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

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            <p type="main">
              <s>
                <pb xlink:href="024/01/061.jpg" pagenum="24"/>
              ſeptentrionali: & ſectio ecliptica octauæ ſphæræ cum æ­
                <lb/>
              quinoctiali mouetur continue per eclipticam octauæ ſphæ­
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              ræ à XIX grad. XV min. uirginis ecliptica octauæ ſphæ­
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              ræ, uſque ad X grad. & XLV min. libræ eclipticæ octauæ
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              ſphæræ cum æquinoctionali recedit à ſtellis fixis, quæ ſunt
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              uerſus occidentem, ab ea eundo uerſus ſtellas fixas, quæ
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              ſunt uerſus orientem, ab ea appropinquando eis: & pro­
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              pter hoc ſtellæ, quæ ſunt uerſus occidentem, ab ea uiden­
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              tur moueri contra ſucceſſionem ſignorum, ſcilicet uerſus
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              occidentem: & quæ ſunt uerſus orientem ab ea uidentur
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              ſequi eas, cum iam in ueritate moueantur ſupra ſucceſſio­
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              nem ſignorum, ſcilicet uerſus orientem. </s>
              <s>cum autem caput
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              arietis octauæ ſphæræ recedit à puncto ſui parui circuli di­
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              ſtinguente quartas eius ab interſectionibus eius cum æqui­
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              noctiali, meridionali uerſus orientem accedens: tunc ſectio
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              ecliptica octauæ ſphæræ mouetur per eclipticam octauæ ſphæ
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              ræ tarde uerſus orientem; quia æquatio octauæ ſphæræ, quam
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              ponit Thebit eſſe arcum. </s>
              <s>ecliptica octauæ ſphæræ à capite
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              arietis octauæ ſphæræ, uſque ad interſectionem eclipticæ o­
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              ctauæ ſphæræ cum æquinoctionali parum decreſcit: & tunc
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              ſtellæ fixæ uidentur moueri uerſus occidentem tarde. </s>
              <s>cum
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              autem caput arietis octauæ ſphæræ eſt prope ſectione ſui par­
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              ui circuli cum æquinoctionali orientali, ex utroque latere
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              eius ſectio ecliptica octauæ ſphæræ ibi, uel multum decre­
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              ſcit, uel multum creſcit; & tunc ſtellæ fixæ uidentur mo­
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              ueri uerſus occidentem uelociter. </s>
              <s>cum autem caput arie­
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              tis octauæ ſphæræ appropinquat puncto ſui parui circuli di­
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              ſtinguenti quartas eius ab interſectionibus eius cum æqui­
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              noctionali, meridionali, donec ueniat ad ipſum, tunc ſectio
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              ecliptica octauæ ſphæræ mouetur per eclipticam octauæ
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              ſphæræ uerſus orientem tarde; quia æquatio octauæ ſphæræ
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              parum creſcit, & tunc ſtellæ uidentur moueri tarde uerſus
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              occidentem. </s>
            </p>
            <p type="main">
              <s>Cum
                <expan abbr="autẽ">autem</expan>
              caput arietis octauæ ſphæræ recedit à
                <expan abbr="pũcto">puncto</expan>
              ſui par­
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              ui circuli diſtinguenti quartas eius ab interſectionibus eius
                <expan abbr="cũ">cum</expan>
              </s>
            </p>
          </chap>
        </body>
      </text>
    </archimedes>
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