DETERMINATION OF ELLIPTIC ORBITS.
145
r
3
2
{\displaystyle r_{3}^{2}}
=
q
3
2
+
.7130624
{\displaystyle =q_{3}^{2}+.7130624}
}
{\displaystyle \scriptstyle {\left.{\begin{matrix}\ \\\\\ \\\ \\\ \\\ \\\ \\\ \ \end{matrix}}\right\}\,}}
III
3
{\displaystyle {\text{III}}_{3}}
corrected.
α
3
=
−
[
9.3810712
]
(
q
3
+
1.5798163
)
(
1
+
R
3
)
{\displaystyle \alpha _{3}=-[9.3810712](q_{3}+1.5798163)(1+R_{3})}
R
3
{\displaystyle R_{3}}
=
[
9.5619251
]
r
3
−
3
{\displaystyle =[9.5619251]r_{3}^{-3}}
β
3
=
+
[
9.6537283
]
(
q
3
−
.4630521
)
(
1
+
R
3
)
{\displaystyle \beta _{3}=+[9.6537283](q_{3}-.4630521)(1+R_{3})}
γ
3
=
+
[
8.8361231
]
(
q
3
+
.5599304
)
(
1
+
R
3
)
{\displaystyle \gamma _{3}=+[8.8361231](q_{3}+.5599304)(1+R_{3})}
Δ
q
3
{\displaystyle \Delta q_{3}}
+ .0003302
+.0000424
q
3
{\displaystyle q_{3}}
+
{\displaystyle +}
2.4036347
2.4039649
2.4040073
log
r
3
{\displaystyle \log r_{3}}
+
{\displaystyle +}
.4061399
.4061929
.4061998
log
R
3
{\displaystyle \log R_{3}}
+
{\displaystyle +}
8.3435055
8.3433463
8.3433257
log
(
1
+
R
3
)
{\displaystyle \log(1+R_{3})}
+
{\displaystyle +}
.094742
.0094708
.0094704
α
3
{\displaystyle \alpha _{3}}
−
{\displaystyle -}
.9790500
.9791236
.9791329
β
3
{\displaystyle \beta _{3}}
+
{\displaystyle +}
.8935824
.8937277
.8937461
γ
3
{\displaystyle \gamma _{3}}
+
{\displaystyle +}
.2076882
.2077097
.2077124
log
s
3
{\displaystyle \log s_{3}}
+
{\displaystyle +}
.1277120
With these corrected equations the last values of
q
1
,
q
2
,
q
3
{\displaystyle q_{1},q_{2},q_{3}}
give the residuals
α
=
.0001135
{\displaystyle \alpha =.0001135}
β
=
−
.0003934
{\displaystyle \beta =-.0003934}
γ
=
−
.0000326
{\displaystyle \gamma =-.0000326}
These give the corrections
Δ
q
1
=
.0002887
{\displaystyle \Delta q_{1}=.0002887}
Δ
q
2
=
−
.0000955
{\displaystyle \Delta q_{2}=-.0000955}
Δ
q
3
=
.0003302
{\displaystyle \Delta q_{3}=.0003302}
The next residuals are
α
=
.0000035
{\displaystyle \alpha =.0000035}
β
=
.0000140
{\displaystyle \beta =.0000140}
γ
=
−
.0000003
{\displaystyle \gamma =-.0000003}
which give the corrections
Δ
q
1
=
.
−
.0000217
{\displaystyle \Delta q_{1}=.-.0000217}
Δ
q
2
=
.0000187
{\displaystyle \Delta q_{2}=.0000187}
Δ
q
3
=
.0000424
{\displaystyle \Delta q_{3}=.0000424}
The next residuals are
α
=
−
.0000001
{\displaystyle \alpha =-.0000001}
β
=
.0000003
{\displaystyle \beta =.0000003}
γ
=
.0000000
{\displaystyle \gamma =.0000000}
which must be regarded as entirely insensible.
It remains to determine the ellipse which passes through the points to which the numbers relate in the last columns under the corrected equations
III
1
,
III
2
,
III
3
,
{\displaystyle {\text{III}}_{1},{\text{III}}_{2},{\text{III}}_{3},}
and also the time of perihelion passage. The computations are as follows: