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

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    <archimedes>
      <text>
        <body>
          <chap>
            <pb pagenum="22" xlink:href="025/01/026.jpg"/>
            <p type="main">
              <s id="s.000276">
                <emph type="italics"/>
              Antim.
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              Hæc ſunt veſtræ hypotheſeos miracula; ſed hæc in noſtra hy­
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              potheſi facilè explicantur. </s>
            </p>
            <figure id="id.025.01.026.1.jpg" xlink:href="025/01/026/1.jpg" number="7"/>
            <p type="main">
              <s id="s.000277">Sit enim Saturnus in I, Mars in M, Sol in C, cùm ſingulis diebus, ſeu dìur­
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              nis revolutionibus Mars relinquatur à Stellis Ortum versùs 3 ò. </s>
              <s id="s.000278">circiter,
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              dum ſcilicet directus eſt, & Saturnus. </s>
              <s id="s.000279">2. Sit arcus FM, grad. 22. 15. minutis
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              circiter; poſt 45. dies Mars erit in F, Saturnus verò diſtabit à puncto I,
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              Ortum versùs grad. 3. igitur ſeptimo poſt die, Mars Saturno conjungetur,
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              directus directo; item Iupiter Marti; crat autem Saturnus in Apogæo,
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              vt conſtat, conjunctus ſcilicet Soli. </s>
              <s id="s.000280">Supponamus autem Martem oppo­
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              ſitum in R, Solem in D, Saturnum in I, cùm Saturnus à ſtatione haud pro­
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              cul abſit, eſt enim juxta Quadraturam, tanto intervallo Mars regredi ne­
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              quit versùs F, vt Saturno directo jungatur; quia ſtatim Saturnus ſtatio­
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              nem attingit, & paucis poſt diebus, fit retrogradus: eadem ratio facit
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              pro Iove, vt ſcilicet nunquam Saturno directo, retrogradus jungatur.
                <lb/>
              </s>
              <s id="s.000281">Sed vt hæc paulò accuratiùs diſcutiamus; cùm Saturni & Solis conjun-</s>
            </p>
          </chap>
        </body>
      </text>
    </archimedes>
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