Apian, Petrus
,
Instrvmentvm Sinvvm, sev primi mobilis
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TABVLARVM SINVVM PER PET. APIANVM.
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ordinem ſignorum, eius diſtantiæ ſinum duc in ſinum maximæ declinationis Solis, & </
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<
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<
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uide in totum, arcus quotientis huius ex 90. </
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<
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</
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<
s
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<
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mæ declinationis Solis, minorem duc in totum, productum diuide in maiorem, ſinus quo
<
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tientis ex 90. </
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<
s
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">ſubtractus, reliquum tibi faciet inuentum ſecundum: </
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<
s
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xml:space
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<
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<
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<
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habebit à medietate eclypticæ in qua ſtella iſta eſt, proinde ſi fuerit in medietate ſepten-
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trionali, dicetur inuentum ſecundum ſeptentrionale. </
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<
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xml:space
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">Et hoc ipſum deinde adde ad lati
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tudinem ſtellæ, ſi tamen ea fuerit in medietate zodiaci ſeptentrionali, & </
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<
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<
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<
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</
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ter ſeptentrionalis. </
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<
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ſcilicet medietas zodiaci & </
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<
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<
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</
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ſubtractione remanet, dicetur argumentum declinationis. </
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<
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nomen argumenti retinebit: </
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<
s
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xml:space
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">ſin autem ex ſubtractione ſupereſt, habebit nomen nume-
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ri maioris. </
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<
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<
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<
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nationis, & </
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<
s
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">diuides productum in totum, arcus quotiẽtis erit declinatio ſtellæ, & </
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<
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nomen argumenti, ſiue ſeptentrionalis ſiue meridionalis. </
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<
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">Porrò ſi nihil in argumento
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fuerit, etiam tunc declinatio erit nulla, nec eſt quod ultra labores, ſed ſi punctum ſiue
<
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ſtella ſit in eclyptica, declinationem retinet eclypticæ, ſicut per 5. </
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<
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nies. </
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<
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PLVM
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E
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Agitatoris, quæ ſecundum Alfonſi regis obſeruationem habet in longitudine 19. </
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<
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<
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<
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libentius, quia ipſa hora intronizationis cum Sole penè in uno fuit circulo poſitionis,
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ex ſecundo pronunciato iam inueni uerificationem ſtellæ 2. </
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<
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<
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<
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<
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rum auges planetarum & </
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<
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ſunt promotæ uſ ad horam intronizationis. </
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<
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<
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</
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<
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">II, quo loci fuit illa ſtella fixa ad horam propoſitã, latitudiuem hanc ſicut omnes Aſtro-
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nomifaciunt, ita retineo fixam & </
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<
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<
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cri eſt 7. </
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<
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<
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<
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<
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<
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diuido per totum ſinum, quotiens dabit 5147. </
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<
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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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men habet intrenti primi, ſinum complementi maximæ declinationis Solis 91706. </
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<
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co in totum, & </
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<
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">productum diuido in ſinum complementi primi inuenti ſcilicet 99867. </
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quotiens producit 91828. </
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<
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<
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<
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<
s
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<
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uentum ſecundum, & </
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<
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tum ſecundum ſcilicet 23. </
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<
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<
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<
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<
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<
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onali plaga participant, & </
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<
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<
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<
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<
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<
s
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nis. </
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<
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xml:space
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<
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<
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<
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<
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<
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num argumenti declinationis ſcilicet 68603. </
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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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">diuido in totum, quotiens producet
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68512. </
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<
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">arcus eius 43 gra. </
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<
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<
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<
s
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xml:space
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">eſt ipſa declinatio ſtellæ quæſita & </
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<
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">ſeptentrionalis, quan
<
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doquidem argumentum nomen hoc habet, & </
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<
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</
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<
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>
<
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<
s
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">Declinationem ſtellæ alio & </
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<
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">iucundiore modo perquirere.</
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preserve
"/>
</
p
>
<
p
>
<
s
xml:id
="
echoid-s6561
"
xml:space
="
preserve
">Conſidera primum an ſtella ſit in medietate zodiaci ſeptentrionali uel meridionali,
<
lb
/>
deinde cuinam puncto æquinoctij propius accedat, ut quicquid inter eſt à principio A-
<
lb
/>
rietis uſ ad finem II, id totũ principio Arietis adnumeratur, & </
s
>
<
s
xml:id
="
echoid-s6562
"
xml:space
="
preserve
">quod à principio Can
<
lb
/>
cri eſt uſ ad principium Libræ, ad ♎ computatur. </
s
>
<
s
xml:id
="
echoid-s6563
"
xml:space
="
preserve
">Eam diſtantiam ſubtrahe à 90. </
s
>
<
s
xml:id
="
echoid-s6564
"
xml:space
="
preserve
">& </
s
>
<
s
xml:id
="
echoid-s6565
"
xml:space
="
preserve
">ſi-
<
lb
/>
num complementi uel reſidui duc in ſinum complementi latitudinis ſtellæ, peracta diui
<
lb
/>
<
note
position
="
right
"
xlink:label
="
note-0079-09
"
xlink:href
="
note-0079-09a
"
xml:space
="
preserve
">
<
emph
style
="
it
">Inuentum</
emph
>
<
lb
/>
<
emph
style
="
it
">primum.</
emph
>
</
note
>
ſione ſinus perfecti, erit arcus complementi quotientis inuentum primum. </
s
>
<
s
xml:id
="
echoid-s6566
"
xml:space
="
preserve
">Poſtea duc
<
lb
/>
ſinum latitudinis ſtellæ in totum, & </
s
>
<
s
xml:id
="
echoid-s6567
"
xml:space
="
preserve
">diuide in ſinum primi inuenti, arcus quotientis uo
<
lb
/>
<
note
position
="
right
"
xlink:label
="
note-0079-10
"
xlink:href
="
note-0079-10a
"
xml:space
="
preserve
">
<
emph
style
="
it
">Inuentum</
emph
>
<
lb
/>
<
emph
style
="
it
">ſecundum.</
emph
>
</
note
>
cabitur inuentum ſecundum, hoc iam adde ad maximam Solis declinationem, quum
<
lb
/>
latitudo in nomine conueniat unà cum medietate eclypticæ, ſum@a e@ erit argumen-
<
lb
/>
tum declinationis, retinebit´ nomen medietatis eclypticæ in qua eſt ſtella propoſita:
<
lb
/>
</
s
>
<
s
xml:id
="
echoid-s6568
"
xml:space
="
preserve
">quòd ſi autem latitudo ſtellæ aliud non habuerit quàm medietas eclypticæ, </
s
>
</
p
>
</
div
>
</
text
>
</
echo
>
