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Mean longitude is the ecliptic longitude at which an orbiting body could be found if its orbit were circular and free of perturbations. While nominally a simple longitude, in practice the mean longitude is a hybrid angle.^{[1]}
From these definitions, the mean longitude, l, is the angular distance the body would have from the reference direction if it moved with uniform speed,
measured along the ecliptic from ♈ to the ascending node, then up along the plane of the body's orbit to its mean position.^{[2]}
Mean longitude, like mean anomaly, does not measure an angle between any physical objects. It is simply a convenient uniform measure of how far around its orbit a body has progressed since passing the reference direction. While mean longitude measures a mean position and assumes constant speed, true longitude meausures the actual longitude and assumes the body has moved with its actual speed, which varies around its elliptical orbit. The difference between the two is known as the equation of the center.^{[3]}
From the above definitions, define the longitude of the pericenter, \varpi=\mathit{\Omega}+\omega. Then mean longitude is also^{[1]}
Another form often seen is the mean longitude at epoch, \epsilon. This is simply the mean longitude at a reference time t_0, known as the epoch. Mean longitude can then be expressed,^{[2]}
where n is the mean angular motion and t is any arbitrary time. In some sets of orbital elements, \epsilon is one of the six elements.^{[2]}
Julian day, Orbit, Terrestrial Time, Astronomy, Perturbation (astronomy)
Orbit, Mean anomaly, Parameter, Astronomy, Orbital mechanics
Orbit, Earth, Parabolic trajectory, Orbital period, Medium Earth orbit
Orbit, Moon, Equator, Mars, Goes