Apian, Petrus
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Instrvmentvm Sinvvm, sev primi mobilis
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<
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TABVLARVM SINVVM.
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arcus eſt ipſe arcus horizontis inter punctũ Solis aſcendentis & </
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>
<
s
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</
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<
s
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xml:space
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<
s
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xml:space
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">? Exemplum ſit hoc tibi, in die intronizationis eſto, ut obſeruarit quis altitudinem So-
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<
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PLVM
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E
<
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style
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pi.</
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</
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lis in circulo uerticali, ea fuit 28. </
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<
s
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<
s
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<
s
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<
s
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<
s
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xml:space
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">duxerit in ſinum totum,
<
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productum diuiſerit in ſinum complementi altitudinis poli 66913. </
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<
s
xml:id
="
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xml:space
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">in quotiente proue-
<
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nerũt 71083. </
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<
s
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"
xml:space
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">ex eo quadrato, hoc eſt in ſe ducto, ꝓdijt numer
<
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">9</
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>
ille q̃dratus 5052792889
<
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deinde ſimili modo quadrato etiam ſinum altitudinis uerticalis, prouenit 2262334096.
<
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</
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>
<
s
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xml:space
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">eo ſubtracto à ſuperiori, remanſit 2790458793. </
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>
<
s
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xml:space
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">radix illius numeri quadrata eſt 52825. </
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<
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<
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arcus eius 31. </
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<
s
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<
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<
s
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<
s
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xml:space
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">amplitudo illa Solis ad diem intronizationis, quam pronuncia-
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to 12. </
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<
s
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</
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<
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xml:space
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<
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<
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">Ex altitudine Solis in circulo uerticali, & </
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<
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">ex amplitudine Solis eiuſdem di
<
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ei altitudinem poli expedite inueſtigare, etiam ſi neſcias gradum Solis ſimul
<
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& </
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>
<
s
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">declinationem illius.</
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<
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</
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<
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<
s
xml:id
="
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xml:space
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">Per hoc q̊d iam docebimus. </
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>
<
s
xml:id
="
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xml:space
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">poteſt ꝗs quotidie tota æſtate mane altitudinem poli ob-
<
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ſeruare, nõ cognito gradu & </
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>
<
s
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="
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xml:space
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">declinatione Solis, ſi modo ꝑ inſtrumentũ aliq̊d amplitudi
<
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nem Solis ortiuã & </
s
>
<
s
xml:id
="
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xml:space
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">occiduã obſeruarit (quicꝗd em̃ hic de amplitudine ortiua dicimus ſi-
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mul & </
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>
<
s
xml:id
="
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xml:space
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">de altitudine uerticali, idẽ etiã de amplitudine occidua & </
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>
<
s
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="
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xml:space
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">altitudine Solis in circu
<
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lo uerticali occiduo intelligi debet) parit’ & </
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>
<
s
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="
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xml:space
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">altitudinẽ Solis in circulo uerticali exiſten-
<
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tis, ſtatim duc ſinũ amplitudinis in ſe ꝗ̃drate, deinde etiã ſinũ altitudinis uerticalis, utrũ
<
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hũc nume℞ quadratũ in unã ſummã cõponito, ex ea rurſus quære radicem quadratã, & </
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<
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<
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</
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lam propone in regulã philoſopho℞ primo loco, ſecũdo ſinũ altitudinis Solis in circulo
<
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uerticali, tertio ſinũ totũ. </
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<
s
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">Et iuxta regulã numerũ ultimũ duc in mediũ, ꝓductũ in primũ
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diuide, & </
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>
<
s
xml:id
="
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">arcus q̊tientis ex quadra circuli ſubtractus, oſtendet tibi altitudinem poli quæ-
<
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<
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<
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PLVM
<
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E
<
emph
style
="
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<
unsure
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pi.</
emph
>
</
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>
ſitam. </
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<
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<
s
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">?Sed obſcurius paulò hoc tibiuidetur, en exemplo ſit dilucidius. </
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>
<
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">Altitudo So
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lis in circulo uerticali in die intronizationis fuit 28. </
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<
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<
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<
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<
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<
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">amplitu
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do q̊ ortiua ꝑ in ſtrumentũ inuenta eſt 31. </
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<
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<
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<
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<
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<
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">quadratũ illi-
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us 2790458793. </
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<
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">quadratũ aũt ſinus altitudinis 2262334096. </
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<
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">utrun quadratũ hoc con
<
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iunctũ in una ſumma, facit 5052792889. </
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<
s
xml:id
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xml:space
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">radix eius quadrata eſt 71083. </
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<
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xml:space
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">Si ergo in regu-
<
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lam proportionũ cõpoſuero hoc modo 71083. </
s
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<
s
xml:id
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xml:space
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">dant mihi 47564. </
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<
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">Quid ita ex toto pro
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ueniet ſinu@ Inueniam uti ex operatione regulæ huius 66913. </
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<
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">Arcus eius 42. </
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<
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">ex circuli
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quadra ſubtra ctus, reliquã faciet altitudinem poli 48. </
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<
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">gra. </
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<
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">quæſitã ad locũ obſeruationis.</
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<
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</
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</
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<
div
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<
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xml:space
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">PRONVNCIATVM XXV.</
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<
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<
s
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">Quocun tempore, ſiue qualibet hora, gradum eclypticæ, quimeridia,
<
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num tangit, ex ſphærica ſupputatione colligere.</
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<
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</
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<
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<
s
xml:id
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">Si quando mediũ cœli in eclyptica noſſe cupis, uel ante uel poſt meridiem: </
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<
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diſtantiã Solis à meridie, & </
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<
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">reſolue eã in gradus, deinde adſume etiã aſcenſionem rectam
<
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gradus Solis ꝑ pronunciatũ 7. </
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>
<
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xml:id
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xml:space
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">Quòd ſi tempus operationis huius fuerit antemeridianũ,
<
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tũc ſubtrahe gradus diſtãtiæ à meridiano: </
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>
<
s
xml:id
="
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xml:space
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">ſin aũt pomeridianũ fuerit, addenda tibi erit di
<
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ſtantia horaria in gradus cõuerſa ad aſcenſionem rectã gradus Solis. </
s
>
<
s
xml:id
="
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xml:space
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">Ex additiõe uel ſub
<
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tractione huiuſmodi quicquid prouenerituel reliquũ manſerit, aſcenſio recta dicet̃ me-
<
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dij cœli. </
s
>
<
s
xml:id
="
echoid-s2184
"
xml:space
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">Hinc ſi adhuc ſcire deſideras gradũ eclypticæ eo ipſo momento tangentem me-
<
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ridianũ, is ſanè eſt, qui cum eo in ſphæra recta aſcendit, quære eũ ex pronunciato 8.
<
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</
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<
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xml:space
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">& </
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>
<
s
xml:id
="
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xml:space
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">habebis punctum eclypticæ, qui mediat cœlum tempore propoſito. </
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<
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">?</
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>
<
s
xml:id
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xml:space
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">?Et ſit eius rei
<
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<
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="
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xml:space
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">EXEM-
<
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PLVM
<
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E
<
emph
style
="
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">piſoo
<
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/>
pi.</
emph
>
</
note
>
exemplum tale. </
s
>
<
s
xml:id
="
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"
xml:space
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">Scire for ſitan cupio ad ipſam horã intronizationis, quid tunc mediũ cœ
<
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li habuerit, quando intronizatio facta eſt hora 9. </
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>
<
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="
echoid-s2190
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xml:space
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">ante meridiem: </
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<
s
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="
echoid-s2191
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xml:space
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">diſtantia uti horaria
<
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eſt 3. </
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<
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">graduũ, quoniã à 9. </
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>
<
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">uſad 12. </
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>
<
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">horæ tres ſunt: </
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<
s
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xml:space
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">in reſolutione ergo ſemper 15. </
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>
<
s
xml:id
="
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xml:space
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">gradus
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pro hora cõnumerando, faciũt horæ tres gradus 45. </
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>
<
s
xml:id
="
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xml:space
="
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">eos ſubtraho ab aſcenſione gradus
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Solis, quem ſupra in pronũciato 7. </
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>
<
s
xml:id
="
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xml:space
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">inueni: </
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>
<
s
xml:id
="
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xml:space
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">ſiquidem tũc Sol ſuit in 2. </
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>
<
s
xml:id
="
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xml:space
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">gra. </
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>
<
s
xml:id
="
echoid-s2201
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xml:space
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">26. </
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>
<
s
xml:id
="
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">mi. </
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>
<
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="
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">II. </
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>
<
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="
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">aſcen
<
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ſio eius eſt 60. </
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>
<
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xml:id
="
echoid-s2205
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xml:space
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">gra. </
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>
<
s
xml:id
="
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"
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">21. </
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>
<
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="
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">mi. </
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<
s
xml:id
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">unde ſubtraho 45. </
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<
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">gra. </
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>
<
s
xml:id
="
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xml:space
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">& </
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>
<
s
xml:id
="
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">remanent 6. </
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<
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">gra. </
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<
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">21. </
s
>
<
s
xml:id
="
echoid-s2214
"
xml:space
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preserve
">mi. </
s
>
<
s
xml:id
="
echoid-s2215
"
xml:space
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">æquatoris,
<
lb
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quæ tangunt medium cœli ipſa hora intronizationis. </
s
>
<
s
xml:id
="
echoid-s2216
"
xml:space
="
preserve
">Si igitur iuxta pronuhciatum 8.</
s
>
<
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xml:id
="
echoid-s2217
"
xml:space
="
preserve
"/>
</
p
>
</
div
>
</
text
>
</
echo
>