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SuperNOVAS v1.5
The NOVAS C library, made better
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Data Structures | |
struct | novas_observable |
Spherical and spectral coordinate set. More... | |
struct | novas_track |
The spherical and spectral tracking position of a source, and its first and second time derivatives. More... | |
struct | sky_pos |
Celestial object's place on the sky; contains the output from place() More... | |
Macros | |
#define | DEFAULT_GRAV_BODIES_FULL_ACCURACY ( DEFAULT_GRAV_BODIES_REDUCED_ACCURACY | (1 << NOVAS_JUPITER) | (1 << NOVAS_SATURN) ) |
Default set of gravitating bodies to use for deflection calculations in full accuracy mode. | |
#define | DEFAULT_GRAV_BODIES_REDUCED_ACCURACY ( (1 << NOVAS_SUN) ) |
Default set of gravitating bodies to use for deflection calculations in reduced accuracy mode. | |
#define | NOVAS_OBSERVABLE_INIT |
Empty initializer for novas_observable. | |
#define | NOVAS_TRACK_INIT |
Empty initializer for novas_track. | |
#define | SKY_POS_INIT |
Initializer for a NOVAS sky_pos structure. | |
Functions | |
short | app_planet (double jd_tt, const object *restrict ss_body, enum novas_accuracy accuracy, double *restrict ra, double *restrict dec, double *restrict dis) |
reference_system: TOD observer location: geocenter position_type: apparent | |
short | app_star (double jd_tt, const cat_entry *restrict star, enum novas_accuracy accuracy, double *restrict ra, double *restrict dec) |
reference_system: TOD observer location: geocenter position_type: apparent | |
int | limb_angle (const double *pos_src, const double *pos_obs, double *restrict limb_ang, double *restrict nadir_ang) |
Determines the angle of an object above or below the Earth's limb (horizon). | |
int | novas_app_to_geom (const novas_frame *restrict frame, enum novas_reference_system sys, double ra, double dec, double dist, double *restrict geom_icrs) |
Converts an observed apparent sky position of a source to an ICRS geometric position, by undoing the gravitational deflection and aberration corrections. | |
int | novas_app_to_hor (const novas_frame *restrict frame, enum novas_reference_system sys, double ra, double dec, RefractionModel ref_model, double *restrict az, double *restrict el) |
Converts an observed apparent position vector in the specified coordinate system to local horizontal coordinates in the specified observer frame. | |
int | novas_approx_sky_pos (enum novas_planet id, const novas_frame *restrict frame, enum novas_reference_system sys, sky_pos *restrict out) |
Calculates an approximate apparent location on sky for a major planet, Sun, Moon, Earth-Moon Barycenter (EMB) – typically to arcmin level accuracy – using Keplerian orbital elements. | |
double | novas_equ_sep (double ra1, double dec1, double ra2, double dec2) |
Returns the angular separation of two equatorial locations on a sphere. | |
int | novas_equ_track (const object *restrict source, const novas_frame *restrict frame, double dt, novas_track *restrict track) |
Calculates equatorial tracking position and motion (first and second time derivatives) for the specified source in the given observing frame. | |
int | novas_hor_track (const object *restrict source, const novas_frame *restrict frame, RefractionModel ref_model, novas_track *restrict track) |
Calculates horizontal tracking position and motion (first and second time derivatives) for the specified source in the given observing frame. | |
double | novas_moon_angle (const object *restrict source, const novas_frame *restrict frame) |
Returns the apparent angular distance of a source from the Moon from the observer's point of view. | |
double | novas_moon_phase (double jd_tdb) |
Calculates the Moon's phase at a given time. | |
double | novas_object_sep (const object *source1, const object *source2, const novas_frame *restrict frame) |
Returns the angular separation of two objects from the observer's point of view. | |
double | novas_sep (double lon1, double lat1, double lon2, double lat2) |
Returns the angular separation of two locations on a sphere. | |
int | novas_sky_pos (const object *restrict object, const novas_frame *restrict frame, enum novas_reference_system sys, sky_pos *restrict out) |
Calculates an apparent location on sky for the source. | |
double | novas_solar_illum (const object *restrict source, const novas_frame *restrict frame) |
Returns the Solar illumination fraction of a source, assuming a spherical geometry for the observed body. | |
double | novas_sun_angle (const object *restrict source, const novas_frame *restrict frame) |
Returns the apparent angular distance of a source from the Sun from the observer's point of view. | |
int | novas_track_pos (const novas_track *track, const novas_timespec *time, double *restrict lon, double *restrict lat, double *restrict dist, double *restrict z) |
Calculates a projected position, distance, and redshift for a source, given its near-term trajectory on sky, in the system for which the track was calculated. | |
int | novas_transform_sky_pos (const sky_pos *in, const novas_transform *restrict transform, sky_pos *out) |
Transforms a position or velocity 3-vector from one coordinate reference system to another. | |
int | place_cirs (double jd_tt, const object *restrict source, enum novas_accuracy accuracy, sky_pos *restrict pos) |
reference_system: CIRS observer location: geocenter position_type: apparent | |
int | place_gcrs (double jd_tt, const object *restrict source, enum novas_accuracy accuracy, sky_pos *restrict pos) |
reference_system: ICRS/GCRS observer location: geocenter position_type: apparent | |
int | place_j2000 (double jd_tt, const object *restrict source, enum novas_accuracy accuracy, sky_pos *restrict pos) |
reference_system: J2000 observer location: geocenter position_type: apparent | |
int | place_mod (double jd_tt, const object *restrict source, enum novas_accuracy accuracy, sky_pos *restrict pos) |
reference_system: MOD observer location: geocenter position_type: apparent | |
int | place_tod (double jd_tt, const object *restrict source, enum novas_accuracy accuracy, sky_pos *restrict pos) |
reference_system: TOD observer location: geocenter position_type: apparent | |
short | virtual_planet (double jd_tt, const object *restrict ss_body, enum novas_accuracy accuracy, double *restrict ra, double *restrict dec, double *restrict dis) |
reference_system: ICRS / GCRS observer location: geocenter position_type: apparent | |
short | virtual_star (double jd_tt, const cat_entry *restrict star, enum novas_accuracy accuracy, double *restrict ra, double *restrict dec) |
reference_system: ICRS / GCRS observer location: geocenter position_type: apparent | |
Variables | |
int | grav_bodies_full_accuracy |
Current set of gravitating bodies to use for deflection calculations in full accuracy mode. | |
int | grav_bodies_reduced_accuracy |
Current set of gravitating bodies to use for deflection calculations in reduced accuracy mode. | |
#define DEFAULT_GRAV_BODIES_FULL_ACCURACY ( DEFAULT_GRAV_BODIES_REDUCED_ACCURACY | (1 << NOVAS_JUPITER) | (1 << NOVAS_SATURN) ) |
Default set of gravitating bodies to use for deflection calculations in full accuracy mode.
#define DEFAULT_GRAV_BODIES_REDUCED_ACCURACY ( (1 << NOVAS_SUN) ) |
Default set of gravitating bodies to use for deflection calculations in reduced accuracy mode.
(only apply gravitational deflection for the Sun.)
#define NOVAS_OBSERVABLE_INIT |
#define NOVAS_TRACK_INIT |
short app_planet | ( | double | jd_tt, |
const object *restrict | ss_body, | ||
enum novas_accuracy | accuracy, | ||
double *restrict | ra, | ||
double *restrict | dec, | ||
double *restrict | dis ) |
reference_system: TOD
observer location: geocenter
position_type: apparent
Computes the True-of-Date (TOD) apparent place of a solar system body as would be seen by an observer at the geocenter. This is the same as calling place() for the body with NOVAS_TOD as the system and a geocentric observer, except the different set of return values used.
The calculated positions and velocities include aberration corrections for the moving frame of the observer as well as gravitational deflection due to the Sun and Earth and other major gravitating bodies in the Solar system, provided planet positions are available via a novas_planet_provider function.
REFERENCES:
jd_tt | [day] Terretrial Time (TT) based Julian date. | |
ss_body | Pointer to structure containing the body designation for the solar system body. | |
accuracy | NOVAS_FULL_ACCURACY (0) or NOVAS_REDUCED_ACCURACY (1) | |
[out] | ra | [h] Apparent (TOD) right ascension for a fictitous geocentric observer, referred to true equator and equinox of date 'jd_tt'. (It may be NULL if not required) |
[out] | dec | [deg] Apparent (TOD) declination for a fictitous geocentric observer, referred to true equator and equinox of date 'jd_tt'. (It may be NULL if not required) |
[out] | dis | [AU] Apparent distance from Earth to the body at 'jd_tt' (it may be NULL if not needed). |
References NOVAS_TOD, and radec_planet().
short app_star | ( | double | jd_tt, |
const cat_entry *restrict | star, | ||
enum novas_accuracy | accuracy, | ||
double *restrict | ra, | ||
double *restrict | dec ) |
reference_system: TOD
observer location: geocenter
position_type: apparent
Computes the True-of-Date (TOD) apparent place of a star, as would be seen by an observer at the geocenter, referenced to the dynamical equator of date, given its catalog mean place, proper motion, parallax, and radial velocity.
Notwithstanding the different set of return values, this is the same as calling place_star() with a NULL observer location and NOVAS_TOD as the system for an object that specifies the star.
The calculated positions and velocities include aberration corrections for the moving frame of the observer as well as gravitational deflection due to the Sun and Earth and other major gravitating bodies in the Solar system, provided planet positions are available via a novas_planet_provider function.
REFERENCES:
jd_tt | [day] Terretrial Time (TT) based Julian date. | |
star | Pointer to catalog entry structure containing catalog data for the object in the ICRS. | |
accuracy | NOVAS_FULL_ACCURACY (0) or NOVAS_REDUCED_ACCURACY (1) | |
[out] | ra | [h] Apparent (TOD) right ascension for a fictitous geocentric observer, referred to true equator and equinox of date 'jd_tt' (it may be NULL if not required). |
[out] | dec | [deg] Apparent (TOD) declination in degrees for a fictitous geocentric observer, referred to true equator and equinox of date 'jd_tt' (it may be NULL if not required). |
References NOVAS_TOD, and radec_star().
int limb_angle | ( | const double * | pos_src, |
const double * | pos_obs, | ||
double *restrict | limb_ang, | ||
double *restrict | nadir_ang ) |
Determines the angle of an object above or below the Earth's limb (horizon).
The geometric limb is computed, assuming the Earth to be an airless sphere (no refraction or oblateness is included). The observer can be on or above the Earth. For an observer on the surface of the Earth, this function returns the approximate unrefracted elevation.
pos_src | [AU] Position 3-vector of observed object, with respect to origin at geocenter, components in AU. | |
pos_obs | [AU] Position 3-vector of observer, with respect to origin at geocenter, components in AU. | |
[out] | limb_ang | [deg] Angle of observed object above (+) or below (-) limb in degrees, or NAN if reurning with an error. It may be NULL if not required. |
[out] | nadir_ang | Nadir angle of observed object as a fraction of apparent radius of limb: lt;1.0 if below the limb; 1.0 on the limb; or >1.0 if above the limb. Returns NAN in case of an error return. It may be NULL if not required. |
References M_PI, and novas_vlen().
int novas_app_to_geom | ( | const novas_frame *restrict | frame, |
enum novas_reference_system | sys, | ||
double | ra, | ||
double | dec, | ||
double | dist, | ||
double *restrict | geom_icrs ) |
Converts an observed apparent sky position of a source to an ICRS geometric position, by undoing the gravitational deflection and aberration corrections.
frame | The observer frame, defining the location and time of observation | |
sys | The reference system in which the observed position is specified. | |
ra | [h] Observed ICRS right-ascension of the source | |
dec | [deg] Observed ICRS declination of the source | |
dist | [AU] Observed distance from observer. A value of <=0 will translate to 1015 AU (around 5 Gpc). | |
[out] | geom_icrs | [AU] The corresponding geometric position for the source, in ICRS. |
References grav_undo_planets(), NOVAS_CIRS, NOVAS_ITRS, NOVAS_J2000, NOVAS_MOD, NOVAS_REFERENCE_SYSTEMS, NOVAS_TIRS, NOVAS_TOD, radec2vector(), spin(), wobble(), and WOBBLE_ITRS_TO_TIRS.
int novas_app_to_hor | ( | const novas_frame *restrict | frame, |
enum novas_reference_system | sys, | ||
double | ra, | ||
double | dec, | ||
RefractionModel | ref_model, | ||
double *restrict | az, | ||
double *restrict | el ) |
Converts an observed apparent position vector in the specified coordinate system to local horizontal coordinates in the specified observer frame.
The observer must be located on the surface of Earth, or else the call will return with an error. The caller may optionally supply a refraction model of choice to calculate an appropriate elevation angle that includes a refraction correction for Earth's atmosphere. If no such model is provided the calculated elevation will be the astrometric elevation without a refraction correction.
frame | Observer frame, defining the time and place of observation (on Earth). | |
sys | Astronomical coordinate system in which the observed position is given. | |
ra | [h] Observed apparent right ascension (R.A.) coordinate | |
dec | [deg] Observed apparent declination coordinate | |
ref_model | An appropriate refraction model, or NULL to calculate unrefracted elevation. Depending on the refraction model, you might want to make sure that the weather parameters were set when the observing frame was defined. | |
[out] | az | [deg] Calculated azimuth angle. It may be NULL if not required. |
[out] | el | [deg] Calculated elevation angle. It may be NULL if not required. |
References novas_timespec::fjd_tt, novas_timespec::ijd_tt, itrs_to_hor(), NOVAS_AIRBORNE_OBSERVER, NOVAS_CIRS, NOVAS_GCRS, NOVAS_ICRS, NOVAS_ITRS, NOVAS_J2000, NOVAS_MOD, NOVAS_OBSERVER_ON_EARTH, NOVAS_REFRACT_ASTROMETRIC, NOVAS_TIRS, NOVAS_TOD, radec2vector(), spin(), wobble(), WOBBLE_PEF_TO_ITRS, and WOBBLE_TIRS_TO_ITRS.
int novas_approx_sky_pos | ( | enum novas_planet | id, |
const novas_frame *restrict | frame, | ||
enum novas_reference_system | sys, | ||
sky_pos *restrict | out ) |
Calculates an approximate apparent location on sky for a major planet, Sun, Moon, Earth-Moon Barycenter (EMB) – typically to arcmin level accuracy – using Keplerian orbital elements.
The returned position is antedated for light-travel time (for Solar-System bodies). It also applies an appropriate aberration correction (but not gravitational deflection).
The orbitals can provide planet positions to arcmin-level precision for the rocky inner planets, and to a fraction of a degree precision for the gas and ice giants and Pluto. The accuracies for Uranus, Neptune, and Pluto are significantly improved (to the arcmin level) if used in the time range of 1800 AD to 2050 AD. For a more detailed summary of the typical accuracies, see either of the top two references below.
For accurate positions, you should use planetary ephemerides (such as the JPL ephemerides via the CALCEPH or CSPICE plugins) and novas_sky_pos()
instead.
While this function is generally similar to creating an orbital object with an orbit initialized with novas_make_planet_orbit()
or novas_make_moon_orbit()
, and then calling novas_sky_pos()
, there are a few important differences to note:
novas_make_planet_orbit()
does not provide orbitals for the Earth directly, and make_moot_orbit()
references the Moon's orbital to the Earth position returned by the currently configured planet calculator function (see set_planet_provider()
). REFERENCES:
id | NOVAS major planet ID. All major planets, plus the Sun, Moon, Earth-Moon Barycenter (EMB), and Pluto system Barycenter are supported. (For Pluto, the Pluto System Barycenter values are returned.) | |
frame | The observer frame, defining the location and time of observation. | |
sys | The coordinate system in which to return the apparent sky location. | |
[out] | out | Pointer to the data structure which is populated with the calculated approximate apparent location in the designated coordinate system. |
References make_planet(), novas_approx_heliocentric(), novas_geom_to_app(), novas_get_time(), NOVAS_TDB, novas_vlen(), and rad_vel2().
double novas_equ_sep | ( | double | ra1, |
double | dec1, | ||
double | ra2, | ||
double | dec2 ) |
Returns the angular separation of two equatorial locations on a sphere.
ra1 | [h] right ascension of first location |
dec1 | [deg] declination of first location |
ra2 | [h] right ascension of second location |
dec2 | [deg] declination of second location |
References novas_sep().
int novas_equ_track | ( | const object *restrict | source, |
const novas_frame *restrict | frame, | ||
double | dt, | ||
novas_track *restrict | track ) |
Calculates equatorial tracking position and motion (first and second time derivatives) for the specified source in the given observing frame.
The position and its derivatives are calculated via the more precise IAU2006 method, and CIRS.
source | Observed source | |
frame | Observing frame, defining the observer location and astronomical time of observation. | |
dt | [s] Time step used for calculating derivatives. | |
[out] | track | Output tracking parameters to populate |
References sky_pos::dec, sky_pos::dis, novas_timespec::fjd_tt, ira_equinox(), NOVAS_CIRS, novas_make_frame(), novas_sky_pos(), NOVAS_TRUE_EQUINOX, novas_v2z(), sky_pos::ra, sky_pos::rv, and SKY_POS_INIT.
int novas_hor_track | ( | const object *restrict | source, |
const novas_frame *restrict | frame, | ||
RefractionModel | ref_model, | ||
novas_track *restrict | track ) |
Calculates horizontal tracking position and motion (first and second time derivatives) for the specified source in the given observing frame.
The position and its derivatives are calculated via the more precise IAU2006 method, and CIRS, and then converted to local horizontal coordinates using the specified refraction model (if any).
source | Observed source | |
frame | Observing frame, defining the observer location and astronomical time of observation. | |
ref_model | Refraction model to use, or NULL for an unrefracted track. | |
[out] | track | Output tracking parameters to populate |
References sky_pos::dec, sky_pos::dis, novas_timespec::fjd_tt, ira_equinox(), NOVAS_AIRBORNE_OBSERVER, novas_app_to_hor(), NOVAS_CIRS, novas_make_frame(), NOVAS_OBSERVER_ON_EARTH, novas_sky_pos(), NOVAS_TOD, NOVAS_TRUE_EQUINOX, novas_v2z(), sky_pos::ra, sky_pos::rv, and SKY_POS_INIT.
double novas_moon_angle | ( | const object *restrict | source, |
const novas_frame *restrict | frame ) |
Returns the apparent angular distance of a source from the Moon from the observer's point of view.
source | An observed source |
frame | Observing frame, defining the observer location and astronomical time of observation. |
References NOVAS_MOON_INIT, and novas_object_sep().
double novas_moon_phase | ( | double | jd_tdb | ) |
Calculates the Moon's phase at a given time.
It uses orbital models for Earth (E.M. Standish and J.G. Williams 1992), and for the Moon (Chapront, J. et al., 2002), and takes into account the slightly eccentric nature of both orbits.
NOTES:
REFERENCES:
jd_tdb | [day] Barycentric Dynamical Time (TDB) based Julian Date. |
References NOVAS_EMB, novas_make_moon_orbit(), novas_make_planet_orbit(), NOVAS_ORBIT_INIT, novas_orbit_native_posvel(), and vector2radec().
double novas_object_sep | ( | const object * | source1, |
const object * | source2, | ||
const novas_frame *restrict | frame ) |
Returns the angular separation of two objects from the observer's point of view.
The calculated separation includes light-time corrections, aberration and gravitational deflection for both sources, and thus represents a precise observed separation between the two sources.
source1 | An observed source |
source2 | Another observed source |
frame | Observing frame, defining the observer location and astronomical time of observation. |
References sky_pos::dec, sky_pos::dis, novas_equ_sep(), NOVAS_GCRS, novas_sky_pos(), sky_pos::ra, and SKY_POS_INIT.
double novas_sep | ( | double | lon1, |
double | lat1, | ||
double | lon2, | ||
double | lat2 ) |
Returns the angular separation of two locations on a sphere.
lon1 | [deg] longitude of first location |
lat1 | [deg] latitude of first location |
lon2 | [deg] longitude of second location |
lat2 | [deg] latitude of second location |
int novas_sky_pos | ( | const object *restrict | object, |
const novas_frame *restrict | frame, | ||
enum novas_reference_system | sys, | ||
sky_pos *restrict | out ) |
Calculates an apparent location on sky for the source.
The position takes into account the proper motion (for sidereal source), or is antedated for light-travel time (for Solar-System bodies). It also applies an appropriate aberration correction and gravitational deflection of the light.
To calculate corresponding local horizontal coordinates, you can pass the output RA/Dec coordinates to novas_app_to_hor(). Or to calculate apparent coordinates in other systems, you may pass the result to novas_transform_sy_pos() after.
And if you want geometric positions instead (not corrected for aberration or gravitational deflection), you may want to use novas_geom_posvel() instead.
The approximate 'inverse' of this function is novas_app_to_geom().
This function implements the same aberration and gravitational deflection corrections as place()
, but at reduced computational cost. See place()
for references. Unlike place()
, however, the output always reports the distance calculated from the parallax for sidereal sources. Note also, that while place()
does not apply aberration and gravitational deflection corrections when sys
is NOVAS_ICRS (3), this routine will apply those corrections consistently for all coordinate systems (and you can use novas_geom_posvel() instead to get positions without aberration or deflection in any system).
NOTES:
object | Pointer to a celestial object data structure that is observed. Catalog sources should have coordinates and properties in ICRS. You can use transform_cat() to convert catalog entries to ICRS as necessary. | |
frame | The observer frame, defining the location and time of observation. | |
sys | The coordinate system in which to return the apparent sky location. | |
[out] | out | Pointer to the data structure which is populated with the calculated apparent location in the designated coordinate system. |
References grav_planets(), NOVAS_CATALOG_OBJECT, NOVAS_FULL_ACCURACY, novas_geom_posvel(), novas_geom_to_app(), NOVAS_ICRS, NOVAS_REDUCED_ACCURACY, novas_vlen(), rad_vel2(), and object::type.
double novas_solar_illum | ( | const object *restrict | source, |
const novas_frame *restrict | frame ) |
Returns the Solar illumination fraction of a source, assuming a spherical geometry for the observed body.
source | Observed source. Usually a Solar-system source. (For other source types, 1.0 is returned by default.) |
frame | Observing frame, defining the observer location and astronomical time of observation. |
References NOVAS_CATALOG_OBJECT, novas_geom_posvel(), NOVAS_ICRS, and novas_vlen().
double novas_sun_angle | ( | const object *restrict | source, |
const novas_frame *restrict | frame ) |
Returns the apparent angular distance of a source from the Sun from the observer's point of view.
source | An observed source |
frame | Observing frame, defining the observer location and astronomical time of observation. |
References novas_object_sep(), and NOVAS_SUN_INIT.
int novas_track_pos | ( | const novas_track * | track, |
const novas_timespec * | time, | ||
double *restrict | lon, | ||
double *restrict | lat, | ||
double *restrict | dist, | ||
double *restrict | z ) |
Calculates a projected position, distance, and redshift for a source, given its near-term trajectory on sky, in the system for which the track was calculated.
Thus if the input track was obtained with novas_hor_track()
it will calculate momentary azimuth and elevation (Az/El) for the specified proximate time. And, if you used novas_equ_track()
then it will give you theinstantaneous R.A. and declination for that time.
Using the quadratic trajectories via a novas_track
to project positions can be much faster than the repeated full recalculation of the source position, but still quite accurate over a suffciently brief period.
In SuperNOVAS terminology a 'track' is a 2nd order Taylor series expansion of the observed position and redshift in time. For most but the fastest moving sources, horizontal (Az/El) tracks are sufficiently precise for telescope positioning on minute timescales, whereas depending on the type of source, equatorial tracks can be precise for up to days, especially for sidereal (non-Solar-system) sources.
track | Tracking position and motion (first and second derivatives), obtained e.g. in horizontal (Az/El) coordinates with novas_hor_track() or in equatorial coordinates with novas_equ_track() . | |
time | Astrometric time of observation for which to calculate projected positions, around the time for which the track was obtained. | |
[out] | lon | [deg] projected observed Eastward longitude in the tracking coordinate system. Thus, if the track was calculated with novas_hor_track() it will return the projected azimuth coordinate for the given time. And, if you used novas_equ_track() , then this will be R.A. (in degrees, nevertheless). |
[out] | lat | [deg] projected observed latitude in the tracking coordinate system. Thus, if the track was calculated with novas_hor_track() it will return the projected elevation angle for the given time. And, if you used novas_equ_track() , then this will be declination. |
[out] | dist | [AU] projected apparent distance to source from observer. |
[out] | z | projected observed redshift (z = Δλ / λrest, e.g. for spectroscopy). |
References novas_track::accel, novas_observable::dist, novas_observable::lat, novas_observable::lon, novas_diff_time(), novas_track::pos, novas_track::rate, novas_track::time, and novas_observable::z.
int novas_transform_sky_pos | ( | const sky_pos * | in, |
const novas_transform *restrict | transform, | ||
sky_pos * | out ) |
Transforms a position or velocity 3-vector from one coordinate reference system to another.
in | Input apparent position on sky in the original coordinate reference system | |
transform | Pointer to a coordinate transformation matrix | |
[out] | out | Output apparent position on sky in the new coordinate reference system. It may be the same as the input. |
References sky_pos::dec, sky_pos::r_hat, sky_pos::ra, and vector2radec().
int place_cirs | ( | double | jd_tt, |
const object *restrict | source, | ||
enum novas_accuracy | accuracy, | ||
sky_pos *restrict | pos ) |
reference_system: CIRS
observer location: geocenter
position_type: apparent
Computes the Celestial Intermediate Reference System (CIRS) dynamical position position of a source as 'seen' from the geocenter at the given time of observation. See place()
for more information.
The calculated positions and velocities include aberration corrections for the moving frame of the observer as well as gravitational deflection due to the Sun and Earth and other major gravitating bodies in the Solar system, provided planet positions are available via a novas_planet_provider function.
jd_tt | [day] Terrestrial Time (TT) based Julian date of observation. | |
source | Catalog source or solar_system body. | |
accuracy | NOVAS_FULL_ACCURACY (0) or NOVAS_REDUCED_ACCURACY (1) | |
[out] | pos | Structure to populate with the calculated apparent CIRS position data for a fictitous geocentric observer. |
References NOVAS_CIRS, and place().
int place_gcrs | ( | double | jd_tt, |
const object *restrict | source, | ||
enum novas_accuracy | accuracy, | ||
sky_pos *restrict | pos ) |
reference_system: ICRS/GCRS
observer location: geocenter
position_type: apparent
Computes the Geocentric Celestial Reference System (GCRS) position of a source (as 'seen' from the geocenter) at the given time of observation. Unlike place_icrs()
, this includes aberration for the moving frame of the geocenter as well as gravitational deflections calculated for a virtual observer located at the geocenter. See place()
for more information.
jd_tt | [day] Terrestrial Time (TT) based Julian date of observation. | |
source | Catalog source or solar_system body. | |
accuracy | NOVAS_FULL_ACCURACY (0) or NOVAS_REDUCED_ACCURACY (1) | |
[out] | pos | Structure to populate with the calculated apparent GCRS position data for a fictitous geocentric observer. |
References NOVAS_GCRS, and place().
int place_j2000 | ( | double | jd_tt, |
const object *restrict | source, | ||
enum novas_accuracy | accuracy, | ||
sky_pos *restrict | pos ) |
reference_system: J2000
observer location: geocenter
position_type: apparent
Computes the J2000 dynamical position position of a source as 'seen' from the geocenter at the given time of observation. See place()
for more information.
The calculated positions and velocities include aberration corrections for the moving frame of the observer as well as gravitational deflection due to the Sun and Earth and other major gravitating bodies in the Solar system, provided planet positions are available via a novas_planet_provider function.
jd_tt | [day] Terrestrial Time (TT) based Julian date of observation. | |
source | Catalog source or solar_system body. | |
accuracy | NOVAS_FULL_ACCURACY (0) or NOVAS_REDUCED_ACCURACY (1) | |
[out] | pos | Structure to populate with the calculated apparent J2000 position data for a fictitous geocentric observer. |
References NOVAS_J2000, and place().
int place_mod | ( | double | jd_tt, |
const object *restrict | source, | ||
enum novas_accuracy | accuracy, | ||
sky_pos *restrict | pos ) |
reference_system: MOD
observer location: geocenter
position_type: apparent
Computes the Mean of Date (MOD) dynamical position position of a source as 'seen' from the geocenter at the given time of observation. See place()
for more information.
The calculated positions and velocities include aberration corrections for the moving frame of the observer as well as gravitational deflection due to the Sun and Earth and other major gravitating bodies in the Solar system, provided planet positions are available via a novas_planet_provider function.
jd_tt | [day] Terrestrial Time (TT) based Julian date of observation. | |
source | Catalog source or solar_system body. | |
accuracy | NOVAS_FULL_ACCURACY (0) or NOVAS_REDUCED_ACCURACY (1) | |
[out] | pos | Structure to populate with the calculated apparent Mean-of-Date (MOD) position data for a fictitous geocentric observer. |
int place_tod | ( | double | jd_tt, |
const object *restrict | source, | ||
enum novas_accuracy | accuracy, | ||
sky_pos *restrict | pos ) |
reference_system: TOD
observer location: geocenter
position_type: apparent
Computes the True of Date (TOD) dynamical position position of a source as 'seen' from the geocenter at the given time of observation. See place()
for more information.
The calculated positions and velocities include aberration corrections for the moving frame of the observer as well as gravitational deflection due to the Sun and Earth and other major gravitating bodies in the Solar system, provided planet positions are available via a novas_planet_provider function.
jd_tt | [day] Terrestrial Time (TT) based Julian date of observation. | |
source | Catalog source or solar_system body. | |
accuracy | NOVAS_FULL_ACCURACY (0) or NOVAS_REDUCED_ACCURACY (1) | |
[out] | pos | Structure to populate with the calculated apparent True-of-Date (TOD) position data for a fictitous geocentric observer. |
short virtual_planet | ( | double | jd_tt, |
const object *restrict | ss_body, | ||
enum novas_accuracy | accuracy, | ||
double *restrict | ra, | ||
double *restrict | dec, | ||
double *restrict | dis ) |
reference_system: ICRS / GCRS
observer location: geocenter
position_type: apparent
Computes the virtual place of a solar system body, as would be seen by an observer at the geocenter, referenced to the GCRS. This is the same as calling place_gcrs() for the body, except the different set of return values used.
The calculated positions and velocities include aberration corrections for the moving frame of the observer as well as gravitational deflection due to the Sun and Earth and other major gravitating bodies in the Solar system, provided planet positions are available via a novas_planet_provider function.
REFERENCES:
jd_tt | [day] Terretrial Time (TT) based Julian date. | |
ss_body | Pointer to structure containing the body designation for the solar system body. | |
accuracy | NOVAS_FULL_ACCURACY (0) or NOVAS_REDUCED_ACCURACY (1) | |
[out] | ra | [h] Virtual apparent right ascension for a fictitous geocentric observer, referred to the GCRS (it may be NULL if not required). |
[out] | dec | [deg] Virtual apparent declination, for a fictitous geocentric observer, referred to the GCRS (it may be NULL if not required). |
[out] | dis | [AU] Apparent distance from Earth to the body at 'jd_tt' (it may be NULL if not needed). |
References NOVAS_GCRS, and radec_planet().
short virtual_star | ( | double | jd_tt, |
const cat_entry *restrict | star, | ||
enum novas_accuracy | accuracy, | ||
double *restrict | ra, | ||
double *restrict | dec ) |
reference_system: ICRS / GCRS
observer location: geocenter
position_type: apparent
Computes the virtual place of a star, as would be seen by an observer at the geocenter, referenced to GCRS, at date 'jd_tt', given its catalog mean place, proper motion, parallax, and radial velocity.
Notwithstanding the different set of return values, this is the same as calling place_star() with a NULL observer location and NOVAS_GCRS as the system, or place_gcrs() for an object that specifies the star.
The calculated positions and velocities include aberration corrections for the moving frame of the observer as well as gravitational deflection due to the Sun and Earth and other major gravitating bodies in the Solar system, provided planet positions are available via a novas_planet_provider function.
REFERENCES:
jd_tt | [day] Terrestrial Time (TT) based Julian date. | |
star | Pointer to catalog entry structure containing catalog data for the object in the ICRS. | |
accuracy | NOVAS_FULL_ACCURACY (0) or NOVAS_REDUCED_ACCURACY (1) | |
[out] | ra | [h] Virtual apparent right ascension for a fictitous geocentric observer, referred to the GCRS (it may be NULL if not required). |
[out] | dec | [deg] Virtual apparent declination for a fictitous geocentric observer, referred to the GCRS (it may be NULL if not required). |
References NOVAS_GCRS, and radec_star().
|
extern |
Current set of gravitating bodies to use for deflection calculations in full accuracy mode.
Each bit signifies whether a given body is to be accounted for as a gravitating body that bends light, such as the bit (1 << NOVAS_JUPITER)
indicates whether or not Jupiter is considered as a deflecting body. You should also be sure that you provide ephemeris data for bodies that are designated for the deflection calculation.
|
extern |
Current set of gravitating bodies to use for deflection calculations in reduced accuracy mode.
Each bit signifies whether a given body is to be accounted for as a gravitating body that bends light, such as the bit (1 << NOVAS_JUPITER)
indicates whether or not Jupiter is considered as a deflecting body. You should also be sure that you provide ephemeris data for bodies that are designated for the deflection calculation.