Gassendi, Pierre
,
De motu impresso a motore translato epistulae duae
,
1642
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mundi: adeò vt, quemadmodum axiculus globuli
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continuatus, & circumductus, intelligitur per me
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dium muſæoli ſpatium deſcribere quaſi columnam,
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cuius baſes ſint memorati in parietibus circuli; ita
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intelligere liceat immanem quandam quaſi colum
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nam per magni orbis ſpatia ab axe Terræ conti
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nüato, circumductoque deſcribi, cuius baſes ſint
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circuli illi iam repetiti in Firmamenti fornice.
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Quintò,
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denique huiuſmodi motum, ſiue continentiam in
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paralleliſmo ita fieri, vt tantillum tamen, ſeu inſen
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ſibiliter lentior ſit ipſo motu centri; efficiaturque,
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vt centro Terræ ad idem æquinoctiale punctum re
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deunte, æquator ſecet Eclipticam nonnihil cite
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rius, ac faciat cum illa angulum inclinationis, ſeu
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declinationis maximum, aliquantò antecedenter.
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<
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">Non quòd angulus inclinationis non ſit ſemper idem,
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aut æqualis, quódque æquator Terræ, axiſque ip
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ſius non ſit ſemper ſibi ipſi parallelus; ſed quòd
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huiuſmodi angulus, ſiue interſectio ſit mobilis,
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fiatque ſenſim in aliis, aliiſque Eclipticæ punctis
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(idque regrediendo, ſiue procedendo contra ſigno
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rum ſeriem, hoc eſt ab Ariete in Piſces, aut à Li
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bra in Virginem) quódque Ecliptica exſiſtente im
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mobili, tum æquatoris planum per ipſam decur
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rere intelligatur; tum poli æquatoris ſeu mundi
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intelligantur lentè moueri, idque regrediendo circa
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polos Eclipticæ, ſeruatâ ſemper eadem diſtantiâ.
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<
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">Quî id fieri valeat, vt poſſis quadamtenùs concipere,
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duc etiam circellum in memorato globulo, qui
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repręſentet Eclipticam, & æquinoctiale eius pun-</
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