Clavius, Christoph
,
In Sphaeram Ioannis de Sacro Bosco commentarius
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[Figure 101]
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[Figure 102]
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[Figure 104]
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Ioan. de Sacro Boſco.
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in Sole reperiri deberet quod falſum eſt. </
s
>
<
s
xml:id
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xml:space
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">Mouetur enim ſemper eadẽ tardita-
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te, dũ eſt in Auge, dũ uero in Augis oppoſito eſt, eadem celeritate.) </
s
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<
s
xml:id
="
echoid-s16719
"
xml:space
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preserve
">ita facilli-
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mo negotio eã tuobimur, ſi in Epicyclo Lunã moueri ponamus, & </
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>
<
s
xml:id
="
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xml:space
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">in E@centri
<
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co, ut ex ſuperiori ſigura cõſtat. </
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<
s
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echoid-s16721
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xml:space
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">Si. </
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<
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xml:space
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<
s
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echoid-s16723
"
xml:space
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">Eccentricus Lunæ ſecundũ ſignorũ ſuc-
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ceſſ@on@ moueatur, (vt re uera mouetur) hoc eſt, ab ♈, in ♉, & </
s
>
<
s
xml:id
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echoid-s16724
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xml:space
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">à ♉, in ♊, &</
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>
<
s
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echoid-s16725
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xml:space
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">c.
<
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</
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<
s
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echoid-s16726
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xml:space
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">nempe in dicta figura ex C, in B, & </
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<
s
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echoid-s16727
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xml:space
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">ex B, in E, &</
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>
<
s
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xml:space
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<
s
xml:id
="
echoid-s16729
"
xml:space
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">Epicyclus autem eiuſdem fe
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ratur in ſuperiori quidẽ parte (ut in eius Theorica oſteneitur) contra ſucceſ
<
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ſionem ſignorum, motu videlicet motui Eccentrici cõtrario, puta, ex G, in H,
<
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ſumendo Epicyclũ ſuperiorem in ſigura, uel ex H, in G, ſumẽdo inferiorẽ, In
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parte autem inferiori Epicycli ſecundum ſignorũ ſucceſſionẽ, quemadmodũ
<
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& </
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<
s
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xml:space
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">Eccentricus, nempe in Epicyclo ſuperiori nominatæ figuræ ex H, in I, at in
<
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inferiori ex I, in H; </
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>
<
s
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"
xml:space
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">perſpicue intelligitur, Lunam, dũ reuoluitur in ſuperiori
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parte Epicyclir ferri tardius, cũ contramotũ Eccentrici vehatur: </
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>
<
s
xml:id
="
echoid-s16732
"
xml:space
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">in parte vero
<
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inferiori incitatius, cum geminetur quodãmodo eius motus uerſus eandẽ pa@
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tem. </
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>
<
s
xml:id
="
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"
xml:space
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">Accedit etiã, quòd Luna in ſuo Eccentrico regulariter mouetur circa cẽ
<
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trum terrę, (vt in eius Theorica cũ Ptolomęo demonſtrabimus) vnde ſine Epi
<
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cyclo rationẽ huiuſce tarditatis, velocitatisq́; </
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>
<
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xml:space
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">reddere non poſſumus. </
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<
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xml:space
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">Hæc va-
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rietas in alijs etiam planetis, præter Solẽ, notata eſt ſuo modo. </
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<
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xml:space
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">Vnde & </
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<
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">ipſi in
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Epicyclis reuoluentur. </
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>
<
s
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xml:space
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">Cęterũ multo euidentius in ſuperioribus tribus pla-
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netis, Marte, Ioue, & </
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>
<
s
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="
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xml:space
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">Saturno, nec nõ in Mercurio, ac Venere, Epicyclus inuẽ-
<
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tus eſt. </
s
>
<
s
xml:id
="
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xml:space
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">Hi enim planetæ nunc progredi in Zodiaco à
<
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/>
partibus occidentalibus
<
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verſus orientales cernuntur, nunc uero retrocedere a partibus orientalibus
<
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uerſus occidentales. </
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>
<
s
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="
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xml:space
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">Dũ em̃ ſunt in ſuperiori parte Epicycli, voluuntur ſecun
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dũ ſucceſſionẽ ſignorũ, quemadmodũ & </
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>
<
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">in Eccentrico: </
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<
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xml:space
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">Vnde incitatur eorũ
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motus ab occaſu in ortũ, & </
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<
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">ſic progredi uidẽtur; </
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<
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">ita ut ſi v. </
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<
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">g. </
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<
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xml:space
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">aliquis illorũ eſt
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in gr. </
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<
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">1. </
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<
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xml:space
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">&</
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<
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">c. </
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<
s
xml:id
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echoid-s16754
"
xml:space
="
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">Dum uero in parte Epicy-
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cli inferiori uerſantur, cientur cõtra ſignorũ ſucceſſionẽ, hoc eſt, cõtra motũ
<
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quẽ Epicyclus habet in Eccentrico: </
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>
<
s
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="
echoid-s16755
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xml:space
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">atque ita retrogredi uidentur, ita ut, ſi v. </
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<
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xml:space
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">g. </
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<
s
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illorum quiſpiã in grad. </
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<
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xml:space
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">4. </
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<
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">♌, uerſatur, mox futurus ſit in grad. </
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<
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">3. </
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<
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&</
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<
s
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<
s
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="
echoid-s16764
"
xml:space
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">quę omnia clarius explicabũtur in Theoricis Cur uero retrogradatio hęc
<
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in Luna non appareat, cum tamen in
<
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Epicyclo in diuerſas cieatur partes,
<
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& </
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>
<
s
xml:id
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xml:space
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">diſſimiles, in eius Eheorica oſtendemus. </
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<
s
xml:id
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xml:space
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">Itaq; </
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>
<
s
xml:id
="
echoid-s16767
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xml:space
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">cũ hæc apparentia nullo mo-
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do ſine Epicyclo, facillime autem, illo poſito, defendi poſſit, ut ex dictis con-
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ſtat, veriſimile erit, quemlibet planetam, Sole excepto, in Epicyclo moueri.</
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<
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<
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Apparentia
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probans da-
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ri Epicyclos@</
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<
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<
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>
ac dilihentes aſtrorum obſeruatores conſiderarunt
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aliquando duas eclipſes Lunares, Sole & </
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>
<
s
xml:id
="
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xml:space
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">Luna in eodem ſitu in utraque ma-
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nentibus, puta Sole in capite Draconis, & </
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<
s
xml:id
="
echoid-s16772
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xml:space
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">Luna in cauda, exiſtenteq́; </
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>
<
s
xml:id
="
echoid-s16773
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xml:space
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">Sole in
<
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vtraque in eodem loco Eccentrici, ita ut in utraq; </
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>
<
s
xml:id
="
echoid-s16774
"
xml:space
="
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">eandem à terra diſtantiam
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habuerit, atque adeo eandem utrobique umbram terra proiecerit; </
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>
<
s
xml:id
="
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xml:space
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">inuene-
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runtq; </
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<
s
xml:id
="
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xml:space
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">alteram eclipſiũ longiori tempore duraſſe, quàm alteram. </
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>
<
s
xml:id
="
echoid-s16777
"
xml:space
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">Cuius qui-
<
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dem inæqualitatis cauſa Eccentrico ſoli tribui non poteſt. </
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<
s
xml:id
="
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xml:space
="
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">Maior enim, uel
<
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minor duratio eclipſis accidit ob ingreſſum Lunæ in maiorem, uel minorem
<
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umbram terræ: </
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>
<
s
xml:id
="
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xml:space
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">At tunc in vtraque eclipſi eadem ſemper fuit umbra terræ, cũ
<
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Sol ponatu@ æqualiter a terra in utraque remotus. </
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>
<
s
xml:id
="
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"
xml:space
="
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">Oportet igitur Lunam
<
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ipſam in altera eclipſium minus remotam fuiſſe à terra, in alt@@@ uero ma-
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gis. </
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>
<
s
xml:id
="
echoid-s16781
"
xml:space
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">Nam cum terræ umbra porrigatur in conum, quod terra minor ſit,
<
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quàm Sol, fit, ut quo propinquior terræ fuerit vmbra, eo latior ſit, quo ne-
<
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/>
ro remotior à terra, eo anguſtior, & </
s
>
<
s
xml:id
="
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">minus lata. </
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>
<
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="
echoid-s16783
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">Ex quo fit, Lunam, </
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