Gassendi, Pierre, De motu impresso a motore translato epistulae duae, 1642

Page concordance

< >
Scan Original
111
112
113
114
115
116
117
118
119
120
121
122
123
124
125
126
127
128
129
130
131
132
133
134
135
136
137
138
139
140
< >
page |< < of 158 > >|
    <archimedes>
      <text>
        <body>
          <chap>
            <p type="main">
              <s id="id.000864">
                <pb pagenum="133" xlink:href="027/01/132.jpg"/>
              tro deſcribat, qui Ecliptica linea dicitur, hæc ipſa
                <lb/>
              erit linea, quam Sol deſcribet apparenter; adeò
                <lb/>
              vt non modò aliorum Planetarum latitudines, con­
                <lb/>
              figurationeſque eodem modo eueniant, ſiue Sol
                <lb/>
              reipſa moueatur, ſiue moueri ſolum appareat; ſed
                <lb/>
              eodem quoque modo Eclipſes tam Solis, quàm
                <lb/>
              Lunæ contingant. </s>
              <s id="id.000865">Quippe cùm Luna motu men­
                <lb/>
              ſtruo ipſi Terræ circumferatur; efficitur eadem ra­
                <lb/>
              tione, vt Terræ, ac Soli directè interpoſita lucem
                <lb/>
              Terræ eripiat; & Terram habens ſibi, ac Soli dire­
                <lb/>
              ctè interpoſitam, eádem Solis luce per Terram pri­
                <lb/>
              uetur. </s>
              <s id="id.000866">Nimirùm eadem inclinatione deſcribere po­
                <lb/>
              teſt orbitam, quæ Eclipticam à Terra deſcriptam
                <lb/>
              duobus in locis interſecet, nodoſque Eclipticos fa­
                <lb/>
              ciat. </s>
              <s id="id.000867">Neque videtur morari debere nos P
                <emph type="italics"/>
              rimò,
                <emph.end type="italics"/>
                <lb/>
              quod abſurdum eſſe videatur, fore ergo Terram
                <lb/>
              vnum ex Planetis, & magis quidem præcipuum,
                <lb/>
              quàm Lunam, eo modo, quo Iupiter eſt præ ſuis
                <lb/>
              Lunis Mediceis præcipuus. </s>
              <s id="id.000868">Siquidem Terra glo­
                <lb/>
              boſa eſt, ſicut Planetæ cæteri; comparata eſt ad
                <lb/>
              motum, vt illi; lucem Solis perinde excipit, re­
                <lb/>
              flectitque, & per illam, non ſecùs quàm illi, collu­
                <lb/>
              cet: quemadmodùm probat lux illa debilior, quæ
                <lb/>
              in Luna tam recente, quàm ſeneſcente obſeruatur,
                <lb/>
              quámque non aliunde eſſe, quàm à Terra per­
                <lb/>
              ſpicuum videtur vel ex eo, quod quando Luna
                <lb/>
              poſt primam & ante ſecundam quadraturam procul
                <lb/>
              eſt à loco reflexionis lucis Solaris, quæ à Terra
                <lb/>
              ſemper verſus Solem ſit, tum Luna ea luce omninô
                <lb/>
              priuatur. </s>
              <s id="id.000869">Prætereà locus congruus inter Venerem </s>
            </p>
          </chap>
        </body>
      </text>
    </archimedes>
Impressum