Gassendi, Pierre, De proportione qua gravia decidentia accelerantur, 1646

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              <s id="s.000664">
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              idcirco eodem, quo DE. </s>
              <s id="s.000665">Et quia ſeruatâ analogià
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              PS percurri debet vno minuto cum triente, efficie­
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              tur, vt non modò SD, verùm ipſa quoque DE per­
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              curratur rursùs non duobus minutis, ſed vnoſolùm
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              cum triente; atque ita bifariam ſecando, diminuendo­
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              que in infinitum. </s>
              <s id="s.000666">Adnoto deinde non tranſire te
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              vltrà comparationem partis DE cum parte SD, ne­
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              que comparare ipſam cum parte PS, vt mox factum
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              eſt, & fieri poſſe nihil prohibet; cùm nulla ſit ratio,
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              ob
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              in hac potiùs biſectione,
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              in vlteriore vlla
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              conſiſtatur; verùm aſſumere te ſolum, id
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              tempus, quo
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              abſoluitur interuallum
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              SD
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              breuius eſſe tempore, quo pars
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              ſuperior
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              AS
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              tranſcurritur, alioquin deſcenſus ſine accelera­
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              tione vniformis eſſet;
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              idque, vt inferas,
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              partem primùm
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              deſignatam
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              DE,
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              cum eodem præcisè tempore percurratur,
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              quo interuallum
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              SD,
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              non in dimidio prioris temporis, ſed
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              tempore breuiore abſolui.
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              <s id="s.000667"> Adnoto, inquam, vt appareat,
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              cui fundamento ſuper-exſtruas quicquid deinceps
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              ædificas, ſupponens nimirùm vt ratum principium
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              (quod obiter, & aliud agendo ſtabilieris) æqualita­
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              tem temporis, quo pars SD, & ipſius dupla DE per­
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              curruntur. </s>
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              DeTempore, quo R. P. colligit ſingulas parteis decur ſumiri.
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              <s id="s.000669">XXXIV. </s>
              <s id="s.000670">Etenim illicò ſic habes;
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              Sed ex his,
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              & eadem prorſus ratione aliud demonstratur, quod ingentis,
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              atque admirabilis paradoxi loco non immeritò fortaßis habe­
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              ri poßit, nempe ſi spatium, per quod corpus graue quod­
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              cumque deſcendit, in parteis quotlibet æqualeis diuiſum intel­
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              ligatur, & primæ, ac ſupremæ partis etiam deſignetur
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