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

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        <body>
          <chap>
            <p type="main">
              <s id="s.000285">
                <pb pagenum="24" xlink:href="025/01/028.jpg"/>
              ctus in Perigæo, à circulo decurſo in Apogæo ; Eſt enim minor propor­
                <lb/>
              tio vnius ad alium; hinc per plures dies ſtare videtur; quia licèt reipſa
                <lb/>
              non ſtet, tam parum tamen promovetur & recedit à Stella, seu versùs
                <lb/>
              Ortum, ſeu versùs Occaſum, vt eandem à Stella diſtantiam ſervare vi­
                <lb/>
              deatur; Cuncta hæc ita perſpicua ſunt, vt negari profectò non poſſint, quale
                <lb/>
              do vltrò in hac tua hypotheſi, huiuſmodi paſſiones Planetarum æquè facilè
                <lb/>
              explicari atque in mea. </s>
            </p>
            <p type="main">
              <s id="s.000286">
                <emph type="italics"/>
              Antim.
                <emph.end type="italics"/>
              </s>
              <s id="s.000287"> Imò longè faciliùs & cum multiplici prærogativa: Nam pri­
                <lb/>
              mò ſimpliciſſimum motum adhibeo; realem ſcilicet & æquabilem, circa
                <lb/>
              mundi Centrum; tu verò duos, & fortè plures, eóſque minimè æquabi­
                <lb/>
              les; vtrumque in Excentrico circa centra ad libitum excogitata & ficta.
                <lb/>
              </s>
              <s id="s.000288">Secundo, nunquam vides Planetam extrà Perigæum & Apogæum, in eo
                <lb/>
              vero loco in quo eſt, ac proinde perpetuæ fallaciæ ſubjaces; ego in eo
                <lb/>
              loco, in quo reverà eſt, Planetam video. </s>
              <s id="s.000289">Tertiò, tu ſenſum decipi
                <lb/>
              aſſeris, quamvis rectè applicatum; ego vt & in aliis minimè falli repo­
                <lb/>
              no, nec quiſquam hoc jure adſtruat, niſi aliqua ratione fretus. </s>
              <s id="s.000290">Quartò;
                <lb/>
              denique habeo in mea cauſas Phyſicas, eáſque tritas & vulgares in doctri­
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              na motuum, iſtorum omnium effectuum, Apogæi ſcilicet, Perigæi, accelera­
                <lb/>
              tionis, retardationis, &c. </s>
              <s id="s.000291">Tu verò meras fallacias, & oculorum illuſiones
                <lb/>
              eſſe contendis. </s>
              <s id="s.000292">Igitur non æquè facilè in tua hypotheſi, ac in mea, res iſta ex­
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              plicatur, ſed in mea longè faciliùs, planiùs, &, vt ſic loquar, connaturaliùs. </s>
            </p>
            <p type="main">
              <s id="s.000293">
                <emph type="italics"/>
              Auguſtin.
                <emph.end type="italics"/>
              </s>
              <s id="s.000294"> Vt vt ſit, quoad hæc, antequam ad alia, quæ fortè magis vrgent,
                <lb/>
              accedam, ex te ſcire vellem, quonam modo latitudinem Planetarum in tua
                <lb/>
              hypotheſi explices; quod eò libentiùs audiam, quò mirabilior mihi videtur
                <lb/>
              ille modus, quo in hypotheſi noſtra explicatur; in qua ſuppoſita orbitæ ex­
                <lb/>
              centricæ Planetæ inclinatione ad planum Eclypticæ, latitudinis variatio per
                <lb/>
              diverſum terræ mobilis
                <expan abbr="ſitũ">ſitum</expan>
              optimè explicatur; nempè arcus, qui maximam
                <lb/>
              latitudinem metitur, in limitibus ſub majore vel minore angulo apparet,
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              quo remotior, vel propior oculus ſtatuetur; quod vt in ſchemate explicem,
                <lb/>
                <figure id="id.025.01.028.1.jpg" xlink:href="025/01/028/1.jpg" number="8"/>
                <lb/>
              Sit centrum mundi A, planum ecli­
                <lb/>
              pticæ EGKH, excentricus FGI
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              H, cuius centrum eſt in D ; nodi G
                <lb/>
              H, arcus inclinationis excentrici F
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              E, IK, Telluris orbita BLCM.
                <lb/>
              </s>
              <s id="s.000295">Sit Terra in B, Planeta in limite Bo­
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              reali F ; apparebit prædictus arcus
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              ſub angulo FBE, poſita verò Terra
                <lb/>
              in C, apparebit ſub angulo FCE,
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              qui priore minor eſt; Si verò ſtatua­
                <lb/>
              tur in limite Auſtrali, I & Terra ſit
                <lb/>
              in C, videbitur arcus IK ſub an­
                <lb/>
              gulo ICK, & ex B ſub angulo
                <lb/>
              IBK, ſed ex Optica, perſpi­
                <lb/>
              cuum eſt, angulum ICK majorem
                <lb/>
              eſſe angulo FBE, quia CI minor </s>
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