Fabri, Honoré
,
Dialogi physici in quibus de motu terrae disputatur
,
1665
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tuatur in QL ducaturque ML ſecans PN in D, haud dubiè erit PO, ad
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QL, vel PN, vt MP ad MQ, id eſt vt 1. ad 6.
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ſed angulus LML, vel
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OMP eſt ad angulum NMP, vt PO, ad PN, nempe in acutiſſimis angu
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lis, qualis ſupponitur is, ſub quo videtur Veneris diameter, arcus ſunt
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ad ſenſum vt tangentes; igitur angulus OMP eſt ad angulum NMP vt
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1. ad 6.
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cùm igitur Veneris diſtantia minima ſit ad maximam, vt vnum ad
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6.
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ejus diameter apparens in minima eſt ad apparentum in maxima vt
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NP ad PO, id eſt vt 6.
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paulò plus ad
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igitur diſcus Veneris perigeæ
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appatens eſt ad diſcum apogeæ vt 40.
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ad 1. & re ipſa talem eſſe Coperni
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canæ ſententiæ defenſores pronunciant. </
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Chryſoc.
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"> Cur appellas Copernicanæ ſententiæ defenſores? </
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">alios etiam
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appellare debueras, cùm etiam ex Tychonico ſyſtemate eadem prorſus
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diametrorum apparentium ratio, ſeu proportio conſequatur. </
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">Fac enim terram eſſe immobilem in B, Solemque per orbem ANML
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ire, ac ſecum deferte centrum epicycli Veneris; hauddubie Venus erit
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perigæa in K, apogæa in H. </
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Antim.
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"> Hoc ipſum in primo noſtro congreſſu à quo aberas, Chryſoco
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me, indicatum à me ſuperat, vt videte eſt, in V.figura, & ideò non circularem
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epicyclum deſcripſi nec etiam ellipticum, ſed ſpital: quadam, ſeu quaſi pa
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rabolica linea terminatum ab apogæo ad maximam digreſſionem, & hinc
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ad perigæum alia curva ad rectam proxime accedente: porrò noſtro </
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