Gassendi, Pierre
,
De proportione qua gravia decidentia accelerantur
,
1646
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tingeret, ſi verſus Lunam dimoueretur? </
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<
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id
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">Dicitur eſſe probabi
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le, fore, vt vbicumque Terra conſtitueretur, illeic quieſceret
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eo modo, quo corpus eiuſce materiæ, vt aquæ ſub pari mole
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æquiponderet, vbicumque in imo, in ſummo, in medio, aut vbi
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uis intra aquam ſtatuatur, conſiſtit. </
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<
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id
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">Nimirùm, quòd Terra
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ſecundum ſi totam neque grauis ſit, neque leuis; & talis affe
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ctio partium propria ſit, prout à tota diſtrahuntur: quódque in
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Mundo spherico exſiſtente, medium quidem, & extremum
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ſit, non item infimum, & ſummum; acta is conditio ſit
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Terræ, globorumque Mundi cæterorum propria, propter
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eandem partium diſtractionem, & retractionem, quæ ſigillatim
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cum speciali cuiuſque centro comparatur. </
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<
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id
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">Non probatur etiam
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aliunde Terram eſſe in Mundi medio; cùm etiam oppoſitum
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arguant excentrici ſiderum motus: neque veriſimile eſt, ſi
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Terra abduceretur in verticem Antipodum, vbi ſuper
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ficies, cui inſiſtimus, excederet punctum, in quo fuiſſet centrum,
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nos ibi hæſuros: aut abreptos vlteriùs, eò auolaturos, ſeu po
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tiùs caſuros. </
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<
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id
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">Ad aliud, quod quærit, quid eueniret lapidi, ſi
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intra cauernam in meditullio Terræ excauatam, oppletamque
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aqua, aut aëre constitueretur? </
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<
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id
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">Dicitur probabile eſſe, ſi Terra
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quidem quaſi magnes ſit, qui ſuis quaſi radijs emißis attrahat
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terrena: euenturum, vt lapis ineam cauernæ partem feratur, è
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qua radij plures, confertioreſque affluxerint; &, ſi ſupponan
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tur ex æquo vndequàque affluere, fore, vtin medio ſuſpenſus
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teneatur. </
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<
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id
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">Vnde &, quod rogat, cur lapis in puteum dimiſſus
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fundum petat, non latera? </
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<
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id
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">Cauſſa eſt in promptu, quòd plu
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res, denſioreſque radij exparte fundi, ad quam eſt tota Terræ
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moles, adueniant, quàm ex parte vlla laterum aduenire
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poßint.
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A p 247. in 254. </
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