Function astro::star::angl_between_north_celes_and_eclip_pole

pub fn angl_between_north_celes_and_eclip_pole(eclip_long: f64, eclip_lat: f64, oblq_eclip: f64) -> f64

Computes the angle between a vector from a star to the north celestial pole of the Earth and a vector from the same star to the north pole of the ecliptic

Returns

• angle: The desired angle | in radians

Arguments

• eclip_long: The star's ecliptical longitude | in radians
• eclip_lat: The star's ecliptical latitude | in radians
• oblq_eclip: Obliquity of the ecliptic | in radians