Gassendi, Pierre
,
De proportione qua gravia decidentia accelerantur
,
1646
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denique gradus exilitatis, quo propter hanc imminu
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tionem Stellæ Fixæ exhibentur incomparabiliter mi
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nores Planetis, habita ratione diſcorum apparentium:
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ſcilicet, quòd ipſarum radii & excurrant longè vberiùs,
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& longè proinde ampliùs circum-radient. </
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<
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<
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commemoro, vt innuam, Qua ratione Sol è Fixis ſpe
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ctatus, tametſi ſuo diſco exilis, appariturus tamen foret
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luce adeò circum-diffuſa, vt, tanquam ſpatia in
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gentia complens, apparenter exæquaretur, aut to
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ti, aut ſaltem inſigni portioni regionis Planetariæ,
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cuiuſmodi eſt Orbis magnus, de quo fuit potiſſimùm
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quæſtio. </
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<
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">Et fac certè Solem non apparere maiorem,
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quàm magnitudinis ſextæ Stellam: quia tunc vera dia
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meter eius erit vno ſecundo minor, hoc eſt, ex iam di
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ctis, tertiorum quinquaginta; orbis magni diameter
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continebit ducenties, aut plus paulò certè, quinqua
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ginta tertia (quippe totidem vicibus diametrum Solis
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continet) efficietur, ſi ea reducas, vt Orbis magni dia
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meter apparitura non ſit maior duobus minutis cum
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dodrante, ſeu quàm appareat diameter Stellæ magni
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tudinis primæ, aut ſecundæ. </
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<
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metri ſint adhûc minores, quàm Galileus cenſuit, ob
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inſinuatam antè cauſſam; & magnitudinis ſextæ Stella
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non ſit maior diametro, quàm ſextans ſecundi, ſiue
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decem tertia; efficietur eadem ratione, vt Orbis magni
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diameter apparitura maior non ſit, quàm appareat dia
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meter Stellæ magnitudinis ſextæ. </
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<
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figmentum meum tantò magis increſcere, quantò hac
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ratione veræ Stellarum diametri magis imminuuntur. </
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