Fabri, Honoré - Dialogi physici in quibus de motu terrae disputatur

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1mentum æſtus, eadem, ſummum decrementum; quod tamen omnibus
Obſervationibus repugnat: ſi enim hac ipſa die, Luna in Meridie ſci
licet exiſtente, ſit ſummum crementum æſtus hora meridiana, vt ſit in no
vilunio, craſtina die, idem ſummum crementum erit minutis 48. circiter
poſt Meridiem; & tertio poſt die hora, 1. 36. minutis poſt Meridiem, at
que ita deinceps; idem de Plenilunio dicendum eſt.

Auguſtin. Ita fortè diſponi poſſunt prædicti duo motus, orbis ſcilicet
& centri, vt motus mixtus inde reſultans tales in æſtu mutationes pro
ducat.

Antim. Nullo ſané modo id fieri poſſe, omni aſſeveratione affirmo; quod
vt clariùs exponam.

10[Figure 10]

Sit A Centrum mundi, DBLC orbita terræ, vel magnus orbis, D cen
trum terræ, quam paulò majorem deſcribo, ne parvitas orbis confuſio
nem patiat; dum centrum D movetur versùs B, ita volvitur circulus cir
ca D, vt Eversùs I, & F, versùs H tendat. Vnde reſultat ex vtroque mo
tu æquabili motus mixtus omnino inæqualis; nempe ab H in I, per E;
additur motus orbis, motui centri; id eſt ſpatio decurſo ſolo motu cen
tri, ſpatium æquale diametro IH ; ab I verò in H per F, idem ſpatium
detrahitur ſpatio decurſo motu centri, hinc ab H in E, acelerationis cre
menta, ſuprà motum centri, ſunt in ratione ſinuum verſorum arcuum
decurſorum; ab E in I, in ratione ſinuum rectorum; decrementa pariter
ab I in F, ſunt in ratione ſinuum verſorum; ab F verò in H, in ratione

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