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

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            <p type="main">
              <s id="s.000159">
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              parti, non ab Authore fuit delectum, ſed
                <expan abbr="ſuppeditatũ">ſuppeditatum</expan>
              à R. P.
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              qui tametſi alicubi non probet ex ijs ſex minutis quatuor priori
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              dimidio, & duo poſteriori attribui: id tamen tum ex varijs
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              eius principijs deducitur: tum recipit Author deducturum ſe
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              eadem, & plura incommoda, ex quacumque alia diſtributione
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              eius numeri, aut alterius à R. P. facienda: ſi modò ſemper
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              velocitates habere ſe vt spatia ſupponat.
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              A p. </s>
              <s id="s.000160">181. in 191. </s>
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              <s id="s.000161">ART. XXXIX. XL. XLI. XLII.
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              </s>
              <s id="s.000162">De Ratione continuò dupla, qua ſpatia de­
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              curri temporibus æqualibus R. P. contendit. </s>
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              <s id="s.000163">
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              Mirum, velle adhûc R. P. incipere acceleratum motum
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              à primæ partis medio, non ab ipſo eius principio; & maximè
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              quidem, cùm aliunde velit velocitates eſſe vt spatia, spatiive
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              parteis, quarum vna ſit tota prima, non dimidium primæ: ac
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              inſignes prætereà ſuboriantur difficultates ex eo, quòd dum
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              ad obiecta de ſubdiuiſione prioris dimidij in alia, aliaque dimi­
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              dia reſpondet, standum ait alicubi, quòd diuiſio eſſe in Phy­
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              ſicas parteis infinita non valeat, & ibi tamen standum, vbi
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              tot partes adhûc ſuperſunt, vt ex ijs ratio accelerati motus
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              perfectè intelligatur. </s>
              <s id="s.000164">Quippe cùm inter cætera aſſumpto
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              caſu ex Luna, Sole, aut Firmamento, & aſſumpta particula
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              prima Phyſicè diuidua, in qua reperiri debeant dimidium
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              inferius, ac in ipſo triens, quadrans, & tot fragmenta cætera,
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              quot ſunt partes ipſi primæ æquales in toto illo ſpatio, quotque
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              etiam diſtingui poßunt in ſuperiore dimidio; incredibilis ſit
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              partium numerus, per quas in priore dimidio contentas opor­
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              teat motum peragi, priuſquam incipiat accelerari; & in qui­
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              bus tamen conſiſtendum ſit, quòd diuiſio vlteriùs fieri in duo
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              </s>
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