22 THE ORBIT OF NEPTUNE. 



II.— SATURN AND NEPTUNE. 





,w 



db't 



/K 



.'K 



i 



^\ 



da 



da'' 



„3 S 



•^ d.' 







2.05341 



0.11342 



0.14186 



0.0986 



1 



0.33010 



.35745 



.08964 



.1313 



2 



.07890 



.16509 



.19632 



.1075 



3 



.02091 



.06476 



.14027 



.1878 



4 



.00581 



.02383 



.07517 



.1701 



5 



.00166 



.00847 



.03514 







i 



"■^i 











0.8045 



0.4003 







1 



0.3686 



.5242 







2 



.1443 



.3456 







3 



.0531 



.1794 







4 



.0189 









5 



0066 







III.— JUPITER AND NEPTUNE. 



i 



(0 





«^ d) 



«^ dJ 







2.01518 



0.03088 



0.0330 



. 0.0067 



1 



0.17474 



.17876 



.0124 



.0139 



2 



.02267 



.04592 



.0483 



.0074 



3 



.00327 



.00989 



.0202 



.0221 



4 



.00049 



.00199 



.0061 



.0125 



dh''' 



i I 



da 







0.3699 



0.4209 



1 



.0948 



.2005 



2 



.0204 



.0634 



3 



.0041 



.0168 



4 



0.0008 





§ 13. From these data the coefficients li of the different terms of the perturb- 

 ative function, their differential coefficients, and the perturbations of the co- 

 ordinates, are found to be as in the following table. The N's, it will be seen, are 

 gi'ouped according to the values of their constant parts, /co'+yo. 



h, its differential coefficients, L, W, and JE, are given in units of the third place 

 of decimals, to avoid writing zeros. The logarithms are reduced to the common 

 base, 10, and are expressed in units of the seventh place. 



