Huygens, Christiaan
,
Christiani Hugenii opera varia; Bd. 2: Opera geometrica. Opera astronomica. Varia de optica
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DE CIRCULI MAGNIT. INVENTA.
"/>
oſtendendum eſt primò centrum gravitatis portionis A B di-
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ſtare à vertice B ultra punctum E; </
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<
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xml:space
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">nam, quod in diametro
<
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ſitum ſit, alibi oſtendimus. </
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<
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xml:space
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">Ducatur per E recta baſi paral-
<
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lela, quæ utrimque circumferentiæ occurrat in punctis F & </
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<
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G. </
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<
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xml:space
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">Per quæ ducantur K I, H L baſi A C ad angulos re-
<
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ctos, atque hæ cum ea, quæ portionem in vertice contingit,
<
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conſtituant rectangulum K L. </
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>
<
s
xml:id
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xml:space
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">Quoniam igitur portio ſemi-
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circulo minor eſt, conſtat rectanguli dicti dimidium F L con-
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tineri intra ſegmentum A F G C, atque inſuper ſpatia quæ-
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dam A F I, L G C. </
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<
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xml:space
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">Alterum vero rectanguli K L ſemiſſem
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K G complecti ſegmentum F B G unà cum ſpatiis F B K,
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B G H. </
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<
s
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xml:space
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">Quæ ſpatia quum ſint tota ſupra rectam F G, et-
<
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iam centrum commune gravitatis eorum ſupra eandem ſitum
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erit. </
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<
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xml:space
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">Eſt autem E punctum in ipſa F G centrum grav. </
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<
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xml:space
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">to-
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tius rectanguli K L. </
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<
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xml:space
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preserve
">Igitur ſpatii reliqui B F I L G B cen-
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trum grav. </
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<
s
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xml:space
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">erit infra rectam F G. </
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<
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xml:space
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<
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xml:space
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">ſpatiorum A F I,
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L G C commune gravitatis centrum eſt infra eandem F G.
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</
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<
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xml:space
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">Ergo magnitudinis ex ſpatiis hiſce & </
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<
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xml:space
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">dicto ſpatio B F I L G B
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compoſitæ, quæ eſt portio ipſa A B C, centrum gravitatis
<
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/>
infra lineam F G reperiri neceſſe eſt, ideoque infra E pun-
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ctum.</
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</
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<
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<
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xml:space
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">Eadem verò diameter B D ſecetur nunc in S, ita ut B S
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xml:space
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">TAB. XL.
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Fig. 3.</
note
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ſit ſeſquialtera reliquæ S D. </
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<
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xml:space
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">portionis
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A B C minus diſtare à vertice B quam punctum S. </
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<
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xml:space
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B D P totius circuli diameter. </
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xml:space
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">& </
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<
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">ducatur per S recta baſi
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parallela quæ circumferentiæ occurrat in F & </
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<
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">G. </
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xml:space
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">Et parabo-
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le intelligatur cujus vertex B, axis B D, rectum vero latus
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æquale S P. </
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<
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xml:space
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">Et occurat baſi portionis in H & </
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<
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xml:space
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igitur quadratum F S æquale eſt rectangulo B S P, hoc eſt,
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ei quod ſub B S & </
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<
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xml:space
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ea per F punctum, itemque per G. </
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<
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xml:space
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">Partes autem lineæ pa-
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rabolicæ B F, B G intra circumferentiam cadent, ſed reli-
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quæ F H, G K erunt exteriores. </
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<
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xml:space
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">Hoc enim oſtenditur du-
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ctâ inter B & </
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<
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xml:space
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">S ordinatim applicatâ N L, quæ circumfe-
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rentiæ occurrat in N, parabolæ autem in M. </
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<
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xml:space
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dratum N L æquale eſt rectangulo B L P, quadratum </
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