d Gatin X,
oſtäteng
) buspron r graptin tis kipgn r. Arnahn , decimin „horisdir ber inte wenitzlen us Lunad. in Xwen XXINgN us gradus edianteinl duo aroun aiterid ſit lonpiudn ec conldm 1s horsar zuinociült xta prtr propio 1 jri decellu Scũ ſaxuam quad hc „Cancripa „unde ay vn. ſelxl dũ meylti e alummi ſtram.Pbd- nà2 cendl
däc
dem //23.& angulus qui ſub 2α partium XII.
REVOLVTIONVM LIB. IIII. 72
eius c, dimetiens Ac. quæ extendatur in rectam lineam ad cen trum terræ, ſitq; à ², capiatur etiam in epicyclo circumferentia A BꝝE partium cccxxxXIII.& coniungantur oꝝ, quæ reſecetur in v, ut ſit Ey partium 2357. quarum ² c eſtοονη.& facto in ꝝ cen tro diſtantia nx deſcribat᷑ epicycli epicyclium r. 4 Sitq; Luna in a ſigno. Circumferentia autem ro ₰oℳ 4. partium xc. ſcrup. x. ratione dupli motus æqua⸗ NM lis à Sole, qui erat part. xL v. ſcrup. v.& conne⸗ I ctantur cs, E, p. Quoniam igitur trianguli ES, dantur duo latera on partium)⁹ν. R& EG 237. æqualis ipſi E ꝶ cum angulo a ν partium xc ſcrup. x. Dantur ergo per demonſtrata triangu⸗ lorum planorum reliquum latus oc partium earun
ſcrup.xi. quibus conſtat etiam circumferentia u, ac proſthaphæreſis adiectiua anomaliæ: fitq́; tota KEEG, partium cccxαv. ſcrup. X.& reliquus G&, angulus partium X IIII. ſcrup. xL. vrI. ueræ diſtantiæ lunaris à ſumma abſide epicycli à 2,& angulus Bα partium cLXv. Xl. Quapropter& trianguli& p o duo quoq; latera data ſunt opart. 23. quarũ op ſunt decẽ miliũ,& op angulus part. cLX v. xl. Habebimus etiã ex his anguluu opo par tis unius, ſcrup. primorũ x αeιαη.& ꝓſthaphæreſim quæ medio motui Lunæ addebat᷑, ut eſſet uera Lu næ diſtãtia à medio motu Solis part. xxL vi. ſcrup. XXXIII.& locus eius apparẽs in xx VilI. xxXVII. 5 Leonis.diſtans à uero loco Solis part. xL VII. ſcru. L vi. deficiẽtibus ab Hipparchi cõſideratiõe ſcrup. primis no-⸗ uem. Verũ ne ꝗs ꝓpterea, uel illius inꝗſitionẽ, uel noſtrũ feſel- liſſe numerũ ſuſpicet᷑, q;uis id modicũ ſit, oſtendemus tñ, nec il⸗ lũ, nec nos errorẽ cõmiſiſſe, ſed hoc modo recte ſe habere. Si e⸗ nim meminerimus lunarẽ obliquũ eſſe circulũ, quẽ ipſa ſeꝗtur, latebimur etiã in ſignifero aliꝗd lõgitudini diuerſitatis ees maxie circa media loca, ꝗᷓ int᷑ utroſq; limites Boreũ& Auſtrinũ & utraſq; eclipticas ſunt ſectiões, eo ferè modo, ut int obliꝗtatẽ ſigniſeri


