Fabri, Honoré
,
Dialogi physici in quibus de motu terrae disputatur
,
1665
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Auguſtin.
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<
s
id
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s.000853
"> Ille motus, qui fit per lineam HPG mixtus eſt ac proinde
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inæqualis, ſed ex duobus æquabilibus, vt iam dixi. </
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Antim.
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</
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<
s
id
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s.000855
"> Vnde porrò ſunt illi duo motus æquabiles' à quo principio? </
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<
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id
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s.000856
">&
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quo tandem organo traducuntur? </
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<
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id
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<
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Auguſtin.
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emph.end
type
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italics
"/>
</
s
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<
s
id
="
s.000858
"> Affulget novæ lux reſponſionis; ſuperficies terræ inæquali
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ter movetur, etiam in eodem circulo majore ; nempe ille arcus, qui ad
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Solem convertitur, tardiſſimus eſt, oppoſitus verò velociſſimus, quid mi
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rum igitur, ſi hic Lunam longiùs promovet, ſcilicet circa Plenilunium,
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ille verò longè minùs, ſcilicet circa Novilunium. </
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Antim.
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type
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</
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<
s
id
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s.000860
"> Non negarim, acutam, & non nemini fortè inexpectatam re
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ſponſionem; ſed præterquam quod ſubſiſtunt alia ſupra oppoſita; quia nec
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in arcubus, diurnis circulis parallelis Luna movetur, non videtur, cur mo
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tus centri in Lunam traductus debilior non exiſtat. </
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<
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id
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<
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type
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"/>
Auguſtin.
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type
="
italics
"/>
</
s
>
<
s
id
="
s.000862
"> Miror, hæc à te dici, cùm vterque debilior exiſtat, vt mani
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feſtum eſt; ſic enim ab H ad O parum progreditur, tum motu centri, tum
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motu orbis; igitur à puncto terræ oppoſito ſuam vim accipit, majorem
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ſcilicet, cùm velociùs illud movetur, quamvis alioquin motu mixto; mi
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norem verò cùm tardiùs, quid ad aliud de arcubus parallelis reſpondeam,
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non habeo, niſi fortè dicam, Lunam à ſe ipſa, vel ab Angelo per illam or
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bitam moveri: Sed cur per illam movetur inæqualiter? </
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>
<
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id
="
s.000863
">deinde hæc orbita
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reſpectum habet ad terram, quæ in ſua libratione diverſam periodum ha
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bet, malim ergo ingenuè fateri, me neſcire, quid ad hoc reſpondeam. </
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Antim.
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</
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<
s
id
="
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"> Reſumo quod ſupra dicere cœperam; præter illa argumenta,
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inquam, quibus allata reſponſio non congruit, dico aliam eamque inſo
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lubilem reſtare difficultatem; admiſſa enim prædicta reſponſione, fateris
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in puncto G majorem vim impetus à puncto terræ oppoſito Lunam ac
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cipere, minorem verò à puncto H, cur ergo Luna impreſſum impetum
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deinde non retinet? </
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>
<
s
id
="
s.000866
">cum nihil ſit à quo deſtruatur; nec enim obſtat, à
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novo puncto terræ oppoſito ad aliam tangentem determinari, quia cùm
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hoc fiat per novi impetus acceſſionem, hic aditus priori majorem vim
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facit; igitur nulla eſſet ratio, cur deinde motus retardaretur versùs Qua
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draturas. </
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<
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Chryſoc.
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type
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</
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>
<
s
id
="
s.000868
"> Vereor, vt inde quiſpiam cauſam deducat, rei miſſionis marini
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æſtus in Quadratoris; nempe, vt in Oppoſitione vegetior eſt, ita in Quadra
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turis minor eſt & flaccidior; quia, inquiet, cùm à Luna procedat, Lunæ
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motus in plenilunio maior eſt, minor in Quadraturis; minorem igitur in
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his, majorem in illo motus effectum producit. </
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<
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<
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type
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Auguſtin.
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emph.end
type
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"/>
</
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>
<
s
id
="
s.000870
"> Sed in Novilunio Lunaris motus adhuc minor eſt, quam in
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Quadraturis, & tamen nemo neſcit, æſtum in Novilunio majorem eſſe; alia
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igitur ratio prædictæ differentiæ inveſtiganda eſt. </
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<
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id
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<
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type
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"/>
Chryſocom.
<
emph.end
type
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italics
"/>
</
s
>
<
s
id
="
s.000872
"> Aliud in mentem venit, quod expromendum eſſe puto;
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nempe ſi ſupponam Lunam 24. horarum ſpatio orbem ſuum circa terram
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abſolvere, illius velocitas ad velocitatem puncti æquatoris in ſuperficie
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terræ erit vt 60.ad 1.ſunt enim motus vt circuli, hi vtrò, vt ſemidiametri;
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igitur non mirum eſt, cùm motus tardus velocem producere nequeat, ſi </
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