Gassendi, Pierre
,
De proportione qua gravia decidentia accelerantur
,
1646
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<
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292
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minuenda ſit pro ratione diſtantiæ, diuide Fixarum
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diſtantiam per diſtantiam Solis à Terra, fiet quotiens
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amplius, quàm duodecim. </
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<
s
id
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s.002169
">Et quia Solis diameter ap
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paret iam nobis dimidij gradus, ſiue minutorum tri
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ginta; ſequitur vt Sole inter Fixas exſiſtente, eius dia
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meter apparitura non ſit, niſi pars huius duodecima,
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ſiue minutorum duorum cùm ſemiſſe. </
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<
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id
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">Porrò hac ea
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dem diametro apparent vulgò quæ Stellæ ſunt magni
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tudinis primæ, aut ſecundæ. </
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<
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id
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">Igitur ſi Sol fuerit inter
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Fixas conſtitutus, non apparebit maior, quàm vna Stel
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larum. </
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<
s
id
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s.002172
">Et vice verſa, ſi quęlibet earumdem Stellarum
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fixarum conſtituta fuerit vbi iam eſt Sol, ſeu pari, qua
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ille à nobis diſtantia: apparebit nobis tanta, quantus
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Sol; atque adeò omnes erunt quaſi Soles. </
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<
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id
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">Quid ſi di
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ſtantiam Fixarum augeas pro opinione Albategnij
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Ptolemæo inhærentis, ſtatuentiſque illam nouemde
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cim millium ſemidiametrorum: an-non apparitura
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fuerit Solis diameter infra duo minuta? </
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<
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id
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s.002174
">Quid ſi adhûc
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ampliùs, vt debere fieri probabile eſt, nihilque repu
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gnat? </
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<
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id
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s.002175
">Verùm hoc ſufficiat, vt intelligas non nos aut
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abſurda tueri, aut ijs
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abbr
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propugnãdis
">propugnandis</
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abſurdiora fingere:
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ſed te potiùs rem non aduertere, & fingere magis. </
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<
s
id
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s.002176
">Qua
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re & cùm ſit Deusipſe, qui tot in cælo ingenteis Soleis
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pro ſua voluntate, ac verbo vnico creauit: ne cauſſare
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nos pro noſtra voluntate, verbóque vno illos creare:
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ſed agnoſce potiùs te eos pro tua voluntate, verbóque
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vno deſtruere. </
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<
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id
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s.002177
">Si illi, inquam, aduerſum me hac
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ratione inſtiterint; dic mihi, te quæſo, quid ſim reſ
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ponſurus? </
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