Huygens, Christiaan, Christiani Hugenii opera varia; Bd. 1: Opera mechanica

Page concordance

< >
Scan Original
271
272
273 171
274 172
275 173
276 174
277 175
278 176
279 177
280 178
281 179
282 180
283 181
284 182
285 183
286 184
287 185
288 186
289 187
290 188
291
292
293
294 189
295 190
296 191
297 192
298
299
300
< >
page |< < (231) of 434 > >|
    <echo version="1.0RC">
      <text xml:lang="la" type="free">
        <div xml:id="echoid-div432" type="section" level="1" n="176">
          <pb o="231" file="0309" n="336" rhead="CONTROVERSIA."/>
          <p>
            <s xml:id="echoid-s5048" xml:space="preserve">Sint A & </s>
            <s xml:id="echoid-s5049" xml:space="preserve">B duo corpora ex Axe D ſuſpenſa ita, ut unius
              <lb/>
              <note position="right" xlink:label="note-0309-01" xlink:href="note-0309-01a" xml:space="preserve">TAB. XXVIII.
                <lb/>
              Fig. 4.</note>
            diſtantia ab Axe quadruplo major ſit alterius diſtantiâ.</s>
            <s xml:id="echoid-s5050" xml:space="preserve"/>
          </p>
          <p>
            <s xml:id="echoid-s5051" xml:space="preserve">Adeoque ſi altitudo perpendicularis B I, ex qua deſcendit
              <lb/>
            corpus B deſcribendo arcum B G, ponatur quatuor pedum,
              <lb/>
            altera A H, unde corpus A delabitur, unius pedis erit.
              <lb/>
            </s>
            <s xml:id="echoid-s5052" xml:space="preserve">Celeritates igitur, quas ſeparatim cadendo acquirunt, quo-
              <lb/>
            niam ſunt ut radices altitudinum, ſe habent ut 2 ad 1. </s>
            <s xml:id="echoid-s5053" xml:space="preserve">Summa
              <lb/>
            3, quæ totalem Penduli celeritatem manifeſtat, quando pro-
              <lb/>
            portionaliter ad altitudines, ſive ad arcus B G & </s>
            <s xml:id="echoid-s5054" xml:space="preserve">A F divi-
              <lb/>
            ditur, dat gradus celeritatis, quos obtinent pondera, quan-
              <lb/>
            do conjunctim in tabulam D G decidunt, videlicet {12/5} & </s>
            <s xml:id="echoid-s5055" xml:space="preserve">{3/5},
              <lb/>
            quorum quadrata ſunt {144/25} & </s>
            <s xml:id="echoid-s5056" xml:space="preserve">{9/25}, unde quæ prodit ſumma,
              <lb/>
            ſane a ſumma altitudinum, e quibus pondera dimittuntur,
              <lb/>
            differt. </s>
            <s xml:id="echoid-s5057" xml:space="preserve">Veruntamen hæc quadrata proportionem ſolummodo
              <lb/>
            altitudinum O M & </s>
            <s xml:id="echoid-s5058" xml:space="preserve">N L, ad quas pondera, dum a tabula
              <lb/>
            reſiliunt, adſcendunt, non ipſas altitudines exprimunt; </s>
            <s xml:id="echoid-s5059" xml:space="preserve">quas
              <lb/>
            inter ratio quidem eſſe poteſt, quæ eſt inter {144/25} & </s>
            <s xml:id="echoid-s5060" xml:space="preserve">{9/25}, hoc eſt
              <lb/>
            inter 16 & </s>
            <s xml:id="echoid-s5061" xml:space="preserve">1, dum ipſa ſumma eſt quinque, quæ eſt ſum-
              <lb/>
            ma altitudinum B I & </s>
            <s xml:id="echoid-s5062" xml:space="preserve">A H unde pondera delapſa ſunt.</s>
            <s xml:id="echoid-s5063" xml:space="preserve"/>
          </p>
          <p>
            <s xml:id="echoid-s5064" xml:space="preserve">Nam ſi ponamus altitudinem O M 4{17/1@} pedum eſſe, & </s>
            <s xml:id="echoid-s5065" xml:space="preserve">alte-
              <lb/>
            ram N L {5/17}, O M ſe habebit ad N L, ut 16 ad 1; </s>
            <s xml:id="echoid-s5066" xml:space="preserve">& </s>
            <s xml:id="echoid-s5067" xml:space="preserve">O M
              <lb/>
            † N L erit æqualis B I † A H. </s>
            <s xml:id="echoid-s5068" xml:space="preserve">Idcirco centrum gravitatis
              <lb/>
            commune ponderum A & </s>
            <s xml:id="echoid-s5069" xml:space="preserve">B, ubi in L, M pervenere, erit
              <lb/>
            ad eandem altitudinem, quam obtinebat ante Oſcillationis ini-
              <lb/>
            tium. </s>
            <s xml:id="echoid-s5070" xml:space="preserve">Id clare ex inſpectione figuræ apparet. </s>
            <s xml:id="echoid-s5071" xml:space="preserve">Pondus enim
              <lb/>
            M tantum ſupra lineam Horizontalem B D elevatur, quan-
              <lb/>
            tum L infra eam deprimitur, videlicet {12/17} unius pedis; </s>
            <s xml:id="echoid-s5072" xml:space="preserve">ſe-
              <lb/>
            quitur hinc in triangulis ſimilibus M P Q & </s>
            <s xml:id="echoid-s5073" xml:space="preserve">L Q R latera
              <lb/>
            M Q & </s>
            <s xml:id="echoid-s5074" xml:space="preserve">Q L eſſe æqualia, hoc eſt medium lineæ M L, quæ
              <lb/>
            duo pondera conjungit, eſſe in interſectione lineæ Horizon-
              <lb/>
            talis.</s>
            <s xml:id="echoid-s5075" xml:space="preserve"/>
          </p>
          <figure number="135">
            <image file="0309-01" xlink:href="http://echo.mpiwg-berlin.mpg.de/zogilib?fn=/permanent/library/xxxxxxxx/figures/0309-01"/>
          </figure>
        </div>
      </text>
    </echo>