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
“Distantiam præterea discimus, per mutuam quandam conspirationem oculorum.
Ut enim cæcus noster duo bacilla tenens, _A E_ et _C E_, de quorum
longitudine incertus, solumque intervallum manuum _A_ et _C_, cum
magnitudine angulorum _A C E_, et _C A E_ exploratum habens, inde, ut ex
Geometria quadam omnibus innata, scire potest ubi sit punctum _E_. Sic
quum nostri oculi _R S T_ et _r s t_ ambo, vertuntur ad _X_, magnitudo
lineæ _S s_, et angulorum _X S s_ et _X s S_, certos nos reddunt ubi sit
punctum _X_. Et idem opera alterutrius possumus indagare, loco illum
movendo, ut si versus _X_ illum semper dirigentes, prime sistamus in
puncto _S_, et statim post in puncto _s_, hoc sufficiet ut magnitudo lineæ
_S s_, et duorum angulorum _X S s_ et _X s S_ nostræ imaginationi simul
occurrant, et distantiam puncti _X_ nos edoceant: idque per actionem
mentis, quæ licet simplex judicium esse videatur, ratiocinationem tamen
quandam involutam habet, similem illi, qua Geometræ per duas stationes
diversas, loca inaccessa dimetiuntur.”
[Illustration]
I might amass together citations from several authors to the same purpose,
but, this being so clear in the point, and from an author of so great
note, I shall not trouble the reader with any more. What I have said on
this head was not for the sake of rinding fault with other men; but,
because I judged it necessary to demonstrate in the first place that we
neither see distance _immediately_, nor yet perceive it by the mediation
of anything that hath (as lines and angles) a _necessary_ connexion with
it. For on the demonstration of this point the whole theory depends(461).
_Secondly_, it is objected, that the explication I give of the appearance
of the horizontal moon (which may also be applied to the sun) is the same
that Gassendus had given before. I answer, there is indeed mention made of
the grossness of the atmosphere in both; but then the methods wherein it
is applied to solve the phenomenon are widely different, as will be
evident to whoever shall compare what I have said on this subject with the
following words of Gassendus:—
Public-domain text, read in full here on John Shaqi.
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