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The ecliptic latitude of Jupiter can be determined with the aid of Tables 50, 69, and 70. Table 50 allows
the mean argument of latitude,
, of Jupiter to be calculated as a function of
time. Next, Table 69 permits the deferential latitude,
, to
be determined as a function of the true argument of latitude,
. Finally, Table 70 allows the quantities
,
, and
to be calculated as functions of the epicyclic
anomaly,
. The procedure for using these tables is analogous to the previously described procedure for
using the Mars tables.
One example of this procedure is given below.
Example: May 5, 2005 CE, 00:00 UT:
From Cha. 8,
JD,
,
,
, and
.
Making use of
Table 50, we find:
|
|
(JD) |
![$\bar{F}(^\circ)$](img1234.png) |
|
|
+1000 |
![$83.081$](img1819.png) |
+900 |
![$74.773$](img1821.png) |
+50 |
![$4.154$](img1823.png) |
+.5 |
![$0.042$](img1824.png) |
Epoch |
![$293.660$](img2073.png) |
|
![$455.710$](img2074.png) |
Modulus |
![$95.710$](img2075.png) |
|
|
Thus,
It follows from Table 69 that
Since
, Table 70 yields
so
Finally,
Thus,
the ecliptic latitude of Jupiter at 00:00 UT on May 5, 2005 CE was
.
Next: Saturn
Up: Planetary Latitudes
Previous: Mars
Richard Fitzpatrick
2010-07-21