Huygens, Christiaan
,
Christiani Hugenii opera varia; Bd. 1: Opera mechanica
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HOROLOG. OSCILLATOR.
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F A, dabit diſtantiam A K, qua centrum oſcillationis K in-
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ferius eſt centro gravitatis A.</
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<
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">Si vero F A ſit axis figuræ B C D, poteſt, pro cuneo
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Fig. 1.</
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abſciſſo per B D ſuper figura tota, adhiberi cuneus ſuper
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figura dimidia D B M abſciſſus plano per D M. </
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hujus ſubcentrica ſuper D M ſit O A, diſtantia vero centri gr.
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<
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">figuræ planæ D B M ab eadem D M ſit N A, æquale eſſe
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conſtat rectangulum O A N rectangulo B A L . </
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huj.</
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rectangulum O A N, additum rectangulo D A H, conſti-
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tuet quoque planum applicandum ad diſtantiam F A, ut
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fiat diſtantia A K.</
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<
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">Et horum quidem manifeſta eſt demonſtratio ex præce-
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dentibus, quippe cum rectangula D A H, B A L, vel
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D A H, O A N, multiplicia ſecundum numerum particu-
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larum figuræ, æqualia ſint quadratis diſtantiarum à centro
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gravitatis A; </
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">ſive, quod idem hic eſt, ab axe gravitatis axi
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oſcillationis parallelo; </
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tiam F A applicata, efficiant longitudinem intervalli A K .</
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huj.</
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">Et in circulo quidem rectangula D A H, B A L, inter
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ſe æqualia eſſe liquet, ſimulque efficere ſemiſſem quadrati à
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ſemidiametro. </
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<
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">Unde, ſi fiat ut F A ad ſemidiametrum A B,
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ita hæc ad aliam, ejus dimidium erit diſtantia A K, à cen-
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tro gravitatis ad centrum oſcillationis. </
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<
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axe D, in circumferentia ſumpto, agitetur, erit D K æqua-
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lis tribus quartis diametri D M.</
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ſcillationis quæſivimus, quæ ſimpliciter adſcripſiſſe ſufficiet-
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Nempe,</
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">In rectangulo omni, ut C B, ſpatium applicandum, ſive
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Fig. 3.</
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rectangulum oſcillationis, invenitur æquale tertiæ parti qua-
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drati à ſemidiagonio A C. </
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