Ecliptic coordinate transforms.
Summary
Functions
Convert an ecliptic cartesian vector to longitude/latitude in degrees.
Rotate an ICRF vector into the J2000 ecliptic frame.
Compute J2000 ecliptic longitude/latitude from an ICRF vector.
Rotate an ICRF vector into the mean-of-date ecliptic frame.
Compute mean-of-date ecliptic longitude/latitude from an ICRF vector.
Rotate an ICRF vector into the true-of-date ecliptic frame.
Compute true-of-date ecliptic longitude/latitude from an ICRF vector.
Functions
Convert an ecliptic cartesian vector to longitude/latitude in degrees.
Rotate an ICRF vector into the J2000 ecliptic frame.
Compute J2000 ecliptic longitude/latitude from an ICRF vector.
@spec icrf_to_mean_ecliptic_of_date({float(), float(), float()}, float()) :: {float(), float(), float()}
Rotate an ICRF vector into the mean-of-date ecliptic frame.
Compute mean-of-date ecliptic longitude/latitude from an ICRF vector.
@spec icrf_to_true_ecliptic_of_date({float(), float(), float()}, float()) :: {float(), float(), float()}
Rotate an ICRF vector into the true-of-date ecliptic frame.
Compute true-of-date ecliptic longitude/latitude from an ICRF vector.