THE GENERAL PERTURBATIONS OF THE MINOR PLANETS. 12] 
we find 
IK NBO Is OAS log k = 9.999614 
Kee — lbOMeol T4 log k, = 9.997849 
3 Ari) log p = 9.932748 
Sa) © 2.4 log v = 0.601463 
W=266 4 39.5 log w = 0.605196 
W,=266 15 380. logw,= 0.601352 
Then from 
We Orn Oe Che ay apn Ole Clas 
we have 
log R = 0.702855, logy, = 7.976024. 
The values of the quantities from Il to y, should be found by a duplicate compu- 
tation without reference to the former computation, since any error in these quantities 
will affect all that follows. 
We now divide the circumference into sixteen parts relative to the mean anomaly, 
and find the corresponding values of the eccentric anomaly # from 
g= H—esn LH, 
where ¢ is regarded as expressed in seconds of are. Substituting the sixteen values 
of ¢ in the equations 
fsin (7 — P) =w sin (HH — W )—ep 
f cos (Ff — P) = w, cos(H+ W,), 
we obtain the corresponding values of f and /. 
A. P. 8S.—VOl. XIX. DP. 
