Fabri, Honoré, Tractatus physicus de motu locali, 1646

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              candum eſt per contactus inadæquatos; tunc enim motus centri longè
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              ſuperat motum orbis. </s>
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            <p id="N25E3C" type="main">
              <s id="N25E3E">Quintò, ſi vera eſſet hypotheſis Copernici, terra moueretur hoc vlti­
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              mo motu mixto ex motu centri, & motu orbis; </s>
              <s id="N25E44">vnde omnia puncta
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              eiuſdem circuli paralleli mouerentur inæquali motui tardiſſimo qui­
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              dem punctum contactus hoc eſt meridiano reſpondens, velociſſimo ve­
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              rò ipſi oppoſitum, ſcilicet de media nocte: porrò in hoc motu motus
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              centri eſſet ferè maior motu orbis iuxta communem de diametro ma­
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              gni orbis ſententiam. </s>
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            <p id="N25E52" type="main">
              <s id="N25E54">Sextò, ſi motus maioris rotæ dirigatur à minore res eodem modo
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              explicanda eſt, quo explicuimus illam per
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              diuerſos inadæquatos
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              tùm Th. 15. num. </s>
              <s id="N25E5F">11. tùm in digreſſione multis locis: </s>
              <s id="N25E63">porrò poſſunt eſſe
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              diuerſæ proportiones circuli mobilis, & immobilis; qui ſi maximus eſt,
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              minimus illius arcus accipi poteſt pro linea recta. </s>
            </p>
            <p id="N25E6B" type="main">
              <s id="N25E6D">Septimò, poteſt ita rota moueri, vt pars ſuperior retrò agatur, id eſt,
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              vt motus orbis ſit oppoſitus motui
                <expan abbr="cétri">centri</expan>
              v.g.ſi punctum N moueatur qui­
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              dem dextrorſum motu centri, O verò ſiniſtrorſum motu orbis; </s>
              <s id="N25E75">ſed tunc
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              punctum B mouebitur dextrorſum motu orbis, ſed eſt noua difficultas: </s>
              <s id="N25E7B">
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              quippe ex hac hypotheſi punctum O deſcriberet ſuo motu lineam ſimi­
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              lem, & æqualem lineæ rotatili BMIHF; punctum verò B moueretur
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              iuxta hanc hypotheſin eo modo, quo mouetur punctum O iuxta prio­
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              rem. </s>
              <s id="N25E86">Sic autem moueri dicuntur quidam Epicycli ab Aſtronomis, quo­
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              rum centrum mouetur in conſequentia, hoc eſt ſecundum ſeriem
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              ſignorum; </s>
              <s id="N25E8E">ſummum verò punctum, ſeu ſtella apogæa retrò agitur, ſeu
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              in partem aduerſam contendit, vel vt vocant, in præcedentia: </s>
              <s id="N25E94">tales
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              vulgò ponuntur Solis Epicycli & Lunæ; vnde obiter colligo, quàm ſit
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              neceſſaria Aſtronomis hæc de motu mixto ſententia, vt ſua phœnome­
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              na ad ſuas cauſas phyſicas reducant. </s>
            </p>
            <p id="N25E9E" type="main">
              <s id="N25EA0">Octauò denique, poſſunt eſſe diuerſæ lineæ huius motus pro diuerſa
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              circulorum proportione, quarum figuras, deſcriptiones, affectiones ſuo
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              loco demonſtrabimus, & nouos latices tum Geometris, tùm Phyſicis
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              aperiemus, ex quibus vbertim fluit infinitarum ferè demonſtrationum
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              materia. </s>
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            <p id="N25EAD" type="main">
              <s id="N25EAF">
                <emph type="center"/>
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              Theorema
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              17.
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              </s>
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            <p id="N25EBB" type="main">
              <s id="N25EBD">
                <emph type="italics"/>
              Explicari poſſunt cuncta phœnomena rotæ maioris mobilis circa minorem̨
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              immobilem
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              ; ſit enim rota minor centro A, cui incubet maior rota cen­
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              tro K, radio KB duplo BA, roteturque circa ſuperficiem BDFTH
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              punctum 5 reſpondebit F & Q poſt decurſam ſuperficiem puncto B,
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              eritque motus mixtus. </s>
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            <p id="N25ECE" type="main">
              <s id="N25ED0">Primò, centrum K mouebitur motu circulari, quia ſemper æqualiter
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              diſtat à puncto A; igitur deſcribit circulum, cuius radius eſt KA. </s>
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              <s id="N25ED8">Secundò, poteſt facilè deſcribi linea motus puncti B v.g. diuidatur
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              enim BDFH in 8 arcus æquales, & B5 in 4; tùm per puncta </s>
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