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

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              <s id="s.000936">
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              fuit, antequam motu circulari moveretur ad Eclipticam, eo modo, quo iam
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              ſupra dictum eſt. </s>
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            <p type="main">
              <s id="s.000937">
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              Auguſtin.
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              </s>
              <s id="s.000938"> Qua quæſo linea, curva an recta? </s>
              <s id="s.000939">deinde an perpen­
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              diculariter cadente in planum Eclipticæ? </s>
              <s id="s.000940">an verò in planum Æqua­
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              toris? </s>
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            <p type="main">
              <s id="s.000941">
                <emph type="italics"/>
              Antim.
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              </s>
              <s id="s.000942"> Ad vtrumque reſpondeo; ad primum quidem, per curvam fieri;
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              vt dixi de Sole v.g. per arcum D.
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              F, vt eandem retineat à centro
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              mundi diſtantiam, vi ſcilicet hujus
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              motus, ſeu inclinationis; quænam
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              verò ſit accelerationis ratio à D ver­
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              sùs F, iam ſupra indicavi. </s>
              <s id="s.000943">Suppone
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              horizontale planum AF & ſuperfi­
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              ciem ſphæræ inclinatam DF, in
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              qua deſcendat corpus grave motu
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              accelerato, hæc eſt accelerationis
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              progreſſio; quæ in ſecundam incli­
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              nationem apprimè quadrat;
                <expan abbr="quænã">quænam</expan>
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              porrò & qualis ſit hæc progreſſio
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              motus accelerati, altioris eſt indagi­
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              nis; Licèt enim
                <expan abbr="eadẽ">eadem</expan>
                <expan abbr="nõ">non</expan>
              ſit cum illa,
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              quam ſervant funependula in de­
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              ſcenſu, ab ea tamen petenda eſt;
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              Vt vt ſit, hæc diſcuſſio hujus noſtri
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              inſtituti non eſt, ad ſecundum re­
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              ſpondeo, Lineam illam cadere per­
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              pendiculariter in planum Æquato­
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              ris,
                <expan abbr="nẽpe">nempe</expan>
              determinatur à Plano cir­
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              culi parallelo Plano Æquatoris, eius
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              tamen terminus eſt Ecliptica, vt di­
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              xi; nempe Plánetæ hinc terram aſpi­
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              ciunt, cui ſerviunt, lumenque refun­
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              dunt; inde verò Solem, ſub primo reſpectu, ſuos orbes agunt circa -
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              terram, tanquam circa ſuum centrum; ſub alio verò, Solis ſequun­
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              tur veſtigia, qui cùm ab Ecliptica nunquam diſcedat, hic ſolus circulus
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              ſecundam inclinationem Planetarum tanquam terminus determinat. </s>
              <s id="s.000944">Ex
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              his autem perſpicuas rationes reddo, in mea hypotheſi, acceleratio­
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              nis, retardationis, retrogreſſionis, ſtationis, Nodorum motus, itemque
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              Apogæi & Perigæi, variæ digreſſionis & latitudinis, vt jam ſupra indicavi­
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              mus. </s>
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            <p type="main">
              <s id="s.000945">
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              Chryſoc.
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              </s>
              <s id="s.000946"> Antequam alia argumenta expromas, per te mihi liceat,
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              Antime, vnum quidpiam, quod jam in mentem venit, breviter expo­
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              nere; ſcilicet in Copernicana hypotheſi, cuncta fetè gratis, vt aiunt,
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              & ad nutum conſtruentis adſtrui, id eſt ſine vlla cauſa, vel ratione, quæ
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              hoc, vel illud fieri poſtulet; v.g. terram moveri volunt in excentrico; cur </s>
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