functions in kepler.i - m
moon
xyz = moon(time) return position XYZ of the moon relative to center of earth at TIME; the XYZ has leading dimension 3; x is along the vernal equinox, z is ecliptic north. The corrections to the lunar orbit are from Schlyter (see sch_moon). Claimed accurate to 2 arc minutes over some reasonable time. TIME is in days since 0/Jan/00 (that is, 0000 UT 31/Dec/99). This is 1.5 days earlier than the J2000 epoch. Interpreted function, defined at i/kepler.i line 261SEE ALSO: solar_system, sch_moon, kepler