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

Page concordance

< >
Scan Original
211 133
212 134
213 135
214 136
215
216
217
218 137
219 138
220 139
221 140
222 141
223 142
224
225
226
227 143
228 144
229 145
230 146
231 147
232 148
233 149
234 150
235 151
236 152
237 153
238 154
239
240
< >
page |< < (151) of 434 > >|
    <echo version="1.0RC">
      <text xml:lang="la" type="free">
        <div xml:id="echoid-div297" type="section" level="1" n="108">
          <p>
            <s xml:id="echoid-s3404" xml:space="preserve">
              <pb o="151" file="0215" n="235" rhead="HOROLOG. OSCILLATOR."/>
            quæque ſuſpenſa ab axe, qui per punctum F ad planum hu-
              <lb/>
              <note position="right" xlink:label="note-0215-01" xlink:href="note-0215-01a" xml:space="preserve">
                <emph style="sc">De centro</emph>
                <lb/>
                <emph style="sc">OSCILLA-</emph>
                <lb/>
                <emph style="sc">TIONIS</emph>
              .</note>
            jus paginæ erectus intelligitur, habeat centrum oſcillationis
              <lb/>
            G. </s>
            <s xml:id="echoid-s3405" xml:space="preserve">Porrò axi per F intelligatur axis alius, per centrum gra-
              <lb/>
            vitatis E transiens, parallelus. </s>
            <s xml:id="echoid-s3406" xml:space="preserve">Diviſaque magnitudine cogita-
              <lb/>
            tu in particulas minimas æquales, ſit quadratis diſtantiarum,
              <lb/>
            ab axe dicto per E, æquale planum I, multiplex nempe ſe-
              <lb/>
            cundum numerum dictarum particularum; </s>
            <s xml:id="echoid-s3407" xml:space="preserve">applicatoque pla-
              <lb/>
            no I ad diſtantiam F E, fiat recta quædam. </s>
            <s xml:id="echoid-s3408" xml:space="preserve">Dico eam æ-
              <lb/>
            qualem eſſe intervallo E G, quo centrum oſcillationis infe-
              <lb/>
            rius eſt centro gravitatis magnitudinis A B C D.</s>
            <s xml:id="echoid-s3409" xml:space="preserve"/>
          </p>
          <p>
            <s xml:id="echoid-s3410" xml:space="preserve">Ut enim univerſali demonſtratione quod propoſitum eſt
              <lb/>
            comprehendamus: </s>
            <s xml:id="echoid-s3411" xml:space="preserve">intelligatur plana figura, magnitudini
              <lb/>
            A B C D analoga, ad latus adpoſita, O Q P; </s>
            <s xml:id="echoid-s3412" xml:space="preserve">quæ nempe,
              <lb/>
            ſecta planis horizontalibus iisdem cum magnitudine A B C D,
              <lb/>
            habeat ſegmenta intercepta inter bina quæque plana, in ea-
              <lb/>
            dem inter ſe ratione cum ſegmentis dictæ magnitudinis, quæ
              <lb/>
            ipſis reſpondent; </s>
            <s xml:id="echoid-s3413" xml:space="preserve">ſintque ſegmenta ſingula figuræ O Q P,
              <lb/>
            diviſa in tot particulas æquales, quot continentur ſegmentis
              <lb/>
            ipſis reſpondentibus in figura A B C D. </s>
            <s xml:id="echoid-s3414" xml:space="preserve">Hæc autem intel-
              <lb/>
            ligi poſſunt fieri, qualiscunque fuerit magnitudo A B C D,
              <lb/>
            ſive linea, ſive ſuperficies, ſive ſolidum. </s>
            <s xml:id="echoid-s3415" xml:space="preserve">Semper vero cen-
              <lb/>
            trum gravitatis figuræ O Q P, quod ſit T, eadem altitu-
              <lb/>
            dine eſſe manifeſtum eſt cum centro gravitatis magnitudinis
              <lb/>
            A B C D; </s>
            <s xml:id="echoid-s3416" xml:space="preserve">ideoque, ſi planum horizontale, per F ductum,
              <lb/>
            ſecet lineam centri figuræ O Q P, velut hic in S, æquales
              <lb/>
            eſſe diſtantias S T, F E.</s>
            <s xml:id="echoid-s3417" xml:space="preserve"/>
          </p>
          <p>
            <s xml:id="echoid-s3418" xml:space="preserve">Porrò autem conſtat quadrata diſtantiarum, ab axe oſcil-
              <lb/>
            lationis F, applicata ad diſtantiam F E, multiplicem ſecun-
              <lb/>
            dum numerum particularum, efficere longitudinem penduli
              <lb/>
            iſochroni ; </s>
            <s xml:id="echoid-s3419" xml:space="preserve">quæ longitudo poſita fuit F G. </s>
            <s xml:id="echoid-s3420" xml:space="preserve">Illorum
              <note symbol="*" position="right" xlink:label="note-0215-02" xlink:href="note-0215-02a" xml:space="preserve">Prop. 6.
                <lb/>
              huj.</note>
            quadratorum ſummam, æqualem eſſe perſpicuum eſt, qua-
              <lb/>
            dratis diſtantiarum à plano horizontali per F, unà cum qua-
              <lb/>
            dratis diſtantiarum à plano verticali F E, per axem F & </s>
            <s xml:id="echoid-s3421" xml:space="preserve">cen-
              <lb/>
            trum gravitatis E ducto . </s>
            <s xml:id="echoid-s3422" xml:space="preserve">Atqui quadrata diſtantiarum
              <note symbol="*" position="right" xlink:label="note-0215-03" xlink:href="note-0215-03a" xml:space="preserve">Prop. 47.
                <lb/>
              lib. 1. Eucl.</note>
            gnitudinis A B C D à plano horizontali per F, æquantur
              <lb/>
            quadratis diſtantiarum figuræ O Q P ab recta S F. </s>
            <s xml:id="echoid-s3423" xml:space="preserve"/>
          </p>
        </div>
      </text>
    </echo>