CALCVLVS ECLIPSIS SOLIS. 37^ 



G A0=:i2". 59' 



G3A=r 7. 23 Log. AO=3.25>0435-3 



■ ■■••n I 



3 0A— 5. 3<J Log.cof.GAO:=9.988753i 



SQA— 77. 32 ^;;Log,OA— 3.3oi<J8 2f 



.AGA = 7i. 5^ GAiz;Vn2003. o 



In 3A produda eapiatur As:zfj.^z:2;fin.;s3 Tab. Ut 

 quae diftantia GA minuitur particula zfm.z^coC- ^^'°' 

 GAO quae ergo reperitur : 0,398.3. Nunc duda 

 eclipticae parallela zza; +0,591.$, qua diftaritia 

 GA minuitur particula =z(.r-}-o. 591. 0) cof. AGA 

 rzo. ^io.x-f-o. 183 9. Denique eclipticae normali- 

 ter ducatur lineola Ajzizj— 0,056. vnde diftantia 

 GA incrementum capit zr (y — o, o5(J. O^fin. AO A 

 :zi 0.951.7—0,053.0. Quare diftanfia OA cor- 

 reda prodit 



2CO3. o — o j '398. % — o , 310.^ + 0, 951.J' 

 -0.235.$ aequanda furamae femidiametrorum -1957.6 

 •4- ^' vnde obtinetur fequens aequatio finalis 



35.4-<5~-o, 398.5;4o, 310. x-o, p^i.j^ + o, 235. $ 



Finis eclipfeos hoc loco obferuatus eft 24^.0^ 26'. 

 So^ vnde fit angulus Q¥ z zz: 5°, 42'. 30" ovtum ver- 

 fus. At huic momento refpondet Parifiis 21^. 8'. ^^ ' ^ ' 

 20" Temp. vef. fiue Temp. med 21^.6'. 12" vnde 

 tempus epochae fubtradum relinquit ;zz+3 5'.45"z=:o, 

 595ii, vndc' L((3-a);z=3. 1038290 at y t zz: 

 — 123.2 vnde 3Lz::/+ 7^— 3223. 5. 



TQm.XIV.Nou.Comm.ParsIL Bbb En 



