last updated 02/14/10
The main steps in calculating the RA and DEC of a planet from the mean elements are:
Notation
Parameters
H - Absolute MAgnitude (Mag), Magnitude of object if it were at 0 phase angle and 1 AU from both sun and Observer
a - mean distance (AU), the value of the semi-major axis of the orbit
(AU - Astronomical Unit - average Sun to Earth distance)
e - eccentricity of the ellipse which describes the orbit (dimensionless)
i - inclination (degrees), angle between the plane of the ecliptic (the plane of Earth's orbit about the Sun) and the plane of the planets orbit
O - longitude of ascending node (degrees), the position in the orbit where the elliptical
path of the planet passes through the plane of the ecliptic, from below the
plane to above the plane
w - Argument of perihelion (degrees), the position in the orbit where the planet is closest to the Sun
T - Time of Periapsis(days), the last time the object was at periapsis in Julian Days
Calculated quantities
M - mean anomaly (degrees)
V - true anomaly (degrees)
R - heliocentric radius (AU)
X,Y,Z - rectangular coordinates (AU)
RA - right ascension (hour angle)
DEC - declination (degrees)
hmag - apparent brightness (mag) in whatever filter used for H
note: hmag for planets is for H at that planet's position
Coming soon?
printing object name in output
moon distance-to-planet calculator
Right here!
References