Benedetti, Giovanni Battista de
,
Io. Baptistae Benedicti ... Diversarvm specvlationvm mathematicarum, et physicarum liber : quarum seriem sequens pagina indicabit ; [annotated and critiqued by Guidobaldo Del Monte]
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DISPVTATIO NES.
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0207
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tarium è contrà ſe habeat, præter id,
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nunquam fuit neque ſit futurus aliquis
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horum
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rectorum, qui naturales dicuntur, qui tam velociter moueatur, ut motus cœli, quia ſi
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voluerimus conſiderare motum diurnum .24. horarum, ſecundum opinionem com-
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munem, reperiemus calculando, Lunam in quadraturis cum Sole, dum inuenitur in
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æquatore, ſingulis horarum minutis moueri per .500. milliaria Italica vel circa, & in
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coniunctionibus, & oppoſitionibus ipſius Solis .1000. vel circa, & Solem tempore
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quinoctiorũ</
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.18000. &
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circa æquatoris
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.260000. &
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de ſtellis
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fixis circa æquatorem poſitis quiuis cogitet; </
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<
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xml:space
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">quod reuera diffi cillimum quibuſdam
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videbitur, quod quidem non occurrit
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pulcherrimam Ariſtarchi ſamij opi-
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nionem, diuinitus à Nicolao Copernico expreſſam, contra quam nil planè valent
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rationes ab Ariſtotele; </
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">neque etiam à Ptolomeo propoſitę. </
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">Motu verò proprio, quo
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libet horę minuto, Sol
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per milliaria circa .48. </
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eſt, aut op
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poſita reperitur Soli .36. milliaria, & in quadraturis .18. Saturnus .24. Iupiter .40:
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Mars .100: Venus .26: Mercur .5. </
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uet̃</
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circa .260000. milliaria, vt diximus Iupiter circa .170000. Mars .75000. Venus.
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10000, Mercurius .2000. corpus
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elementare, & ſi
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motu recto hoc
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,
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& velocius etiam corpore cęleſti, non obſeruans
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uniformitatem, ut dictum cœ
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leſte facit, cum eodem nullo modo comparari poſſet, quia rectus dictus naturalis,
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ſuam ſemper velocitatem adauget, ob continuam impreſſionem, quam recipit à cau
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ſa perpetuò coniuncta cum ipſo corpore, quę eſt propenſio illa naturalis eundi bre-
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uiori quadam via ad locum ſuum, ita vt etiam ſi dictum corpus elementare à motu
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tardiore ad velociorem, ſuperare poſſet
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alicuius corporis cęleſtis, ij duo motus
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interſecarent ſeſe in vno ſolo
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, quod diuidi
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in partes nequiret, ideſt
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non niſi in vno ſolo temporis inſtanti redderentur æquales, vt ita dicam. </
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loquor de circulari cœleſti cum recto elementari, ſed de qualibet alia motuum ſpe-
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cie, ſiue ſint ambo recti, ſiue ambo curui, quando aliquis eorum irregularis erit.</
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">Minus ſufficienter exploſam fuiſſe ab Ariſtotele opinionem cre-
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dentium plures mundos exiſtere.</
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">MAior ratio, qua Ariſtoteles eorum opinionem, qui plures eſſe mundos dixe
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runt, refutare nititur, in eo conſiſtit, quod is credat partes terræ, quæ alijs
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mundis aſſignarentur, ad huius mundi centrum inclinationem habere, & ſic ignem
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illorum, propenſionem habiturum ad circunferentiam huius.</
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<
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">Quæ certè ratio tam debilis eſt, vt per ſe cadat, non conſideransipſe, quòd ſi
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eſſent dicti mundi, eorum quilibet ſuum proprium centrum,
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propriam cir-
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cunferentiam haberet,
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& ignes haberent inclinationem ad centra circunfe-
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ſuorum mundorum, abſque eo,
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vna terra, alterius centrum appeteret; </
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exempli gratia, ſi doctiſſimi Ariſtarchi opinio eſt vera, rationi
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conſentaneum
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erit maximè, vt quod Lunæ contingit, cuilibet
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ex aliis quinque planetis eue-
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niat, ideſt, vt quemadmodum Luna ſuorum epicyclorum ope
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terram voluitur,
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quaſi per circunferentiam alterius cuiuſdam epicycli, in quo terra ſit inſtar centri
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naturalis (ideſt ſit in medio) delati ab orbe annuo circa Solem; </
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Iupiter, Mars, Venus, atque Mercurius, cir cum aliquod corpus in medio ſui epici- </
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