[Astronomiae Physicae & Geometricae Elementa] Astronomiæ Physicæ & Geometricæ Elementa, fol. 126
Machine transcription. Not an edition. Errors are expected: about 8% character error rate on Latin and French lines, higher on German. Mean line confidence on this page: 0.92.
Original at the GWLB · Page image · Annotations (IIIF) · Download text
The machine reads it as
- ASTRONOMLA PHYSIC A
- Lib. I
- 120
- Differentia gnonas elE ditterentia inter RIentionem rectam
- e obliquam. Faceique de Descensione Oolguu Lurc Incellisenda.
- In Sphard Parallela, UBI LIOLILOM H0 cum A quatoro RO coin
- cidit, unumque ex motiis diurni parallelis constituit, illorum LOI
- (nempe Lenith e Mundi Polus) etiam co-
- incident: adeoque hac Sphaera positio
- solis ad Dinos Terra Polos desentibus
- competit; omniaque Calescia per motum
- diurnum circulos Aiguatori parallelos
- describentia, describent etiam circulosTIO
- rixonti parallelos. Inde nullus erit per
- motum hunc diurnum ortus aut occatus,
- nullaque adeo in hac Sphaera AIcenSiODC.
- scentiore, nullusque Meridianus, cum hic
- per Polum locique verticem traducatur; cumque hi duo in hac Sphae-
- ra coincidant, circulum nequeunt determinare, quolibet verticali
- Meridiani nomen pari jure sibi vendicante. Solis vero phanomena
- ex motu Terra annuo oriunda, in Sphaera parallela conspicua, Prop.
- ZEXITT. LIb. P. explicata sunt; competentia nempe alterutrius Poli
- incolis. In Syctemate rero apparenti patet Solem, dum ad illum
- ab quatore Polum declinat qui Zenith occupat, perpetuo con-
- Epici, lemeltremque diem constituere; sicut ex adverlo lemeltrem
- ehse noctem, dum Sol ad alteras Aquatoris ac proinde FTorirontis
- partes declinat; dicique ee noctis initia incidere in Solis ingrestus
- in puncta quinoctialia.
- PROPOSEPEO VIT
- ddullo loci est arcus similis arcui elevationts Lod supra
- LorLCM.
- Sit acb9 Lelluo, Clsco Cerumt P, foI a aB, A. quator eg. Suma-
- tur in hujus superticie locus quiris I, cujus Latitudo eAt LC arcus MC.
- ridiani inter ipsum ee Aequatorem inter-
- ceptus. Sit concentrica Sphara Caloctis, cu
- jus Poli, sRquator, _ MeridianuS B, A, F. 9.
- e BF AO relpondeant Polis, Aiquatori, e
- Meridiano Terrestribus. Sit loci IZenith
- 2 _ NTadir n; nempe in recta rI produ.
- eta intersectionibus cum superticie spha
- rica Celesti. Ouare HO circulus in Sphae-
- ra maximus super Dolos 2 d V deseriptus
- eAt loci FToriron, e Meridiani arcus OB
- ell Altitudo Poli conspicui e supra Horizontem, quem aio similem
- elle arcui 2e, Latitudini nimirum loci. Nam quia a e B sunt Poli
- circuli E. C, CA (per PrOp. X. Lib. I. Sphaeric. Pheod.) ans ulUS B FF
- rectus; et ob eandem rationem ansulus 2 r0 est rectus. Si erso
- ab xqualibus P xB, Z. x0 auteratur communis angulus ZFB, rC.
- ligui
Cite
[Astronomiae Physicae & Geometricae Elementa] Astronomiæ Physicæ & Geometricæ Elementa, fol. 126. Machine transcription, not an edition: Leibniz Legible (model FoNDUE-GD_v2_ft_Leibniz, run 74). https://leibnizlegible.com/page/1040780814:0144?run=74