Fabri, Honoré, Dialogi physici in quibus de motu terrae disputatur, 1665

List of thumbnails

< >
11
11
12
12
13
13
14
14
15
15
16
16
17
17
18
18
19
19
20
20
< >
page |< < of 248 > >|
    <archimedes>
      <text>
        <body>
          <chap>
            <p type="main">
              <s id="s.000195">
                <pb pagenum="15" xlink:href="025/01/019.jpg"/>
              Sol Martem aſſequitur; hinc Martem occultari neceſſe eſt; quia verò
                <lb/>
              poſt aliquod tempus, Sol à Perigæo, & Mars ab Apogæo recedunt, Mars
                <lb/>
              citiùs ſuos orbes decurrit; hinc Solem poſt ſe relinquit; hinc demum
                <lb/>
              emergit. </s>
              <s id="s.000196">Si hoc phænomenum verum eſt, vix puto aliam illius cauſam
                <lb/>
              aſſignari poſſe; ſed vt iam indicavi, Kepleri dictis parum fidei haben­
                <lb/>
              dum eſſe putarem; præterquàm quòd fieri potuit, vt craſſiores vapores
                <lb/>
              Martem circa horizontem ortivum oculis ſubduxerint per aliquot dies,
                <lb/>
              quibus deinde diſcuſſis, ſeſe iterum Planeta videndum præbuerit, ac
                <lb/>
              proinde non fuerit vera immerſio, vel emerſio; Vt vt ſit, nec enim de
                <lb/>
              hoc laboramus, ſi phænomenum verum eſt, in noſtra etiam hypotheſi
                <lb/>
              ſua cauſa & ratione non caret, & vix ſcio, quonam pacto in veſtra ex­
                <lb/>
              plicari poſſit. </s>
            </p>
            <p type="main">
              <s id="s.000197">
                <emph type="italics"/>
              Auguſtin.
                <emph.end type="italics"/>
              </s>
              <s id="s.000198"> Rectè omnia explicas,
                <emph type="italics"/>
              Antime,
                <emph.end type="italics"/>
              nec etiam dubito, quin
                <lb/>
              ablegato etiam veſtro Epicyclo, retardationem, accelerationem, retro
                <lb/>
              gradationem, ſtationem Martis explices; ſupponamus enim, Martei
                <lb/>
              motu ſemper æquabili ſuos agere orbes, cum maiorem circulum deſcri
                <lb/>
              bat in Apogæo, & minorem in Perigæo, hunc citiùs, tardiùs illum per
                <lb/>
              ficit; Supponamus autem, versùs Apogæum ſuum orbem decurrere tar­
                <lb/>
              diùs, quàm ſtellas, citiùs verò verſus Perigæum; haud dubiè versùs Apo­
                <lb/>
              gæum, longè retro à ſtellis relinquitur versùs ortum, vnde progredi vi
                <lb/>
              detur in conſequentia ſignorum, idque maiore intervallo, quò propiùs
                <lb/>
              ad Apogæum accedit; minore verò, quo longiùs ab eo recedit; at verò
                <lb/>
              versùs Perigæum ſtellas verſus ortum poſt ſe relinquit; igitur versùs oc­
                <lb/>
              caſum progredi videtur, id eſt, à ſtella recedere, quod retrogredi vocant;
                <lb/>
              vbi demum ſuum orbem æquè citò conficit atque ſtella, ſtare dicitur: Hæc
                <lb/>
              ſatis bene intelligo, etiam, ex principiis Phyſicis, quæ per optica tan­
                <lb/>
              tùm in noſtra hypotheſi, explicantur; nonnulla tamen à te ſcire deſide­
                <lb/>
              ro, v. g. vtrùm Mars in mediocri diſtantia citiùs ſuum orbem decurrat,
                <lb/>
              quàm ſtellæ, an verò tardiùs; deinde, cur Mars ſit retrogradus breuiori
                <lb/>
              tempore, & longiore directus; cur ab Apogæo ad Quadraturam plus
                <lb/>
              temporis ponat, quàm ab iſta ad Perigæum. </s>
            </p>
            <p type="main">
              <s id="s.000199">
                <emph type="italics"/>
              Antim.
                <emph.end type="italics"/>
              </s>
              <s id="s.000200"> Mars haud dubiè in mediocri diſtantia tardiùs ſuum orbem
                <lb/>
              quàm ſtellæ, & non procul à Perigæo æquè citò illum decurrit; vnde
                <lb/>
              non mirum eſt, ſi cum ab vna coniunctione ad aliam dies circiter 780. ſeu
                <lb/>
              revolutiones ſpirales intercurrant, ſit directus in 705. retrogradus in 73.
                <lb/>
              in 2. demum ſtationarius. </s>
              <s id="s.000201">Si autem in mediocri diſtantia ſuum orbem
                <lb/>
              æquè citò ac ſtella conficeret, æque diu eſſet retrogradus, ac </s>
              <s id="s.000202">directus;
                <lb/>
              ac proinde nunquam ad oppoſitionem pervenire poſſet, & in Perigæo
                <lb/>
              eſſet etiam Soli coniunctus, vt Venus; vnde parum omnino regreditur,
                <lb/>
              ſi obſervationes conſulamus, quibus haud dubiè ſtandum eſt, non verò
                <lb/>
              fictitio Syſtemati. </s>
            </p>
            <p type="main">
              <s id="s.000203">
                <emph type="italics"/>
              Auguſtin.
                <emph.end type="italics"/>
              </s>
              <s id="s.000204"> Syſtema ex obſeruationibus ſtatuitur, ac proinde his ſtan­
                <lb/>
              tibus, ſyſtema etiam ſtare neceſſe eſt. </s>
            </p>
            <p type="main">
              <s id="s.000205">
                <emph type="italics"/>
              Antim.
                <emph.end type="italics"/>
              </s>
              <s id="s.000206"> Vis liberè dicam, quod ſentio; cum ex multis obſervationi­
                <lb/>
              bus ſyſtema ſtatuatur, eo ſemel ſtatuto, reliquas ad illud vt plurimùm </s>
            </p>
          </chap>
        </body>
      </text>
    </archimedes>