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

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              <s id="s.001522">
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              adhûc pars AS, ſubdiuidi in plura, pluraque dimidia.
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              </s>
              <s id="s.001523">Deinde, cùm in dimidio SD, tot requiris parteis, vt
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              ex ipſis ratio accelerati motus perfectè intelligatur:
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              quot­
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              nam quæſo ſunt, quas requiris? </s>
              <s id="s.001524">An aliquot pauculas,
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              v. c. ſex, quas nempe recenſes, dum rationem motus
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              accelerati explicas per trientem, quadrantem, per quin­
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              tam, perque ſextam parteis tantum? </s>
              <s id="s.001525">Sanè vel neſciens
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              tot requiris, vt innumerabiles ſint; & tum abſis longiſ­
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              ſimè ab eo, vt cauſſeris ſtandum, quòd
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              diuiſio eſſe infinita
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              non poßit,
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              quaſi vel in fine, vel certe non longè à fine
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              conſiſtendum ſit: tum etiam ab eo, vt ex cognitis par­
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              tibus
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              ratio motus intelligatur.
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              </s>
              <s id="s.001526"> Rem vt experiamur, ac­
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              cipiamus, ecce, caſum globi ferrei (quod tuum poſteà
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              exemplum eſt) ex cælo Lunæ in centrum terræ: atque
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              in ipſo talem partem,
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              in qua iam primum,
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              vt ais,
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              conſiſta­
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              mus.
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              Cùm tuo ex decreto, menſura durationis om­
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              nium partium iſti primæ æqualium ſit æqualis duratio
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              totidem minutiorum partium ſigillatim acceptarum
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              in inferiore eius dimidio: ergo inferius eius dimidium
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              diuiſibile eſt in tot parteis, non Mathematicas, men­
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              teve confictas, ſed Phyſicas, ſiue in ipſa rerum natura
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              exſiſtenteis, quot partes ſunt à cælo Lunæ, vſque in
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              centrum terræ, ipſi AD æquales. </s>
              <s id="s.001527">Hæ verò partes quot­
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              nam ſunt? </s>
              <s id="s.001528">Certè, cùm aſſumendo pedes (vt facis) pro
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              Galilei cubitis, admittas à Luna in centrum nonagies
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              octies mille myriadas pedum: oportebit, etiam ſi pri­
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              mam partem AD, non minorem pede habeas, vt di­
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              cas dimidium illius inferius, ſeu ſemi-pedem totidem
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              pati diuiſiones, & continere totidem parteis Phyſicas
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              non mente confictas. </s>
              <s id="s.001529">Quid verò ſi acceperis partem </s>
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