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

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              <s id="s.002194">
                <pb pagenum="295" xlink:href="028/01/335.jpg"/>
              rum cum ſemiſſe: tertiæ duorum: quartæ vnius, ac ſe­
                <lb/>
              miſſis: quintæ vnius: ſextæ ſemiſſis: deduxi exinde ſin­
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              gularum diſculos: eoſque in vnum componendo, com­
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              parandóque ad diſcum Solis, cuius diameter, vt iam
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              dictum eſt, ſit dimidii gradus, ſiue minutorum triginta,
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              collegi debere ex iis diſcum fieri, cuius diameter ſit
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              minutorum quinquaginta, & vnius; quique ſit proinde
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              ad diſcum Solarem, vt ad nouem, viginti ſex, ſeu pro­
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              ximè triplus. </s>
              <s id="s.002195">Et quia tamen harum Stellarum, non­
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              niſi dimidium horizonti conſpicuum eſt; facile fuit
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              agnoſcere diſcum ex iſto dimidio eſſe Solaris ſeſqui­
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              alterum, ſiue exæquari Soli ſemel cum ſemiſſe. </s>
              <s id="s.002196">Quare
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              & deprehendi me non abſque ratione admiratum fuiſ­
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              ſe, quamobrem, ſi diſci Stellarum tanti ſint, quanti &
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              apparent, & eſſe dicuntur; Terra ex iis noctu non ma­
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              gis reſplendeat. </s>
              <s id="s.002197">Subinde verò, quia tantas non eſſe dia­
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              metros Stellarum perſpectum
                <expan abbr="habebã">habebam</expan>
              (quippe minores
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              etiam ducebam, quàm Galileus cenſuerit, quòd in no­
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              cturnis tenebris pupillæ
                <expan abbr="dilatationẽ">dilatationem</expan>
              maiorem
                <expan abbr="cẽſerem">cenſerem</expan>
              ,
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              quàm ſuppoſitum ab eo videretur) ideò explorare rem
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              placuit iuxta veriores diametros, quales videlicet appa­
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              rent reſectâ non tam teleſcopio, quàm funiculo, aut ba­
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              cillo tereti interpoſito, circumradiatione. </s>
              <s id="s.002198">Et ne videret
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              tamen mihi potiùs, quàm Galileo fidere: ſupponere
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              volui, quod is obſeruanit, Stellam magnitudinis pri­
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              mæ eſſe diametri ſecundorum quinque, ſiue tertiorum
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              trecentorum; & conſequenter habere Stellam ſecundæ
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              magnitudinis diametrum tertiorum ducentorum quin­
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              quaginta: tertiæ ducentorum: quartæ centum quin­
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              quaginta: quintæ centum: ſextæ quinquaginta. </s>
              <s id="s.002199">Hoc </s>
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