Ege University Observatory Application ve Research Center
Latitude (φ): 38° 24' 16" N
Longitude (λ): 27° 10' 03" E
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Instantaneous Apparent Positions of Planets
The semi-analytical planetary theory VSOP87
(Bretagnon and Francou, 1988, A&A, 202, 309) was adopted for position calculations. The equations used in the
calculations are taken from the second edition of Jean Meeus's book "Astronomical Algorithms"
* Meeus, J. “Astronomical Algorithms”. Second edition
1998, Willmann-Bell, Inc.,Richmond, Virginia, USA.
| Planet | α (h:m) | δ (d:m) | Distance to the Sun (AU) | Azimuth (d) | Altitude (d) |
|---|---|---|---|---|---|
| Mercury | |||||
| Venus | |||||
| Mars | |||||
| Jupiter | |||||
| Saturn | |||||
| Uranus | |||||
| Neptune |
