Clavius, Christoph
,
Geometria practica
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LIBER OCTAVVS.
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quadratum æquale eſt rectangulo ſub AD, AB, quo diuiſo per AB, altitudinem
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montis, prodibit in Quotiente recta A D; </
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<
s
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A B, nota relinquetur diameter terræ BD. </
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<
s
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xml:space
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"> Ac proinde circumferentia B C
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xml:space
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Dimens. cir-
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culi lib. 4. hu-
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i{us}.</
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cognita fiet.</
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<
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quia in hac ratione metiendi ambitus terreſtris aſſumitur, arcum B C,
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à linea recta non diſferre. </
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<
s
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xml:space
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">quod verum non eſt, quando mons tam altus eſt, vt
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ſpacium 200. </
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<
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">vel 300. </
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<
s
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xml:space
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">milliariorum cerni poſsit, quod tunc arcus BC, iuxta am-
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bitum à Ptolomæo poſitum contineat grad. </
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<
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proinde non rectè linea tangens A C, ex lateribus A B, BC, colligitur. </
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<
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quod per ptoblemata lib. </
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">3. </
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<
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">citata inuenitur perpendicularis BE, in plano,
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ad quod mons eſt ad angulos rectos: </
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">Redigemus rationem hanc ad meliorem
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formam multis viis hoc modo. </
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<
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">Deprehenſo angulo A, per Quadrantem, vel
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Quadratum, quando radius viſualis per dioptram circulum terræ tangit. </
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<
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tum denique certiſsimè fiet, cum per dioptram conſpicitur Sol, aut alia ſtella,
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quando oritur, vel occidit. </
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<
s
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xml:space
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">Deprehenſo, inquam, angulo A, inuenienda erit
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perpendicularis BE, per problemata paulò ante citata. </
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<
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xml:space
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">47. primi.</
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A B, B E. </
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">Si enim ad A E, adiicietur BE, hoc eſt, EC, quæ ipſi BE, æqualis
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">2. coroll. 36.
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tertii.</
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nota fiet tota tangens AC, ex qua, vt ſupra dictum eſt, & </
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<
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">diameter terræ BD, & </
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circumferentia inueſtigabitur. </
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<
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">Quin etiam cognito angulo A, ac proinde & </
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<
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">eius
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complemento E, reperietur tam latus B E, quam baſis A E,
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rectil.</
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bus ex lib. </
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<
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ſic agemus. </
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<
s
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">Cognito per dioptram angulo A, cognitus etiam erit (du-
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<
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">5. triang. re-
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ctil.</
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cta recta F C, quæ ad A C, perpendicularis erit) angulus F, eius complemen- tum in centro. </
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<
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">Quia verò ducta recta FE, duo latera EC, CF, duobus lateribus
<
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<
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">18. tertii.</
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E B, BF, æqualia ſunt, comprehenduntque angulos æquales, nemperectos:
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</
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<
s
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"> erunt anguli ad F, æquales. </
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<
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xml:space
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">Cum ergo totus angulus B F C, cognitus ſit,
<
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proximè diximus; </
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<
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">cognitus etiam erit BFE, tanquam ſemiſsis ipſius: </
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<
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de & </
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<
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">eius complementum B E F, notum erit. </
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<
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xml:space
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">Igitur in triangulo ABE, ex an-
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gulis A, E, & </
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<
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">latere AE, reperietur BE, in partibus altitudinis montis A B,
<
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rectil.</
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tæ. </
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<
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xml:space
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">Atque eodem modo in triangulo B E F, ex angulis E, F, & </
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<
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noſcetur ſemidiameter B F, in partibus lateris BE, hoc eſt, in partibus altitudinis
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montis A B; </
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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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hoc etiam modo idem aſſequemur. </
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<
s
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xml:space
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">Cognito per dioptram an-
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gulo A, quando radius viſualis terram contingit, cognitus etiam erit angulus
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A F C, eius complementum. </
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<
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xml:space
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">Ergo huius anguli ſecans AF, cognita erit in parti-
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busſinus totius FC. </
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<
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xml:space
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">Ex qua ſecante, ſi dematur ſinus BF, nota relinquetur alti-
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tudo montis AB, in partibus ſinus totius BF. </
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>
<
s
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xml:space
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">Si igitur fiat, vt altitudo montis
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AB, nota in partibus ſinus totius ad eandem A B, notam in data menſura, ita ſi-
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nus totus BF, ad aliud; </
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<
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">proueniet ſemidiameter BF, nota in partibus altitudinis
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montis, &</
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<
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<
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<
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æqualem: </
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<
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xml:space
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">Ac viciſsim Cylindro Priſma æquale, & </
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<
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Pyramidem conſtituere.</
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