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

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    <archimedes>
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            <figure id="id.025.01.014.1.jpg" xlink:href="025/01/014/1.jpg" number="4"/>
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              <s id="s.000139">
                <emph type="italics"/>
              Antim.
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              </s>
              <s id="s.000140"> Schemate opus eſſe non putarem, quia tamen ita iubes, tibi
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              morem geram. </s>
              <s id="s.000141">Sit A. centrum vniverſi, ſitque BCDE magnus Orbis,
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              vt vocant, in quo, primo loco, iuxta tuam hypotheſim, terreſtrem globum
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              moveri ſuppono; ſit orbita Martis FRPS. </s>
              <s id="s.000142">Terra moveatur ex C. per B.
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              in conſequentia, vt vocant, id eſt, iuxta ſeriem Signorum; Item Mars ex F
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              per R. ſupponatur Mars in F, & terra in B; Supponamus lineam AF pro­
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              ductam ad ſtellas, terminari ad principium Cancri, ac proinde AB. pro­
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              ductam ad initium Libræ; ex puncto B, Mars videbitur per lineam BFL.
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              </s>
              <s id="s.000143">Igitur in eo Zodiaci puncto, quod, a principio Cancri versùs Occaſum di­
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              ſtat, toto angulo BFA, vel quod idem eſt, FAM. </s>
              <s id="s.000144">Item ſi ſtatuamus initio
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              Terram in D, Martem in S. erit Mars in Perigæo, & in oppoſitione; ſpatio
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              vorò ſex menſium, circiter, Mars ab S. pervenit ad F, & Terra à D.ad IB;
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              tunc autem Mars eſt in mediocri diſtantia, & videtur retrogredi à puncto
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              in, quo non videtur ex B, ſed in quo eſt, ad punctum L, vel K, in quo non eſt,
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              ſed in quo videtur ex B. </s>
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            <p type="main">
              <s id="s.000145">In noſtra communique hypotheſi, hæc æquè facilè explicantur, ſit enim
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              Terra in Centro A ſit BCDE orbita Solis, ſit FRPS, deferens centrum
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              Epicych Marris; ſit demum ONCM, Epicyclus Martis, cuius motus, cir-</s>
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          </chap>
        </body>
      </text>
    </archimedes>