Gassendi, Pierre
,
De proportione qua gravia decidentia accelerantur
,
1646
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parti, non ab Authore fuit delectum, ſed
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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. </
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curri temporibus æqualibus R. P. contendit. </
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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. </
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<
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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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