Delfino, Federico, De fluxu et refluxu aquae maris, 1559

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            <p type="main">
              <s>
                <pb xlink:href="024/01/057.jpg" pagenum="22"/>
              quartas ſui parui circuli ab interſectionibus eius cum æquato­
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              re meridiano, eſt per gradus X, & XLV minutorum in arie­
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              te ecliptica mobilis. </s>
              <s>ſimiliter dicendum eſt de capite libræ mo
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              bilis. </s>
              <s>quando enim caput arietis mobilis eſt in puncto ſui par­
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              ui circuli diſtinguente quartas parui circuli ab interſectioni­
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              bus eius cum æquatore ſeptentrionale: caput libræ mobilis
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              tunc eſt in puncto ſui parui circuli diſtinguente quartas parui
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              circuli ab interſectionibus eius cum æquatore ſeptentrionali.
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              </s>
              <s>& tunc ſicut maxima diſtantia capitis arietis mobilis ab inter­
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              ſectione ecliptica mobilis cum æquatore eſt per gradus de­
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              cem, & XLV minutos in piſcibus eclipticæ mobilis; ita ma­
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              xima diſtantia capitis libræ mobilis ab interſectione eclipticæ
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              mobili æquatore eſt per gradus X, & XLV minutos ecli­
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              pticæ mobilis in uirgine eclipticæ mobilis. </s>
              <s>& quando caput
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              arietis mobilis eſt in puncto ſui parui circuli diſtinguente
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              quartas parui circuli ab interſectionibus eius cum æquatore
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              meridionali, tunc caput libræ mobilis eſt in puncto ſui parui
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              circuli diſtinguente quartas parui circuli ab interſectionibus
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              eius cum æquatore ſeptentrionali: & tunc ſicut maxima di­
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              ſtantia capitis arietis mobilis à ſeptione ecliptica mobili cum
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              æquatore eſt per gradus X, & XLV minutos eclipticæ
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              mobilis in ariete eclipticæ mobilis; ita maxima diſtantia capi­
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              tis libræ mobilis ab interſectione eclipticæ mobilis cum æqua­
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              tore eſt per gradus X, & XLV minutos eclipticæ mobi­
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              lis in libra ecliptica mobilis; & ſic ecliptica mobilis ſecatur ab
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              æquinoctiali in ſingulis punctis duorum arcuum eius: quos ar
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              cus exiſtentibus capitibus arietis, & libræ mobilibus in duo­
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              bus punctis duorum circulorum paruorum diſtinguentibus
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              quartas eorum ab interſectionibus eorum cum æquinoctiali;
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              quorum unus eſt ab ſeptentrionale æquinoctionali, et alter
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              meridionalis ſeparat à toto reſiduo eclipticæ mobilis: quorum
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              arcuum unus eſt ex parte arietis mobilis à XIX gradus XV
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              minutos piſcium ecliptica mobilis, uſque ad X gradus,
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              et XLV minutos arietis eiuſdem eclipticæ mobilis, et ali­
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              ter eſt XIX gradus, et XV minutos uirginis eclipticæ </s>
            </p>
          </chap>
        </body>
      </text>
    </archimedes>
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