Clavius, Christoph
,
Gnomonices libri octo, in quibus non solum horologiorum solariu[m], sed aliarum quo[quam] rerum, quae ex gnomonis umbra cognosci possunt, descriptiones geometricè demonstrantur
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uenirentur, vt perſpicuum eſt, ſi res paulo diligentius conſideretur.</
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<
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nationum om-
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nium punctor
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ũ
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Eclip@icæ in A-
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nalẽmate, una
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c
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um demonſtra
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tione.</
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<
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<
s
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">CVM hæc demonſtrarem, venit mihi in mentem, eadem fere ratione demonſtrari poſſe con
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ſtructionem Analemmatis lib. </
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<
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<
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<
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<
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<
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enim Meridianus Analemmatis A B C D, circa centrum E, in quo diameter Horizontis B D; </
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<
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ticalis A C; </
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<
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<
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<
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xml:space
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">diametri parallelorum ſemper apparentium, ſem-
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perq́ue latentium maximorum D k, B L. </
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<
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xml:space
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</
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<
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xml:space
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">ad angulos rectos ſecabitur,
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<
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fig-0668-01
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0668-01
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xlink:href
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http://echo.mpiwg-berlin.mpg.de/zogilib?fn=/permanent/library/xxxxxxxx/figures/0668-01
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</
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vt propoſ. </
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<
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<
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<
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<
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xml:space
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<
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que ex O, circa M N, circulo M P N Q, eoq́;
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</
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<
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<
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xml:space
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">partes æquales, ducãtur per quæ-
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libet bina puncta à P Q, æqualiter diſtantia li-
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neę rectæ Y S λ, X R μ, Z T ξ, α V π, quæ ex
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ſcholio propoſ. </
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<
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<
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<
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<
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<
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rectæ Q P I. </
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<
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huiuſmodi parallelæ, ſi à puncto I, ſupputetur
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quoque vtrinque maxima Solis declinatio vſ-
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quead θ, & </
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<
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">ρ, iunctaq́ue recta θ ρ, ſemicircu-
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lus ex puncto 8, deſcribatur, qui in ſex æquales
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partes ſecetur, &</
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<
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mus. </
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<
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xml:space
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<
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ex eodem ſcholio ipſi H I, æquidiſtabunt. </
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<
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haſce rectas diametros eſſe parallelorum, nem-
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pe communes eorum cum Meridiano ſectio-
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nes, ita vt arcus H γ, H ß, H δ, H ε, metiantur
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declinationes aliorum parallelorum, qui per ſi-
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gnorum initia ducũtur, quemadmodum H M,
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H N, maximas declinationes Solis metiuntur:
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</
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<
s
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">hoc ordine, vt arcus H γ, H ß, metiantur declinationes illorum punctorũ Eclipticę, quæ à prin-
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cipio ♋, verſus ♈, vel ♎, tot gradibus abſunt, quot gradibus puncta X, Y, R, S, à puncto M, di-
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ſtant; </
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<
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, illorum punctorum Eclipticæ declinationes metiantur, quæ tantum
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<
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à principio ♑, verſus ♈, vel ♎, diſtant, quanto ſpatio puncta Z, α, T, V, in ſuo circulo à puncto
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N, abſunt. </
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<
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<
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">Ducta recta M ρ, quæ diameter erit Eclipticæ, poſito princi
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pio ♋, in M, & </
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<
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<
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<
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pendicularis ducatur p b, intelligaturq́; </
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<
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nec rectus ſit ad Meridianum A B C D. </
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<
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dianum, ex propoſ. </
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<
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<
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<
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<
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<
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<
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que per b, punctum Eclipticæ duci circulus Aequatori æquidiſtans, & </
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<
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quoniam tam Ecliptica, quàm hic parallelus rectus eſt ad Meridianum, erit quoque communis
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eorum ſectio per punctum b, tranſiens ad Meridianum recta: </
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<
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<
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pendicularis, ex defin. </
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<
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<
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<
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<
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b, ducti; </
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<
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<
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tore, & </
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<
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<
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la diametro Aequatoris H I, communis ſectio dicti paralleli, & </
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ſius paralleli. </
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<
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<
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autem arcus Eclipticę M b, ſimilis arcui M X, in circulo M P N Q, ex lemmate propoſ. </
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<
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<
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<
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</
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<
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vt M p, ſinus verſus arcus M b, ad M φ, ſinum verſum arcus M X. </
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<
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xml:space
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metro Aequatoris parallela per punctum X, dat in Meridiano arcũ H γ, declinationis puncti Ecli
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pticę b, quod totidẽ gradibus à puncto M, diſtat, quot gradibus punctũ X, ab eodẽ puncto M, di-
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ſtat in circulo M P N Q. </
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<
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<
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<
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<
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xml:space
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<
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tione liquido cõſtat, ſi circulus A B C D, ſecetur in 12. </
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<
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partibus circuli M P N Q, initio facto à puncto M, & </
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<
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">quælibet bina puncta æqualiter remota ab
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M, rectis lineis iungantur a 7, b 6, d 5, e 4, 23, quæ perpendiculares ſunt ad M ρ, in punctis l,
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p, E, q, u, (quod demonſtrabitur, vt propoſ. </
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<
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<
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<
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">1. </
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<
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xml:space
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">oſtenſum eſt, rectam
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M N, ſectam eſſe ad rectos
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angulos) rectas per hæc puncta ductas rectæ H I, parallelas, quales ſunt ß λ, γ μ, δ ξ, ε π, auferre
<
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<
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quoque ex Meridiano arcus declinationum. </
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<
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<
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<
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<
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<
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<
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</
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<
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demonſtrauimus de puncto b, quod tot gradibus abeſt ab M, in circulo A B C D, quot
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gradibus punctum X, diſtat in circulo M P N Q, ab M, eademq́ue ratio eſt de cęteris.</
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<
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">ANTEQVAM huic operi extremam manum apponerem, ſedulo in eam curam incumbe-
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bam, vt praxim illam ſcholij propoſ. </
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<
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<
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<
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<
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">qua Andreas Schonerus breuiſſime ac facilime
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radios arcuum diurnorum inquirit, ratione aliqua Geometrica corroborarem: </
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