Calculate the apparent geocentric equatorial coordinates of the Sun.
- Parameters
-
| jde | The julian ephemeris day number, which is based on TT. |
- Returns
- The apparent right ascension α (normalized to [0°, 360°)) and declination δ.
Composes geocentric_coord::apparent (ecliptic λ, β, with FK5 + nutation + aberration) with the true obliquity ε and Meeus (13.3)–(13.4) via coords::ecliptic_to_equatorial. The result is of-date apparent equatorial place of the Sun, suitable as input to sunrise/sunset hour-angle calculations.
- See also
- Jean Meeus, "Astronomical Algorithms", Second Edition, Chapters 13 and 25.