Fabri, Honoré, Dialogi physici in quibus de motu terrae disputatur, 1665

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      <text>
        <body>
          <chap>
            <p type="main">
              <s id="s.000351">
                <pb pagenum="31" xlink:href="025/01/035.jpg"/>
              mentum æſtus, eadem, ſummum decrementum; quod tamen omnibus
                <lb/>
              Obſervationibus repugnat: ſi enim hac ipſa die, Luna in Meridie ſci­
                <lb/>
              licet exiſtente, ſit ſummum crementum æſtus hora meridiana, vt ſit in no­
                <lb/>
              vilunio, craſtina die, idem ſummum crementum erit minutis 48. circiter
                <lb/>
              poſt Meridiem; & tertio poſt die hora, 1. 36. minutis poſt Meridiem, at­
                <lb/>
              que ita deinceps; idem de Plenilunio dicendum eſt. </s>
            </p>
            <p type="main">
              <s id="s.000352">
                <emph type="italics"/>
              Auguſtin.
                <emph.end type="italics"/>
              </s>
              <s id="s.000353"> Ita fortè diſponi poſſunt prædicti duo motus, orbis ſcilicet
                <lb/>
              & centri, vt motus mixtus inde reſultans tales in æſtu mutationes pro­
                <lb/>
              ducat. </s>
            </p>
            <p type="main">
              <s id="s.000354">
                <emph type="italics"/>
              Antim.
                <emph.end type="italics"/>
              </s>
              <s id="s.000355"> Nullo ſané modo id fieri poſſe, omni aſſeveratione affirmo; quod
                <lb/>
              vt clariùs exponam. </s>
            </p>
            <figure id="id.025.01.035.1.jpg" xlink:href="025/01/035/1.jpg" number="10"/>
            <p type="main">
              <s id="s.000356">Sit A Centrum mundi, DBLC orbita terræ, vel magnus orbis, D cen­
                <lb/>
              trum terræ, quam paulò majorem deſcribo, ne parvitas orbis confuſio­
                <lb/>
              nem patiat; dum centrum D movetur versùs B, ita volvitur circulus cir­
                <lb/>
              ca D, vt Eversùs I, & F, versùs H tendat. </s>
              <s id="s.000357">Vnde reſultat ex vtroque mo­
                <lb/>
              tu æquabili motus mixtus omnino inæqualis; nempe ab H in I, per E;
                <lb/>
              additur motus orbis, motui centri; id eſt ſpatio decurſo ſolo motu cen­
                <lb/>
              tri, ſpatium æquale diametro IH ; ab I verò in H per F, idem ſpatium
                <lb/>
              detrahitur ſpatio decurſo motu centri, hinc ab H in E, acelerationis cre­
                <lb/>
              menta, ſuprà motum centri, ſunt in ratione ſinuum verſorum arcuum
                <lb/>
              decurſorum; ab E in I, in ratione ſinuum rectorum; decrementa pariter
                <lb/>
              ab I in F, ſunt in ratione ſinuum verſorum; ab F verò in H, in ratione </s>
            </p>
          </chap>
        </body>
      </text>
    </archimedes>
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