Bernoulli, Daniel
,
Hydrodynamica, sive De viribus et motibus fluidorum commentarii
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SECTIO UNDECIMA.
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verſæ habere denſitatis ſpecificæ mihi admodum eſt probabile, quia nullam vi-
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deo rationem, cur in omnibus planetis ſimiles eſſe debeant iſtæ particulæ. </
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<
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à particularum gravium denſitate in quolibet planeta pendet hujus vis centrifuga
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ſeu conatus recedendi à ſole. </
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<
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">Igitur nondum licet colligere planetarum vires
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centrifagas ſe habere, in ratione quadr ata reciproca eorundem diſtantiarum à
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ſole ex eo, quod tempora periodica rationem ſequantur ſeſquiplicatam diſtan-
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tiarum: </
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<
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">talis enim concluſio ſupponit ſimilem in omnibus planetis particula-
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rum gravium denſitatem.</
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<
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">Planetarum vires centrifugæ æquales utique ſunt viribus contra-
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riis quibus verſus ſolem trahuntur: </
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<
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">Quia autem, ut dixi in ſuperiori paragra-
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pho, nondum certum eſt, in quanam ratione reſpectu diſtantiarum à ſole vi-
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res planetarum centrifugæ mutentur, ideo neque de eorum viribus gravitatis
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verſus ſolem aliquid certi ſtatuere licet; </
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<
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">Et plurima quidem ſunt in vorticum
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hypotheſi, quæ vires gravitatis in diverſis diſtantiis conſtituunt & </
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<
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<
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<
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">Cum enim vis gravitatis ſit æqualis vi centrifugæ materiæ ſubtilis, quæ
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particulas corporis graves penetrare nequit, ſequitur eo majorem eſſe vim gra-
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vitatis, quo majori materiæ ſubtilis quantitati tranſitus negatur; </
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<
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">quia vero ſci-
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mus corpus ſæpe fluido uni impenetrabile eſſe, quod alii fluido ſubtiliori li-
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berrimum concedit transfluxum, fieri poteſt, ſi modo materiam vorticoſam
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in diverſis à centro vorticis diſtantiis inæqualiter ſubtilem putemus, ut unus
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idemque planeta in inæqualibus à ſole diſtantiis inæqualiter ad ſolem pellatur,
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quod idem facilius contingere poteſt @in diverſis planetis, quia accedit diverſa
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quæ eſſe poteſt particularum gravium, ſtructura.</
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<
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">Præter hæc ſunt etiam diverſa materiæ vorticoſæ denſitas, velocitas di-
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ftantiaque à centro, quæ concurrunt ad vim gravitatis formandam. </
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<
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eorum ratio habeatur, apparebit poſſe quidem vires gravitatis decreſcere
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creſcentibus diſtantiis à centro virium, neque tamen propterea vires centrifugas
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æqualium materiæ vorticoſæ voluminum pariter decreſcere, quod poſterius
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ob rationem §. </
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ſta vero quæ generaliter & </
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rumque ad Phænomena gravitatis applicatione, ſufficiant: </
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