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

Table of figures

< >
[Figure 171]
[Figure 172]
[Figure 173]
[Figure 174]
[Figure 175]
[Figure 176]
[Figure 177]
[Figure 178]
[Figure 179]
[Figure 180]
[Figure 181]
[Figure 182]
[Figure 183]
[Figure 184]
[Figure 185]
[Figure 186]
[Figure 187]
[Figure 188]
[Figure 189]
[Figure 190]
[Figure 191]
[Figure 192]
[Figure 193]
[Figure 194]
[Figure 195]
[Figure 196]
[Figure 197]
[Figure 198]
[Figure 199]
[Figure 200]
< >
page |< < of 701 > >|
    <archimedes>
      <text>
        <body>
          <chap>
            <pb xlink:href="040/01/949.jpg" pagenum="256"/>
            <p type="main">
              <s>
                <emph type="italics"/>
              Let there be a Conoid whoſe Axis is A B, and the Center of the
                <lb/>
              circumſcribed Figure C, and the Center of the inſcribed O. </s>
              <s>I ſay
                <lb/>
              the Center of the Conoid is betwixt the points C and O. </s>
              <s>For if
                <lb/>
              not, it ſhall be either above them, or below them, or in one of them. </s>
              <s>Let
                <lb/>
              it be below, as in R. </s>
              <s>And becauſe R is the Center of Gravity of the
                <lb/>
              whole Conoid; and the Center of Gravity of the inſcribed Figure is O:
                <lb/>
              Therefore of the remaining proportions by which the Conoid exceeds
                <lb/>
              the inſcribed Figure the Center of Gravity ſhall be in the Line O R ex­
                <lb/>
              tended towards R, and in that point in which it is ſo determined, that,
                <lb/>
              what proportion the ſaid proportions have to the inſcribed Figure, the
                <lb/>
              ſame ſhall O R have to the Line falling betwixt R and that falling point.
                <lb/>
              </s>
              <s>Let this proportion be that of O R to R X. </s>
              <s>Therefore X falleth either
                <lb/>
              without the Conoid or within, or in its
                <emph.end type="italics"/>
                <lb/>
                <figure id="id.040.01.949.1.jpg" xlink:href="040/01/949/1.jpg" number="170"/>
                <lb/>
                <emph type="italics"/>
              Baſe. </s>
              <s>That it falleth without, or in its
                <lb/>
              Baſe it is already manifeſt to be an abſur­
                <lb/>
              dity. </s>
              <s>Let it fall within: and becauſe X R
                <lb/>
              is to R O, as the inſcribed Figure is to
                <lb/>
              the exceſs by which the Conoid exceeds
                <lb/>
              it; the ſame proportion that B R hath to
                <lb/>
              R O, the ſame let the inſcribed Figure
                <lb/>
              have to the Solid K: Which neceſſarily
                <lb/>
              ſhall be leſſer than the ſaid exceſs. </s>
              <s>And let
                <lb/>
              another Figure be inſcribed which may be
                <lb/>
              exceeded by the Conoid a leſs quantity
                <lb/>
              than is K, whoſe Center of Gravity falleth betwixt O and C. </s>
              <s>Let it
                <lb/>
              be V. And, becauſe the firſt Figure is to K as B R to R O, and the ſe­
                <lb/>
              cond Figure, whoſe Center V is greater than the firſt, and exceeded
                <lb/>
              by the Conoid a leſs quantity than is K; what proportion the ſecond
                <lb/>
              Figure hath to the exceſs by which the Conoid exceeds it, the ſame
                <lb/>
              ſhall a Line greater than B R have to R V. </s>
              <s>But R is the Center of Gra­
                <lb/>
              vity of the Conoid; and the Center of the ſecond inſcribed Figure V:
                <lb/>
              The Center therefore of the remaining proportions ſhall be without
                <lb/>
              the Conoid beneath B: Which is impoſſible. </s>
              <s>And by the ſame means
                <lb/>
              we might demonſtrate the Center of Gravity of the ſaid Conoid not to
                <lb/>
              be in the Line C A. </s>
              <s>And that it is none of the points betwixt C and
                <lb/>
              O is manifeſt. </s>
              <s>For ſay, that there other Figures deſcribed, greater
                <lb/>
              ſomething than the inſcribed Figure whoſe Center is O, and leſs than
                <lb/>
              that circumſcribed Figure whoſe Center is C, the Center of the Conoid
                <lb/>
              would fall without the Center of theſe Figures: Which but now was
                <lb/>
              concluded to be impoſſible: It reſts therefore that it be betwixt the Cen­
                <lb/>
              ter of the circumſcribed and inſcribed Figure. </s>
              <s>And if ſo, it ſhall ne­
                <lb/>
              ceſſarily be in that point which divideth the Axis, ſo as that the part
                <lb/>
              towards the Vertex is double to the remainder; ſince N may circum­
                <lb/>
              ſcribe and inſcribe Figures, ſo, that thoſe Lines which fall between
                <emph.end type="italics"/>
              </s>
            </p>
          </chap>
        </body>
      </text>
    </archimedes>