Huygens, Christiaan
,
Christiani Hugenii opera varia; Bd. 1: Opera mechanica
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HOROLOG. OSCILLATOR.
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ex B, centro circuli ſui, fit pendulum ipſi iſochronum {3 pr/4b},
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hoc eſt, trium quartarum rectæ, quæ ſit ad radium B F ut
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arcus C F D ad ſubtenſam C D. </
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<
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cognitis ſubcentricis cuneorum; </
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<
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">tum illius qui ſuper ſectore
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toto abſcinditur, plano ducto per B K parallelam ſubtenſæ
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C D, cujus cunei ſubcentricam ſuper B K invenimus eſſe
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{3/8} y
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- {3/8} a + {3 p r/8 b}, vocando a ſinum verſum E F; </
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<
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<
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">qui ſuper dimidio ſectore B F C abſcinditur plano per
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B F, cujus nempe cunei ſubcentricam ſuper B F invenimus
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{3/8} b - {3 b r/8 a} + {3 p r/8 a}.</
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">Sed & </
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<
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">alia via, ſectoris centrum oſcillationis, facilius in-
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<
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Fig. 6.</
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venitur, quæ eſt hujusmodi. </
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<
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pars minima ſector B C P, qui trianguli loco haberi poteſt.
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<
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">Quadrata autem, à diſtantiis particularum ejus à puncto B,
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æqualia ſunt quadratis diſtantiarum ab recta B R, bifariam
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ſectorem dividente, una cum quadratis diſtantiarum ab recta
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B Q, quæ ipſi B R eſt ad angulos rectos. </
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quadratorum ad illa, ratio quavis data eſt major, quoniam
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angulus C B P minimus; </
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ſunt.</
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">Poſitâ vero B O duarum tertiarum B R, hoc eſt, poſito
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O centro gravitatis trianguli B C P; </
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tarum B R: </
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">ut nempe N ſit centrum gravitatis cunei, ſu-
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per triangulo B C P abſciſſi plano per B Q. </
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<
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">His poſitis,
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conſtat quadrata, à diſtantiis particularum trianguli B C P
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ab recta B Q, æquari rectangulo N B O multiplici ſecun-
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dum particularum ejuſdem trianguli numerum. </
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<
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gulum N B O, ita multiplex, æquale cenſendum quadratis
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diſtantiarum à puncto B particularum trianguli B C P. </
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<
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autem quadrata diſtantiarum harum, ad quadrata diſtantia-
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rum totius ſectoris B C D, ſicut ſector B C P ad ſectorem
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B C D, hoc eſt, ſicut numerus particularum ſectoris B C P,
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ad numerum particularum ſectoris B C D; </
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<
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intelligitur, eo quod ſector B C D dividatur in ſectores qua-
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lis B C P. </
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