Casati, Paolo, Terra machinis mota : dissertationes geometricae, mechanicae physicae hydrostaticae

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              <s>
                <pb xlink:href="018/01/041.jpg" pagenum="33"/>
              totum hoc ſpa­
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                <figure id="id.018.01.041.1.jpg" xlink:href="018/01/041/1.jpg" number="13"/>
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              tium illud eſt,
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              cui Sol ad per­
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              pendiculum im­
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              minet. </s>
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            <p type="margin">
              <s>
                <margin.target id="note18"/>
                <emph type="italics"/>
              XVII
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              Terræ ma­
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              gnitudinem
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              eiuſque ad
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              Solem pro­
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              portionem̨
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              inueſtigare
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              ex ſpatio,
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              quod umbris
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              caret.
                <emph.end type="italics"/>
              </s>
            </p>
            <p type="main">
              <s>Sed
                <expan abbr="quærendũ">quærendum</expan>
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              ſupererat, quo­
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              ta totius circuli
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              maximi pars eſ­
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              ſent ſtadia 300.
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              Conſtituto ita­
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              que terræ centro
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              in C, & oculo
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              obſeruatoris iņ
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              O, ductum
                <expan abbr="in-telligebã">in­
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                telligebam</expan>
              ex cen­
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              tro S radium S
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              OC, qui cum̨
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              radio OT Solem
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              contingente da­
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              bat angulum S
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              OT ſemidiametrum apparentem Solis Apo­
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              gæi gr.o.m.15., vt placet Tychoni, Longo­
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              montano, Magino, Keplero. </s>
              <s>Item ex C du­
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              ctus intelligatur radius Solem tangens, qui
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              terræ circulum maximum ſecat in K; & eſt
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              OK ſemiſsis ſpatij, quod caret vmbris meri­
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              dianis die ſolſtitij æſtiui; continet autem ſta­</s>
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