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

Page concordance

< >
Scan Original
51
52
53
54
55
56
57
58
59
60
61
62
63
64
65
66
67
68
69
70
71
72
73
74
75
< >
page |< < of 75 > >|
    <archimedes>
      <text>
        <body>
          <chap>
            <p type="main">
              <s>
                <pb xlink:href="024/01/059.jpg" pagenum="23"/>
              nunc uerſus orientem, nunc motu ueloci, nunc motu tar­
                <lb/>
              do propter diuerſum ſitum capitis arietis octauæ ſphæræ in
                <lb/>
              ſuo circulo paruo, & propter diuerſum motum ſectionis
                <lb/>
              æquinoctialis per eclipticam octauæ ſphæræ. </s>
              <s>nam in toto
                <lb/>
              tempore, in quo caput arietis octauæ ſphæræ recedit à
                <lb/>
              puncto ſui parui circuli diſtinguente quartas ab interſe­
                <lb/>
              ctionibus eius cum æquatore meridionali, donec ueniat
                <lb/>
              ad punctum ſui parui circuli diſtinguentem quartas ab in­
                <lb/>
              terſectionibus eius cum æquatore ſeptentrionale ſectio e­
                <lb/>
              clipticæ octauæ ſphæræ cum æquinoctiali primi mobilis,
                <lb/>
              ſcilicet quæ mouetur continue per eclipticam octauæ ſphæ­
                <lb/>
              ræ contra ſucceſſionem ſignorum à X grad. arietis eclipti­
                <lb/>
              cæ octauæ ſphæræ, & XLV min. uſque ad XIX grad. pi­
                <lb/>
              ſcium, & XV min. eclipticæ octauæ ſphæræ cum æquino­
                <lb/>
              ctionali: recedit à ſtellis fixis octauæ ſphæræ, quæ eſt uer­
                <lb/>
              ſus orientem ab ea eundo uerſus ſtellas fixas, quæ eſt uer­
                <lb/>
              ſus occidentem ab ea appropinquando eis: & propter hoc
                <lb/>
              ſtellæ, quæ ſunt uerſus orientem, ab ea uidentur moue­
                <lb/>
              ri ſupra ſucceſſionem ſignorum, ſcilicet uerſus orientem:
                <lb/>
              & ſtellæ, quæ ſunt uerſus occidentem, ab ea uidentur ſe­
                <lb/>
              qui eas ſupra ſucceſſionem ſignorum: cum tamen in ue­
                <lb/>
              ritate moueantur contra ſucceſſionem ſignorum, ſcilicet
                <lb/>
              uerſus occidentem: & tunc caput libræ octauæ ſphæræ re­
                <lb/>
              cedit à puncto ſui parui circuli diſtinguente quartas eius
                <lb/>
              ab interſectionibus eius cum æquatore ſeptentrionali, &
                <lb/>
              uenit ad punctum ſui parui circuli diſtinguentem quartas
                <lb/>
              ſui parui circuli ab interſectionibus eius cum æquatore
                <lb/>
              meridionali, & ſectio eclipticæ octauæ ſphæræ cum æqui­
                <lb/>
              noctionali primi mobilis mouetur ſimiliter continue per
                <lb/>
              eclipticam octauæ ſphæræ contra ſucceſſionem ſignorum
                <lb/>
              à X grad. libræ eclipticæ octauæ ſphæræ, & XLV mi­
                <lb/>
              nut. </s>
              <s>uſque ad XIX grad. & XV minut. </s>
              <s>uirginis eiuſdem
                <lb/>
              eclipticæ octauæ ſphæræ: & tunc ſectio ecliptica octauæ </s>
            </p>
          </chap>
        </body>
      </text>
    </archimedes>
Impressum