Gassendi, Pierre, De motu impresso a motore translato epistulae duae, 1642

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            <p type="main">
              <s id="id.000887">
                <pb pagenum="139" xlink:href="027/01/138.jpg"/>
              tum videamus, ac dum Terra in Capricorno eſt, vn­
                <lb/>
              de ille gibbus nihil nobis obſtat. </s>
              <s id="id.000888">Fit quoque proin­
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              de, vt Terra exſiſtente in Cancro, diem minimum,
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              hiememque habeamus, & exſiſtente in Capricorno,
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              diem maximum, æſtatemque, & in locis aliis eadem
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              proportione. </s>
              <s id="id.000889">Quod perſpicuè intelliges, ſi quem glo­
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              bulum ſupra vulgaris ſphæræ Zodiacum reuoluen­
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              dum monuï, notes in boreo aliquo puncto, & ipſum
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              punctum compares cum Sole in medio Sphæræ de­
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              gere intellecto; idque dum globulum (axe eius ſibi
                <lb/>
              ſemper parallelo detento) in Cancro, in Capricor­
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              no, in partibus aliis Zodiaci reuolueris. </s>
              <s id="id.000890">Neque mo­
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              rari debet
                <emph type="italics"/>
              Quintò,
                <emph.end type="italics"/>
              quòd ſphæra Fixarum obſeruetur
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              moueri in ortum; ac ſecundum Eclipticæ longitudi­
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              nem, lento illo motu, ob quem conſtellatio Arietis,
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              quæ ante bis mille circiter annos ad interſectionem
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              æquinoctialem erat, ab ea receſſit, diſtatque iam toto
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              penè ſigno, ſeu duodecima Zodiaci parte; qua ea­
                <lb/>
              dem ratione receſſerunt, ac promotæ ſunt cæteræ,
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              omneſque adeò ſtellæ fixæ ſedibus ſuis ſunt emotæ,
                <lb/>
              ac ſpeciatìm Polaris dicta, quæ manifeſtè effecta eſt
                <lb/>
              longè, quàm olim, polo propinquior. </s>
              <s id="id.000891">Siquidem &
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              ſtellæ Arietis, & cæteræ omnes non ita apparent mo­
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              ueri, quòd motu ſibi proprio ſecundum ſignorum
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              ſeriem progrediantur ab æquinoctialibus punctis; ſed
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              quòd æquinoctialia puncta ob Terræ motum, retar­
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              dationemve antè expoſitam, regrediantur contra ſi­
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              gnorum ſucceſſionem. </s>
              <s id="id.000892">Quemadmodum nempe ſeu
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              Terra moueatur in ortum, ſeu Sol moueatur in oc­
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              caſum, Sol ſemper moueri in occaſum nobis apparet, </s>
            </p>
          </chap>
        </body>
      </text>
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