Stevin, Simon
,
Mathematicorum hypomnematum... : T. 4: De Statica : cum appendice et additamentis
,
1605
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L*IBER* S*TATICÆ*
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<
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xml:space
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<
s
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xml:space
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">Videtur Archimedes, @altero horum modorum problematis hujus inventionens
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aſſecutus, ut dum aut parabolici ſui ſpeculi exemplar fabricatur, aut alterius gratia pa-
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rabolam ſolidam, boc eſt conoïdale rectangulum efformat, reapſe edoctus ſit, ſegmentums
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vertici co nterminum reliqui eſſe ſeſquialterum, in cujus cauſam hâc viâ inquiſierit & </
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quaſi inſpexerit: </
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<
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xml:space
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">Cum ambæ B A I, B A C parabolæ ſint, diametros I F, A D àgra-
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vitatis centris in homologa ſegmenta per 11 propoſ. </
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<
s
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xml:space
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">ſecari neceſſe erit, ideo{q́ue} I L, L F,
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hoc eſt O N, N H ipſis æquales, rectis A E, E D proportionales erunt: </
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<
s
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xml:space
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">ſed ſi N com-
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mune utriuſque par abolicæ portionis gravitatis centrum foret, P verò centrum trian-
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guli A B C, quia triangulum ſimulutriuſque portionis eſt triplum, etiam jugum N E
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jugi E P quoque triplum erit. </
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<
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xml:space
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">Vnde propoſitio iſtiuſmodi exiſtit. </
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">Invenire duo puncta
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N, E, quæ ſegmentorum O N, N H rationem faciant eandem quam A E habet
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ad E D. </
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<
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xml:space
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">aſſumpta deinde A E {3/5} totius A D, & </
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<
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">E D {2/5}, facto{q́ue} periculo, quid ex his dedu-
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catur; </
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<
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xml:space
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">tandem iſtudipſum veritati congruere comperit. </
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<
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xml:space
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">Aut ſi coniectur â huius ſeſ-
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quialteræ rationis id ipſum aſſecutus non ſit, verùm arte duce in hæc penetralia pene-
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traverit, videtur numeris hæc primùm expertus: </
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">Dati duo numeri O H {1/4}, H P {1/6} am-
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bo ita dividuntor, ut minus ſegmentum rectæ O H cum majore ipſius H P, tri-
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plum ſit ſegmenti minoris rectæ H P cum majore ipſius H O, ea lege ut majus
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ſegmentum rectæ O H ad minus habeat rationem, quam majus ſegmentum
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H P + {1/3} habet ad minus ſegmentum H P + {1/3}.</
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">Datâ parabolâ curtâ, gravitatis centrum invenire.</
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<
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biſecat diameter E F. </
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xml:space
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">Parabolam curtam abſolvito, defectu A B G addito, hinc G E ſecetur in
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H ut ſegmentum G H vertici vicinum reliqui H E ſit ſeſquialterum, itemq́uc
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G I ipſius I F; </
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<
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xml:space
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">denique fiat ut A B C D ad A B G ſic H I ad I K: </
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optatu m gravitatis centrum eſſe.</
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trum eſt I, & </
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eſt H I ad I K ut parabola curta ad
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dictam portionem, K curtæ parabolæ
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centrum erit.</
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tuit, curtæ parabolæ centrum gravita-
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tis invenimus, Generaliter autem ſive
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A B parallela ſit contra D C, ſive an-
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nuat ita efficies. </
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<
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">inveniatur H centrum
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gravitatis parabolæ A G B & </
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<
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xml:space
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">I centrum totius D G C quæ connectantur ju-
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go H I & </
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<
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xml:space
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">fiat H I ad continuationem I K ſicut parabola curta A B C D ad
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complementum ſui A G B. </
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<
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xml:space
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">utriuſque autem ratio ad rectilineas figuras revo-
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cari poteſt, cum utraque D G C, A G B trianguli quæ ipſis & </
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<
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dinem habet æqualem ſeſquitertia ſit; </
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<
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no congruet.</
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