Fabri, Honoré
,
Dialogi physici in quibus de motu terrae disputatur
,
1665
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Antim.
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Hæc ſunt veſtræ hypotheſeos miracula; ſed hæc in noſtra hy
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potheſi facilè explicantur. </
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<
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">Sit enim Saturnus in I, Mars in M, Sol in C, cùm ſingulis diebus, ſeu dìur
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nis revolutionibus Mars relinquatur à Stellis Ortum versùs 3 ò. </
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">circiter,
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dum ſcilicet directus eſt, & Saturnus. </
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<
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">2. Sit arcus FM, grad. 22. 15. minutis
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circiter; poſt 45. dies Mars erit in F, Saturnus verò diſtabit à puncto I,
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Ortum versùs grad. 3. igitur ſeptimo poſt die, Mars Saturno conjungetur,
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directus directo; item Iupiter Marti; crat autem Saturnus in Apogæo,
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vt conſtat, conjunctus ſcilicet Soli. </
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">Supponamus autem Martem oppo
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ſitum in R, Solem in D, Saturnum in I, cùm Saturnus à ſtatione haud pro
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cul abſit, eſt enim juxta Quadraturam, tanto intervallo Mars regredi ne
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quit versùs F, vt Saturno directo jungatur; quia ſtatim Saturnus ſtatio
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nem attingit, & paucis poſt diebus, fit retrogradus: eadem ratio facit
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pro Iove, vt ſcilicet nunquam Saturno directo, retrogradus jungatur.
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</
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<
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id
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">Sed vt hæc paulò accuratiùs diſcutiamus; cùm Saturni & Solis conjun-</
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