Salusbury, Thomas, Mathematical collections and translations (Tome I), 1667

Table of figures

< >
[Figure 11]
[Figure 12]
[Figure 13]
[Figure 14]
[Figure 15]
[Figure 16]
[Figure 17]
[Figure 18]
[Figure 19]
[Figure 20]
[Figure 21]
[Figure 22]
[Figure 23]
[Figure 24]
[Figure 25]
[Figure 26]
[Figure 27]
[Figure 28]
[Figure 29]
[Figure 30]
[Figure 31]
[Figure 32]
[Figure 33]
[Figure 34]
[Figure 35]
[Figure 36]
[Figure 37]
[Figure 38]
[Figure 39]
[Figure 40]
< >
page |< < of 701 > >|
    <archimedes>
      <text>
        <body>
          <chap>
            <p type="main">
              <s>
                <pb xlink:href="040/01/317.jpg" pagenum="297"/>
              think of accomodating the body of
                <emph type="italics"/>
              Venus
                <emph.end type="italics"/>
              in ſuch a manner that
                <lb/>
              its ſtate and motion may agree with what ſenſible experiments do
                <lb/>
              ſhew us; and therefore recall to mind that. </s>
              <s>which either by the
                <lb/>
              paſt diſcourſes, or your own obſervations you have learnt to
                <lb/>
              fal that ſtar, and afterwards aſſign unto it that ſtate which you
                <lb/>
              think agreeth with the ſame.</s>
            </p>
            <p type="main">
              <s>SIMP. </s>
              <s>Suppoſing thoſe
                <emph type="italics"/>
              Phænomena
                <emph.end type="italics"/>
              expreſſed by you, and
                <lb/>
              which I have likewiſe read in the little treatiſe of Concluſions, to
                <lb/>
                <figure id="id.040.01.317.1.jpg" xlink:href="040/01/317/1.jpg" number="18"/>
                <lb/>
              be true, namely, that that ſtar never recedes from the Sun beyond
                <lb/>
              ſuch a determinate ſpace of 40 degrees or thereabouts, ſo as that
                <lb/>
              it never cometh either to appoſition with the Sun, or ſo much as
                <lb/>
              to quadrature, or yet to the ſextile aſpect; and more than that,
                <lb/>
                <arrow.to.target n="marg526"/>
                <lb/>
              ſuppoſing that it ſheweth at one time almoſt 40 times greater than
                <lb/>
              at another; namely, very great, when being retrograde, it goeth to
                <lb/>
              the veſpertine conjnnction of the Sun, and very ſmall when with a </s>
            </p>
          </chap>
        </body>
      </text>
    </archimedes>