Convert a direction (vector) to R.A. and Dec in Skyfield
问题 Within Skyfield, if I have a vector (x, y, z) from the center of the earth, how can I back-convert it to a point on the "Celestial Sphere" (i.e. Right Ascension and Declination)? For example purposes, suppose I have a few points in the orbit of a telescope around the earth, and I want to calculate the exact RA and Dec of the direction normal to the orbit - for whatever reason. Effects like aberration and gravitation can be neglected here - I'm just looking to transform a direction in ICRF to