DelMonte, Guidubaldo, Le mechaniche

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    <archimedes>
      <text id="id.0.0.0.0.3">
        <body id="id.2.0.0.0.0">
          <chap id="N13354">
            <p id="id.2.1.573.0.0" type="main">
              <s id="N14374">
                <pb xlink:href="037/01/108.jpg"/>
                <emph type="italics"/>
              il detto peſo. </s>
              <s id="id.2.1.573.2.0">ſimilmente ſe la leua ſi moue in BO, & la poſſanza ſoſtenente ſia
                <lb/>
              in N, ſi moſtrerà
                <lb/>
              la poſſanza in N eſ­
                <lb/>
              ſere maggiore della
                <lb/>
              poſſanza in D. </s>
              <s id="N1438B">pe­
                <lb/>
              roche SB ha pro­
                <lb/>
              portione maggiore
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              à BN che LB
                <lb/>
              à BD. </s>
              <s id="id.2.1.573.3.0">Moſtre­
                <lb/>
              raßi ancora, che
                <lb/>
              quanto il peſo più
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              s'abbaſſerà, ſempre
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              ricercarſi poſſanza
                <lb/>
              maggiore à ſoſtene­
                <lb/>
              re il peſo. </s>
              <s id="id.2.1.573.4.0">che biſo­
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              gnaua moſtrare.
                <emph.end type="italics"/>
              </s>
            </p>
            <figure id="id.037.01.108.2.jpg" xlink:href="037/01/108/2.jpg" number="101"/>
            <p id="id.2.1.576.0.0" type="main">
              <s id="id.2.1.576.1.0">
                <emph type="italics"/>
              Di quì
                <expan abbr="parimēte">parimente</expan>
              è chia
                <lb/>
              ro, che le poſſanze
                <lb/>
              in GDN coſi tra loro ſono, come BM à BL, & come BL à BS, & vlti­
                <lb/>
              mamente come BM à BS.
                <emph.end type="italics"/>
              </s>
            </p>
            <p id="id.2.1.577.0.0" type="head">
              <s id="id.2.1.577.1.0">COROLLARIO</s>
            </p>
            <p id="id.2.1.578.0.0" type="main">
              <s id="id.2.1.578.1.0">Da queſte coſe è manifeſto, che ſe la poſsanza con la leua moue
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              rà in sù il peſo, il cui centro della grauezza ſia ſopra la leua,
                <lb/>
              quanto più ſarà alzato il peſo, ſempre vi vorrà poſsanza mi­
                <lb/>
              nore per mouere il peſo. </s>
            </p>
            <p id="id.2.1.579.0.0" type="main">
              <s id="id.2.1.579.1.0">
                <emph type="italics"/>
              Percioche doue la poſſanza ſoſtenente il peſo è ſempre minore, ſarà parimente la poſ­
                <lb/>
              ſanza, che lo moue ſempre minore.
                <emph.end type="italics"/>
              </s>
            </p>
            <p id="id.2.1.580.0.0" type="main">
              <s id="id.2.1.580.1.0">
                <emph type="italics"/>
              Da queſte coſe dimoſtreraßi etiandio, ſia pur il centro della grauezza del peſo medeſi­
                <lb/>
              mo ò più da preſſo, ò più da lunge della leua AB egualmente diſtante dall' ori­
                <lb/>
              zonte, che la poſſanza medeſima in A ſoſterrà nondimeno il peſo: come ſe il cen
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              tro H della grauezza del peſo BD ſia più da lunge dalla leua BA, che il cen­
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              tro N della grauezza del peſo PV, pur che la linea HL tirata dal punto H
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              à piombo dell'orizonte, & della leua AB paßi per N, & ſia il peſo PV
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              eguale al peſo BD; ſarà sì il peſo BD, & sì il peſo PV come ſe ambidue ſoſ­
                <lb/>
              ſero appiccati ad L; & ſono eguali per eſſere preſi in luogo di vn peſo ſolo, dun­
                <lb/>
              que la iſteſſa poſſanza in A ſoſtenente il peſo BD ſoſterrà anche il peſo PV.
                <emph.end type="italics"/>
              </s>
            </p>
          </chap>
        </body>
      </text>
    </archimedes>
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