Full text: Theoria motus corporum coelestium in sectionibus conicis solem ambientium (7. Band)

190 
LlBElt II. SECTIO I. 
Quum calculus liic prorsus eodem modo tractandus sit, ut in hypothesi 
prima, praecipua eius momenta hic apposuisse sufficiet: 
to 13° 15' 38" 13 
co + a 13 38 5 1,25 
log’ Q c sin io. . . 0,5989389 
2 14 33 19,00 
log/ 0,3259918 
loff— 0,6675193 
log’ V ~ir 0,5 885 029 
C 203 16 38,16 
C" 210° 8' 24”9 8 
logr 0,3307676 
log' v 0,3222280 
\{u"-\-u) . . 205 22 15,58 
i-{u"—u) . . —3 14 4,79 
2/ 7 34 53,32 
2/ 3 29 0, 18 
2 f" 4 5 5 3,12 
Reductiones temporum propter aberrationem denuo computarefoperae haud 
pretium esset, vix enim l” ab iis quas in hypothesi prima eruimus^differunt. 
Calculi ulteriores praebent log*vj = 0,0002270, log"/]"= 0,0003173, unde 
deducitur 
log P = 0,0790167, A r = -j- 0,0000003 
logQ = 8,5476110, Y= -j- 0,0000 129 
Hinc patet, quanto adhuc magis exacta sit hypothesis secunda quam prima. 
154. 
Ne quidquam desiderandum relinquatur, adhuc tertiam hypothesin ex- 
truemus, ubi rursus valores ipsarum P\ Q' in hypothesi secunda erutos tam 
quam valores ipsarum P, Q adoptabimus. Statuendo itaque 
x — lo gP = 0,0 790167 
y — log Q — 8,54761 10 
praecipua calculi momenta haec inveniuntur: 
. 13° 15'38” 39 
r" 
210° 8' 25 65 
co —0 . . . . 
. 13 38 51,51 
logr. . 
. . . 
. . 0,33 07640 
log' Q c sii i to. 
. . 0,5989542 
logr" . 
. . . 
. . 0,3222239 
z 
. 14 33 19,50 
*(«"+ 
u) . . 
205 22 14,57 
logr' . . . . 
. . 0,3259878 
\{u"— 
a) . . 
—3 14 4,78 
1 n r 
loo- — ... 
& n 
2/ . . 
. 7 34 53,73 
i n'r' 
10 g„- • • • 
. . 0,5884987 
2/ . . 
. . . 
. 3 29 0,39 
r 
203 16 3 8,4 1 
2f • . 
. 4 5 53, 34
	        
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