659!
TABLE GENERALE
Pour servir a calculer le mouvement
des Comètes dans un orbe Parabolique.
3
= s
3 2
Anomal.
vraye.
Diffé-
M. S.
n. jo27.1Ȕff. 4426. 12
-5- 39
Logarith.pour ladistanceau Soleil.
Moyen
mouvement.
Anomal.
vraye.
Diffé-
rences.
M. S.
24- 5 224 1723. 42
23. 1022. 38
22 0821. 38
21. Op
20. 4320. 16
19. 50ip. 26ip. 03
il" 35
45- 0442. 5640. 583»- 1037- 2835-JT434- 273 3- 053«. 4930. 3729. 30
28. 2827* 28
25. 39
24. 49
L ogithpour ladistanceu Soleil.
3
f 32 ^
3 **
3 3
Anomal.
vraye.
DifFé-
D.M.S.
Logarith.pour ladistanceau Soleil.
D. M. S.
I). M. S.
D.M.S-
142
144
146
148
i$o
202.32.41203.00.3 I
20} 27.47
123.54 Zl104.20.43
0.407380
0.411784
0.416232
0 4204300.424676
244
248
252
256
160
118.25. 5118.49.57Ii9.i4.i4119*37-56120. I. 6
0.5816160.5869220.592 2220.5972520.602301
640
660
680
700
>37-33-13138. 3-5»>38.33.2,>39- 1.29139.28.25
0.30.45
0.29.23
0.28.08
0.26.56
0.25.51
0.882575
0 8926490.9024010.922866
0 921022
IJ2
154
i$6
158
160
162
164
166
208
170
172
174
176
178
180
1©4 46.22105.II.33105.36.16106.00 32106.24.23
0.4288660.4330120.4371100.441164
0.445178
264
268
272
276
280
284
238
292
296
ZOO
120 23.44I2O.45.52121. 7.3O121.28.39121.49.22
0.6072740.6121740.6269980.6217500.62643 8
720
740
760
780
800
139.54.>6
140.19- 5140.42.5614 l-05.55141-28. 3
0.9299070.938,490.9469510-955 1140.963082
2 5. 2224. 4324. 162Z. 5123. 24
22. 57
22. 3322. 20
21. 57
22. 23
22. 02
20. 41
20. 20
20. 00I£. 40Ip. 22
29. 0318. 44
18. 27
0.24.490.23 510.22 590.22.08
106.47.4?
iO7.iO.44
207.3M7
207.55.2?
208.27.14
0.44P144
0.453060
0.456x36
0.460772
0.464208
122. 9.3S122.29.28222.48.54
123. 7*57123.26.36
0.631056
0.635608
0.640098
0.644525
0.648893
820
840
860
880
pOO
141.49.24
142.10 OO142.29.56
142.49.10143- 7.48
0.20.36O.I9.56O.19.140 18.380.17-03
0.17.30
0.16.57
0.16.28
0.16.00
4.J3.22
3.00.07
2.06.05
1*35*07
1.15.2»
1.01.47
0.52 000.44.360.38.530.34*190.30.36
0.970836
0.978397
0.985771
0.9929:0
1 OOOOOO
108.38.37
108.59.39209.20.20
209.40.40
2 IO.OO.4O
0.4683 1 80.4720300à»757c>t0.4793400.482937
310z 20
330
340
350
124.11.40
124.54-36
125.35.34
126.14.44
126.52.12
0.659559
0.669880
0.679876
0.689568
0.698970
92094095 O9801000
143.25 51>43.43.2114400.18
144.16.46
144.32.46
I.OO687I1.0235861.0201551.0265831.032876
182
184
186
288
ipo
2 20.20.20I 1 0.39.4IIlO.58.44
I I 2.27.28
m 35 55
O 4864989.4900220.493512
O.496965
0.500384
3603 70380390400
127.28. 6
128. 2.33128.3s.38
129. 7.27129.38. 4
0.708104
0.716976
0.725606
0.734006
0.742186
1500
2000
2500
3000
3500
149.26. 8152.26.15154.32.20156. 7.27157.22.49
1.158188
1.246058
1.313703
t.368678
I.414974
292
194
196
198.
200
222.54.05
122.22.58
2 22.29.34
2 2 2 46.55223. 4.OO
>7- 5327. 3617. 2127. 05
33-25
32. 27
32- Z230. 3929. 4929. 01
0.5037690.5072220.$104410.5137290.516984
420
420
430
440
450
130. 7-34130.36. 2
«31. 3-30«31.30. 2«3«.55-4«
0.7501600.7579300.7655160.77291 80.780148
4000
4500
JOOO
5500
6coo
158.24.36159.16.z6160. 2.12160.40. 5161.14.24
1.454950
2.490125
1.521521
1.549874
1.575718
204
208
212
2l6
220
2i3.37.25214. 9.52H4.4i.2Z
2 25 22.022i5.42.52
0.523406
0.529705
0.535886
0.541958
0.547922
460
470
480
490
500
132.20.30132.44.32133. 7.50133.30.25133-52.20
0.7872I60.7942220.8008820.807494
O.81396P
65^0
7000
7500
8000
8500
161.45.OO
162.12.34
162.37.34163.00.23163.21.20
1.599460
1.621417
1.64283
1.660922
1.678834
24. 0223. 2222. 35ri. 55
41. 5839- 4237* 2835* 3333 51
0.27.34
0.25.00
0.22.49
0.20.57
0.19.22
224
228
232
236
240
226.20.52226.39. ?227. 6.38227.33.27227.59.35
0.553782
0.559538
0.565199
0.570762
0.576233
520
540
560
580
600
«34-34 >8«35-14- 0
«35-51-28136.27. S137.OO.57
O.826522
O.8386OO
O.85OI87
O.861369
0.872155
9000
9500
toooo
50000
[ 00 DOC
163.40.42163.58.38164 15.20170.52.0
172.45.44
1.6957081.7116621.7267842.197960-.39-655
28. 2527. 3 1r6. 4926. 08
0.17.58
0.16.42
6.36.40--5 8-44
Le logarithme scfquialtere est déterminé, puisqu’il est toujours à celui de la distance Périhé-lie , comme 3 est à 2. Mais si l’on ajoute ensemble les trois logarithmes seivans, celui de la dis-tance Périhélie , le logarithme pour la distance, & celui du cosinus de la latitude, la sommefera le logarithme de la distance accourcie. O O 0 0 ij