HCRS#

class astropy.coordinates.HCRS(*args, copy=True, representation_type=None, differential_type=None, **kwargs)[source]#

Bases: BaseRADecFrame

A coordinate or frame in a Heliocentric system, with axes aligned to ICRS.

The ICRS has an origin at the Barycenter and axes which are fixed with respect to space.

This coordinate system is distinct from ICRS mainly in that it is relative to the Sun’s center-of-mass rather than the solar system Barycenter. In principle, therefore, this frame should include the effects of aberration (unlike ICRS), but this is not done, since they are very small, of the order of 8 milli-arcseconds.

For more background on the ICRS and related coordinate transformations, see the references provided in the See Also section of the documentation.

The frame attributes are listed under Other Parameters.

Parameters:

dataBaseRepresentation subclass instance: A representation object or None to have no data (or use the coordinate component arguments, see below).
raAngle, optional, keyword-only: The RA for this object (dec must also be given and representation must be None).
decAngle, optional, keyword-only: The Declination for this object (ra must also be given and representation must be None).
distanceQuantity [:ref: ‘length’], optional, keyword-only: The Distance for this object along the line-of-sight. (representation must be None).
pm_ra_cosdecQuantity [:ref: ‘angular speed’], optional, keyword-only: The proper motion in Right Ascension (including the cos(dec) factor) for this object (pm_dec must also be given).
pm_decQuantity [:ref: ‘angular speed’], optional, keyword-only: The proper motion in Declination for this object (pm_ra_cosdec must also be given).
radial_velocityQuantity [:ref: ‘speed’], optional, keyword-only: The radial velocity of this object.
representation_typeBaseRepresentation subclass, str, optional: A representation class or string name of a representation class. This sets the expected input representation class, thereby changing the expected keyword arguments for the data passed in. For example, passing representation_type='cartesian' will make the classes expect position data with cartesian names, i.e. x, y, z in most cases unless overridden via frame_specific_representation_info. To see this frame’s names, check out <this frame>().representation_info.
differential_typeBaseDifferential subclass, str, dict, optional: A differential class or dictionary of differential classes (currently only a velocity differential with key ‘s’ is supported). This sets the expected input differential class, thereby changing the expected keyword arguments of the data passed in. For example, passing differential_type='cartesian' will make the classes expect velocity data with the argument names v_x, v_y, v_z unless overridden via frame_specific_representation_info. To see this frame’s names, check out <this frame>().representation_info.
copybool, optional: If True (default), make copies of the input coordinate arrays. Can only be passed in as a keyword argument.

Other Parameters:

obstimeTime: The time at which the observation is taken. Used for determining the position of the Sun.

Attributes Summary

`default_differential`	Default representation for differential data (e.g., velocity)
`default_representation`	Default representation for position data
`frame_attributes`
`frame_specific_representation_info`	Mapping for frame-specific component names
`name`
`obstime`

Attributes Documentation

default_differential#: Default representation for differential data (e.g., velocity)

default_representation#: Default representation for position data

frame_attributes = {'obstime': <astropy.coordinates.attributes.TimeAttribute object>}#

frame_specific_representation_info#: Mapping for frame-specific component names

name = 'hcrs'#

obstime = <Time object: scale='tt' format='jyear_str' value=J2000.000>#