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

List of thumbnails

< >
221
221 		222
222
223
223 		224
224
225
225 		226
226
227
227 		228
228
229
229 		230
230
< >
page |< < of 701 > >|
    <archimedes>
      <text>
        <body>
          <chap>
            <p type="main">
              <s>
                <pb xlink:href="040/01/276.jpg" pagenum="256"/>
              underſtand the ſame, I have upon this paper tranſcribed the
                <lb/>
              cluſions that he inferreth from his twelve indagations; the firſt of
                <lb/>
              which is upon the two
                <lb/>
                <arrow.to.target n="table1"/>
              </s>
            </p>
            <p type="margin">
              <s>
                <margin.target id="marg510"/>
                <emph type="italics"/>
              The greateſt and
                <lb/>
              leaſt elevations of
                <lb/>
              the new ſtar differ
                <lb/>
              not from each
                <lb/>
              ther more than the
                <lb/>
              polar allitudes, the
                <lb/>
              ſaid ſtar being in
                <lb/>
              the Firmnment.
                <emph.end type="italics"/>
              </s>
            </p>
            <table>
              <table.target id="table1"/>
              <row>
                <cell>Of
                  <emph type="italics"/>
                Maurolicus
                  <emph.end type="italics"/>
                and
                  <emph type="italics"/>
                Hainzelius,
                  <emph.end type="italics"/>
                from which the Star is collected to have been diſtant from the centre leſſe than 3 ſemidiameters of the Earth, the difference of Parallaxes being 4
                  <emph type="italics"/>
                gr. 42 m.
                  <emph.end type="italics"/>
                30
                  <emph type="italics"/>
                ſec.
                  <emph.end type="italics"/>
                </cell>
                <cell>3
                  <emph type="italics"/>
                ſemid.
                  <emph.end type="italics"/>
                </cell>
              </row>
              <row>
                <cell>2. And is calculated on the obſervations of
                  <emph type="italics"/>
                Hain-zelius,
                  <emph.end type="italics"/>
                with Parall. of 8.
                  <emph type="italics"/>
                m. 30 ſec.
                  <emph.end type="italics"/>
                and its di-ſtance from the centre is computed to be more than</cell>
                <cell>25
                  <emph type="italics"/>
                ſemid.
                  <emph.end type="italics"/>
                </cell>
              </row>
              <row>
                <cell>3. And upon the obſervations of
                  <emph type="italics"/>
                Tycho
                  <emph.end type="italics"/>
                and
                  <emph type="italics"/>
                Hain-zelius,
                  <emph.end type="italics"/>
                with Parall. of 10
                  <emph type="italics"/>
                m.
                  <emph.end type="italics"/>
                and the diſtance of the centre is collected to be little leſſe than</cell>
                <cell>19
                  <emph type="italics"/>
                ſemid.
                  <emph.end type="italics"/>
                </cell>
              </row>
              <row>
                <cell>4. And upon the obſervations of
                  <emph type="italics"/>
                Tycho
                  <emph.end type="italics"/>
                and the
                  <emph type="italics"/>
                Landgrave,
                  <emph.end type="italics"/>
                with Parall. of 14
                  <emph type="italics"/>
                m.
                  <emph.end type="italics"/>
                the diſtance from the centre is made to be about</cell>
                <cell>10
                  <emph type="italics"/>
                ſemid.
                  <emph.end type="italics"/>
                </cell>
              </row>
              <row>
                <cell>5. And upon the obſervations of
                  <emph type="italics"/>
                Hainzelius
                  <emph.end type="italics"/>
                and
                  <emph type="italics"/>
                Gemma,
                  <emph.end type="italics"/>
                with Parall. of 42
                  <emph type="italics"/>
                m. 30 ſec.
                  <emph.end type="italics"/>
                whereby the diſtance is gathered to be about</cell>
                <cell>4
                  <emph type="italics"/>
                ſemid.
                  <emph.end type="italics"/>
                </cell>
              </row>
              <row>
                <cell>6. And upon the obſervations of the
                  <emph type="italics"/>
                Landgrave
                  <emph.end type="italics"/>
                and
                  <emph type="italics"/>
                Camerarius,
                  <emph.end type="italics"/>
                with Parall. of 8
                  <emph type="italics"/>
                m.
                  <emph.end type="italics"/>
                the di-ſtance is concluded to be about</cell>
                <cell>4
                  <emph type="italics"/>
                ſemid.
                  <emph.end type="italics"/>
                </cell>
              </row>
              <row>
                <cell>7. And upon the obſervations of
                  <emph type="italics"/>
                Tycho
                  <emph.end type="italics"/>
                and
                  <emph type="italics"/>
                Hage-cius,
                  <emph.end type="italics"/>
                with Parall. of 6
                  <emph type="italics"/>
                m.
                  <emph.end type="italics"/>
                and the diſtance is made</cell>
                <cell>31
                  <emph type="italics"/>
                ſemid.
                  <emph.end type="italics"/>
                </cell>
              </row>
              <row>
                <cell>8. And upon the obſervations of
                  <emph type="italics"/>
                Hagecius
                  <emph.end type="italics"/>
                and
                  <emph type="italics"/>
                Vr-ſinus
                  <emph.end type="italics"/>
                with Parall. of 43
                  <emph type="italics"/>
                m.
                  <emph.end type="italics"/>
                and the ſtars diſtance from the ſuperficies of the Earth is rendred</cell>
                <cell>1/2
                  <emph type="italics"/>
                ſemid.
                  <emph.end type="italics"/>
                </cell>
              </row>
              <row>
                <cell>9. And upon the obſervations of
                  <emph type="italics"/>
                Landgravius
                  <emph.end type="italics"/>
                and
                  <emph type="italics"/>
                Buſchius,
                  <emph.end type="italics"/>
                with Parall. of 15
                  <emph type="italics"/>
                m.
                  <emph.end type="italics"/>
                and the di-ſtance from the ſuperficies of the Earth is by ſupputation</cell>
                <cell>1/48
                  <emph type="italics"/>
                ſemid.
                  <emph.end type="italics"/>
                </cell>
              </row>
              <row>
                <cell>10. And upon the obſervations of
                  <emph type="italics"/>
                Maurolice
                  <emph.end type="italics"/>
                and
                  <emph type="italics"/>
                Munocius,
                  <emph.end type="italics"/>
                with Parall. of 4
                  <emph type="italics"/>
                m. 30 ſec.
                  <emph.end type="italics"/>
                and the compnted diſtance from the Earths ſurface is</cell>
                <cell>1/5
                  <emph type="italics"/>
                ſemid.
                  <emph.end type="italics"/>
                </cell>
              </row>
              <row>
                <cell>11. And upon the obſervations of
                  <emph type="italics"/>
                Munocius
                  <emph.end type="italics"/>
                and
                  <emph type="italics"/>
                Gemma,
                  <emph.end type="italics"/>
                with Parall. of 55
                  <emph type="italics"/>
                m.
                  <emph.end type="italics"/>
                and the diſtance from the centre is rendred</cell>
                <cell>13
                  <emph type="italics"/>
                ſemid.
                  <emph.end type="italics"/>
                </cell>
              </row>
            </table>
          </chap>
        </body>
      </text>
    </archimedes>
Impressum