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SuperNOVAS v1.3
The NOVAS C library, made better
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#include <novas.h>
Data Fields | |
double | dec |
[deg] apparent, topocentric, or astrometric declination (degrees) | |
double | dis |
[AU] true (geometric, Euclidian) distance to solar system body or 0.0 for star (AU) | |
double | r_hat [3] |
unit vector toward object (dimensionless) | |
double | ra |
[h] apparent, topocentric, or astrometric right ascension (hours) | |
double | rv |
Celestial object's place on the sky; contains the output from place()
double rv |
[km/s] radial velocity (km/s). As of SuperNOVAS v1.3, this is always a proper observer-based spectroscopic velocity measure, which relates the observed wavelength to the rest wavelength as λobs = (1 + rv / c) λrest.