Clavius, Christoph
,
In Sphaeram Ioannis de Sacro Bosco commentarius
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Ioan. de Sacro Boſco.
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qui tranſit per punctum Verticale Romæ, cuius declinatio ponatur grad. </
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<
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videlicet 74314. </
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ſinum totum, & </
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<
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">inuenio gradus 267 {1/2}. </
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">fere. </
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<
s
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xml:space
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">Habebit igitur Aequator ad pa-
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rallelum, qui per uerticem Romæ incedit, uel etiam unus gradus Aequatoris
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ad unũ gradum dicti paralleli, proportionem, quam 360. </
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fere, hoc eſt, fere ſeſquitertiam, qualis eſt 4. </
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">&</
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<
s
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">QVANTA eſt etiam maxima Solis declinatio, ſe
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ilicet ab Aequi
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">Diſtanti@
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poli zodia-
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ci à polo
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mũ di æqua
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lis eſt maxi
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mæ Solis
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declinati@-
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ni.</
note
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noctiali, tanta eſt diſtantia poli mundi à polo Zodiaci, quod ſic patet. </
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matur Colurus diſtinguens Solſtitia, quitranſit per polos mundi, & </
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polos Zodiaci Cum igitur omnes quartæ unius, & </
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<
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">eiuſdem circuli inter
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ſe ſint æquales, quarta huius Coluri, quę eſt ab Aequinoctiali uſque ad
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polum mundi, erit æqualis quartæ eiuſdem Coluri, quæ eſt à primo puncto
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Cancri uſque ad polum Zodiaci. </
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xml:space
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">Igitur ab illis ęqualibus dempto commu-
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ni arcu, qui eſt à primo puncto Cancri uſque ad polum mundi, reſidua
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erunt æqualia, ſcilicet maxima Solis declinatio, & </
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<
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">diſtantia poli mundi
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à polo Zodiaci.</
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<
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, tanto ſpatio polos Zo-
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341-01
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xlink:href
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http://echo.mpiwg-berlin.mpg.de/zogilib?fn=/permanent/library/xxxxxxxx/figures/341-01
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figure
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diaci à polis mundi recedere, quanta eſt
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utrauis maxima declinatio Solis: </
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quidem demonſtrat eodem modo, quo nos
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idem oſtendimus in 6. </
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<
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xml:space
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">officio Colurorum,
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ut perſpicuũ eſt in hac figura, in qua cir-
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culus A B C D, eſt Colurus Solſtitiorum;
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</
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<
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">A B, quarta ab Aequinoctiali A C, vſque
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intelligen-
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dũ ſit, diſtã
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tiam polo-
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rũ zodiaci
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à polis mũ
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d@ ęqualem
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eſſe maxi-
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mæ declina
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tioni Solis.</
note
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ad mundi polum B; </
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<
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puncto ♋, vſque ad polum Zodiaci K;
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</
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<
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ſtantia poli mundi a polo Zodiaci, &</
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<
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<
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vero ſupra diximus, maxi-
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mam Solis declinationem uariari propter
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motum trepidationis octauæ ſphæræ, efficitur, vt hæc ratio tantum conclu-
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dat, maximam declinationem Eclipticæ nonæ ſphæræ æqualem eſſe diſtantiæ
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polorum Eclipticæ eiuſdem ſphæræ a polis mundi, quoniam hæc ſphæra mo-
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tu trepidationis non citetur. </
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<
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xml:space
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">Non enim declinatio maxima Solis, cum va-
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rietur, æqualis eſſe poterit diſtantiæ poli Zodiaci a polo mundi, quæ in nona
<
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<
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xlink:label
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arcus Colu
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ri inter tro
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picum Ca@
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cri, & circu
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lum arcti-
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cum.</
note
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ſphæra ſumitur, permanetq́ue ſemper eadem.</
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<
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æque diſtet à polo mũdi, patet, quòd illa pars Coluri, quę eſt inter primum
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punctum Cancri, & </
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