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
66. We are nevertheless exceedingly prone to imagine those things which
are perceived only by the mediation of others to be themselves the
immediate objects of sight, or at least to have in their own nature a
fitness to be suggested by them before ever they had been experienced to
coexist with them. From which prejudice every one perhaps will not find it
easy to emancipate himself, by any the clearest convictions of reason. And
there are some grounds to think that, if there was one only invariable and
universal language in the world, and that men were born with the faculty
of speaking it, it would be the opinion of some, that the ideas in other
men’s minds were properly perceived by the ear, or had at least a
necessary and inseparable tie with the sounds that were affixed to them.
All which seems to arise from want of a due application of our discerning
faculty, thereby to discriminate between the ideas that are in our
understandings, and consider them apart from each other; which would
preserve us from confounding those that are different, and make us see
what ideas do, and what do not, include or imply this or that other
idea(355).
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67. There is a celebrated phenomenon(356) the solution whereof I shall
attempt to give, by the principles that have been laid down, in reference
to the manner wherein we apprehend by sight the magnitude of objects.—The
apparent magnitude of the moon, when placed in the horizon, is much
greater than when it is in the meridian, though the angle under which the
diameter of the moon is seen be not observed greater in the former case
than in the latter; and the horizontal moon doth not constantly appear of
the same bigness, but at some times seemeth far greater than at others.
68. Now, in order to explain the reason of the moon’s appearing greater
than ordinary in the horizon, it must be observed that the particles which
compose our atmosphere do intercept the rays of light proceeding from any
object to the eye; and, by how much the greater is the portion of
atmosphere interjacent between the object and the eye, by so much the more
are the rays intercepted, and, by consequence, the appearance of the
object rendered more faint—every object appearing more vigorous or more
faint in proportion as it sendeth more or fewer rays into the eye. Now,
between the eye and the moon when situated in the horizon there lies a far
greater quantity of atmosphere than there does when the moon is in the
meridian. Whence it comes to pass, that the appearance of the horizontal
moon is fainter, and therefore, by sect. 56, it should be thought bigger
in that situation than in the meridian, or in any other elevation above
the horizon.
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