CALCVLVS ECLIPSIS SOLIS. 39T 



F —.2911. I 



d zz 1015, I 

 A zz: P47. o 



A -{- d — 1962. I 

 Pro triangufo G 3 O. 

 tog. 3:=3<J2 8495i Log. O 3=3.^284954^ 

 £;fin.G3A— 9.^1 82809 Lcol 02)^=^9.9589077 



L. G t) — 3 24-6 77<^o L. 3 O =13.5874028 

 L. A O :=:2.98o54S7 3 O :::i38«S7. 3 



LT GAOz=io.2()(J2273 3) A 11:2911. I 



G AOn:(Ji°. 33' AO= 95<J. 2 ,- 



G 3 A zz 24. 32 Log.OO— 3.24^77<Jcj 



3GAz:37. t L.fin.GAO=:9.944io4i 



AOC:=:57. 8 L. G A zrL. Vi=:3.302<57i9 

 A O A z:: 20^ 7' O A zi: V — 2007. ^ 



Sumta Azrr z.Cia.z^, diftantiaOA roinuitur Tab. III. 

 particuh z. fin. 2 ^. cof. O A O =: o. 375-2 Deinde Fig. 8- 

 cclipticae duda parallela = j: + o. 591. , diftantia 

 OA m nuetur particula o, 939. .r 4; 0,555. 0. Deni- 

 qxre al cc'ipticam normaliter du(fta Aj rr A y — o, 

 cs€'.^ hinc diftantia OA augebitur particula o, s^^.j' 

 — o.,o2o. d, quocirca diftantia centrorum coreda 

 feperitnr , ' 



2007; 6-0,375..«— o, 939. x-\-o.. 3'44.J'-o, 575-^ 



D d d 3. fummae 



