Rotate full ecliptic longitude/latitude into the equator associated with the
explicitly supplied true obliquity. Both angles and the obliquity are degrees.
The source frame/corrections must already be appropriate: this rotation does
not add light time, aberration, precession or an ephemeris precision guarantee.
Rotate full ecliptic longitude/latitude into the equator associated with the explicitly supplied true obliquity. Both angles and the obliquity are degrees. The source frame/corrections must already be appropriate: this rotation does not add light time, aberration, precession or an ephemeris precision guarantee.