Valerio, Luca, De centro gravitatis solidorvm libri tres

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                <pb xlink:href="043/01/271.jpg" pagenum="92"/>
              liqui ſolidi AEBFC centrum grauitatis eſse G. </s>
              <s>Secta
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              enim BD bifariam in puncto H, & poſita GK ipſius GH
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              minori quantacumque longitudine propoſita, ſumptoque
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              in GK quolibet puncto L, intelligantur id enim (fieri poſ­
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              ſe manifeſtum eſt ex ſupra demonſtratis) tres figuræ vna in­
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              ſcripta conoidi EBF, & duæ circumſcriptæ altera alteri
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              conoidum, vt ſupra factum eſt, compoſitæ ex cylindris
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              æqualium altitudinum ita multiplicatis, vt vtrumque illud
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              accidat; & vt ſecundi exceſſus centrum grauitatis quod ſit
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              M (omnium autem trium dictorum exceſſuum in axe
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              BD erunt centra grauitatis) ſit puncto G propinquius
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                <figure id="id.043.01.271.1.jpg" xlink:href="043/01/271/1.jpg" number="198"/>
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              quàm punctum L: & vt primus exceſſus ad ſecundum mi­
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              norem habeat proportionem ea, quæ eſt LK, ad KH. </s>
              <s>Dein
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              de vt HK ad KL, ita ſit HN ad NM, & vt primus
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              exceſſus ad ſecundum, ita MO ad OH. </s>
              <s>Quoniam igitur
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              cylindri omnes deficientes, & ſummus integer, ex quibus
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              primus exceſſus conſtat, inter ſe ſunt æquales, habentque
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              in axe BD centra grauitatis æqualibus interuallis à bipar­
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              titi axis BD ſectione H & inter ſe diſtantia; totius pri­
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              mi exceſſus centrum grauitatis erit H: ſecundi autem ex­
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              ceſſus centrum grauitatis ponitur M; cum igitur ſit vt pri­
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              mus exceſſus ad ſecundum, ita ex contraria parte MO </s>
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