Descartes, René
,
Renati Des-Cartes principia philosophiae
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praeterea etiam Solis maculae (ſaltem ſi verae ſint obſer
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vationes Scheineri S. 1. a, poſt cujus diligentiam nihil
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circa iſtarum macularum phaenomena deſiderari poſſe
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videtur), in planis 7 gradibus aut ampliús ad Eclipticam
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inclinatis, circa Solem volvuntur adeò ut earum mo
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tus hac in re non differat à motibus Planetarum. </
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>Luna
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etiam circa Terram fertur, in plano quod 5 gradibus
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ab Eclipticà deflectit; & Terra circa proprium axem
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in plano AEquatoris 23 ¬Ω gradibus ab Eclipticâ defle
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ctente; quod planum AEquatoris ipſa ſecum defert. </
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Atque hae Planetarum aberrationes ab Eclipticâ vo
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cantur motus in latitudinem b. </
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XXXV.
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De aberratione Plane
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tarum in latitudinem. </
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Ipſorum autem circuitiones circa Solem vocantur
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motus in longitudinem. </
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>Hique etiam in eo aberrant,
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quòd non aequaliter ubique à Sole diſtent; ſed hac
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aetate, Saturnus ab eo remotior eſt in Sagittario quàm
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in Geminis, viceſimâ circiter diſtantia ſuae parte; Ju
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piter in Librâ remotior eſt quàm in Ariete; ſicque alii
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Planetae habent Aphelia & Perihelia ſua aliis in locis c.
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Poſt aliquot autem ſaecula, haec omnia mutata eſſe
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deprehendentur; ac ſinguli Planetae, nec non etiam
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Terra, planum in quo nunc eſt Ecliptica, diverſis in
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locis ſecabunt, & paulo magis vel minús ab illà defle
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ctent; & illorum maximae ac minimae à Sole diſtantiae
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in aliis ſignis reperientur d. </
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XXXVI.
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De motu in longitui
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nem. </
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Jam verò non opus eſt ut oſtendam, quo pacto ex
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hac hypotheſi ſequantur phaenomena diei & noctis,
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aeſtatis & hyemis, ſive acceſſús Solis ad Tropicos, & </
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