Ceva, Giovanni
,
Geometria motus
,
1692
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Scholium.
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Cum prorsùs geometricè oſtenderimus ſuperiores duas pro
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poſitiones, vtiliſſimum eſt obſeruare, quomodo liceat vti tem
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poris inſtantibus, non vt punctis prorsùs geometricis, ſed vt
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quantitatibus dicam minoribus quibuſcunque datis. </
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oritur indiuiſibilium methodus, quæ intelligentiam affert
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faciliorem, ac ſi rigori geometrico penitus inſiſteremus, quam
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quam eæ tamen difficiliores Geometras mihi magis decerę
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videantur.
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PROP. III. THEOR. III.
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Tab.
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2,
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Fig.
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1.</
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">SPatia, quæ curruntur iuxta quaslibet homogeneas ve
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locitatum imagines, nectuntur ex rationibus tempo
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rum, ac æquatricum. </
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gines velocitatum ſint ABCD, EFHI ponantur AG, EL.
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porum AD ad EI; & ex ea æquatricum AE ad EL. </
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ſi motus, qui eſt iuxta imaginem ABCD perſeueret velo
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citate AG, eſſet quidem æquabilis, idemque ſpatium illa </
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velocitate, & tempore AD percurreretur, ac ſecundùm̨
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imaginem ABCD; Itaque exiſtente rectangulo DE, quod
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eſset imago velocitatum illius motus æquabilis, foret idem
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æquale imagini ABCD (nam imagines ABCD, & DG
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homogeneæ ſunt) eodem modo imago rectangulum VL
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æquale eſset imagini EFHI. </
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<
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">Cum ergo duæ imagines re
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ctangula DE, IL componantur ex rationibus temporum
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AD ad EI, & ex ea æquatricum AG ad EL; ex ijſdem̨
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prorsùs rationibus etiam imagines propoſitæ prædictis re
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ctangulis æquales nectentur. </
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ſitis imaginibus tranſiguntur, quæque ipſis proportionalia </
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