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

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              <s id="s.002199">
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              autem poſito, Stellarum mille viginti duarum diſculos
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              in diſcum vnum compoſui, ipſumque ad diſcum Solis
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              comparando, comperi non eſſe, niſi illius particulam
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                <expan abbr="quadringẽteſimam">quadringenteſimam</expan>
              trigeſimam vnam: ac proinde, dia­
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              metro Solis exſiſtente minutorum triginta, ratiocina­
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              tus ſum diametrum diſci ex omnibus Stellis compoſiti,
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              non eſſe maiorem vno minuto cum ſemiſſe; quantæ
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              vulgò eſſe apparet Stella magnitudinis quartæ. </s>
              <s id="s.002200">Quod
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              ſi dimidium detrahas, ob Stellas, quæ ſub horizonte:
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              ſequitur diſcum ex reſiduis, non fore maiorem vna
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              octingenteſima ſexageſima tertia diſci Solaris particu­
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              la: ac eius diametrum futuram vnius proximè minuti
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              dumtaxat: hoc eſt, quantæ eſſe apparet Stella magni­
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              tudinis quintæ. </s>
              <s id="s.002201">Quare & ex hoc deſii admirari, quam­
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              obrem lux omnium Stellarum ſupra horizontem lu­
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              centium tam parum Terræ faciem illuſtrent; tuque ex­
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              inde animaduertis quo progreſſu peruenerim ad in­
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              credibile fig mentum. </s>
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              <s id="s.002202">XXXVI. </s>
              <s id="s.002203">At verò, inquies, ecquiſ-nam capiat non
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              eſſe ingens totum maius tantulâ ſui particulâ: ſeu tan­
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              tam, quæ apparet lucem in omnibus Stellis ſupra hori­
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              zontem coruſcantibus, in exiguum adeò ſpatium con­
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              trahi, vt non ſit eo maius, quod à ſtellula magnitudinis
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              quintæ occupatur? </s>
              <s id="s.002204">Sed nimirùm conſidera; ſi foret
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              Stella, quæ reuerâ eſſet diametro minuti vnius, fore, vt
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              lux eius ſpectata intra nocturnas tenebras appareret
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              oculo incompa biliter maior. </s>
              <s id="s.002205">Si enim quæ Stella eſt
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              diametro ſolùm vnius ſecundi cum beſſe: apparet ni­
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              hilominùs diametro vnius minuti: ſanè, ſi proportio­
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              nem admittas, ea apparitura erit diametro minutorum </s>
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