Fabri, Honoré, Tractatus physicus de motu locali, 1646

Page concordance

< >
Scan Original
31
32
33
34
35
36
37
38
39
40
41
42
43
44
45
46
47
48
49
50
51
52
53
54
55
56
57
58
59
60
< >
page |< < of 491 > >|
    <archimedes>
      <text>
        <body>
          <chap id="N15AC3">
            <pb pagenum="107" xlink:href="026/01/139.jpg"/>
            <p id="N177E0" type="main">
              <s id="N177E2">Si verò in noſtra hypotheſi ſpatium, quod reſpondet primæ parti tem­
                <lb/>
              poris AC ſit idem cum illo, quod reſpondet eidem parti in ſententia
                <lb/>
              Galilei, id eſt æquale triangulo CAG, ſumma ſpatiorum erit minor in
                <lb/>
              noſtra hypotheſi triangulo AFN ſex triangulis æqualibus triangulo
                <lb/>
              ACG; igitur erit vt 10.ad 16. igitur minor 1/8. </s>
              <s id="N177EE">ſi verò diuidantur in 8.
                <lb/>
              temporis partes, triangulum AFN continebit 64. triangula æqualia
                <lb/>
              AXQ: </s>
              <s id="N177F6">at verò ſumma quæ reſpondet noſtræ hypotheſi 36.igitur minor
                <lb/>
              (7/16). denique ſi diuidantur in 16. partes, triangulum AFN continebit
                <lb/>
              256. triangula æqualia AYZ; at verò ſumma noſtra 136. igitur minor
                <lb/>
              (15/52) ſed nunquam erit minor 1/2. </s>
            </p>
            <p id="N17800" type="main">
              <s id="N17802">Obſeruabis obiter dictum eſſe ſuprà ſummam rectangulorum CB CI
                <lb/>
              EK EN eſſe maiorem triangulo AFN, 2.quadratis æqualibus CB; </s>
              <s id="N17808">ſi
                <lb/>
              verò diuidatur tempus in 8. partes, ſumma rectangulorum eſt minor præ­
                <lb/>
              cedenti ſummâ, toto quadrato æquali CB, id eſt 4.quadratis æqualibus
                <lb/>
              XB, id eſt 1/2 primæ differentiæ, quæ eſt ſumma duorum quadratorum
                <lb/>
              æqualium CB; </s>
              <s id="N17814">at ſi diuidatur in 16. partes, tempus AF, ſumma rectan­
                <lb/>
              gulorum eſt minor præcedente 8. quadratis æqualibus QZ, vel ſubdu­
                <lb/>
              plo quadrati CB, id eſt 1/4 primæ differentiæ quæ eſt ſumma duorum
                <lb/>
              quadratorum æqualium CB; </s>
              <s id="N1781E">ſi 4. partes temporis diuidantur in 8. de­
                <lb/>
              trahitur 1/2 differentiæ, quæ eſt inter ſummam primam rectangulorum,
                <lb/>
              & triangulum AFN; </s>
              <s id="N17826">ſi diuidantur in 16. detrahitur 1/4 eiuſdem diffe­
                <lb/>
              rentiæ; </s>
              <s id="N1782C">ſi diuidantur in 32. detrahitur 1/8, ſi in 64. (1/16); </s>
              <s id="N17830">atque ita deinceps,
                <lb/>
              & nunquam hæ minutiæ ſubtractæ in infinitum totam differentiam ex­
                <lb/>
              haurient; hinc minutiæ iſtæ 1/2 1/4 1/8 (1/16) (1/32) (1/64) &c. </s>
              <s id="N17838">in infinitum non fa­
                <lb/>
              ciunt vnum integrum; ſed hæc ſunt facilia. </s>
            </p>
            <p id="N1783E" type="main">
              <s id="N17840">Quarta ratio, quam afferunt aliqui, eſt; </s>
              <s id="N17844">quia ſi cum eadem velocita­
                <lb/>
              te acquiſita in fine temporis dati ſine augmento nouo moueatur mobi­
                <lb/>
              le; </s>
              <s id="N1784C">haud dubiè acquiret duplum ſpatium tempore æquali tempori dato; </s>
              <s id="N17850">
                <lb/>
              v. g. ſit triangulum AFE; </s>
              <s id="N17859">ſitque velocitas acquiſita EF in 4. parti­
                <lb/>
              bus temporis AE, vt iam ſuprà dictum eſt, ne cogar repetere: </s>
              <s id="N1785F">certè ſi du­
                <lb/>
              catur velocitas EF in tempus AE, vel EL æquale; </s>
              <s id="N17865">habebitur rectan­
                <lb/>
              gulum EK duplum trianguli AFE: </s>
              <s id="N1786B">ſed triangulum AFE eſt ſumma
                <lb/>
              ſpatiorum motus accelerati tempore AE, & rectangulum EK eſt ſum­
                <lb/>
              ma ſpatiorum motus æquabilis cum velocitate EF; igitur duplum eſt
                <lb/>
              ſpatium motus æquabilis, quod erat demonſtrandum. </s>
              <s id="N17875">Præterea ſi diui­
                <lb/>
              datur velocitas EF, & eius ſubdupla ducatur in tempus AE; habebitur
                <lb/>
              rectangulum æquale triangulo AFE, vt conſtat. </s>
              <s id="N1787D">Reſpondeo facilè ex di­
                <lb/>
              ctis, hoc ipſum etiam ex noſtra hypotheſi proxime ſequi; </s>
              <s id="N17883">ſint enim duo
                <lb/>
              inſtantia; </s>
              <s id="N17889">haud dubie ſi non creſcit velocitas, ſecundo inſtanti æquale
                <lb/>
              ſpatium percurretur; </s>
              <s id="N1788F">ſi vero ſecundo inſtanti creſcat, percurrentur illo
                <lb/>
              motu 3.ſpatia; </s>
              <s id="N17895">& cùm velocitas
                <expan abbr="ſecũdi">ſecundi</expan>
                <expan abbr="inſtãtis">inſtantis</expan>
              ſit dupla velocitatis primi
                <lb/>
              inſtantis, primo inſtanti ſit 1.gradus v.g. ſecundo erunt 2. gradus; </s>
              <s id="N178A5">igi­
                <lb/>
              tur moueatur per duo inſtantia motu æquabili veloci vt 2. percurrentur
                <lb/>
              4. ſpatia; </s>
              <s id="N178AD">igitur totum ſpatium, quod percurritur motu veloci vt 2. per
                <lb/>
              2.inſtantia eſt ad totum ſpatium, quod percurritur æquali tempore mo-</s>
            </p>
          </chap>
        </body>
      </text>
    </archimedes>