CustomBarycentricEcliptic¶
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class
astropy.coordinates.CustomBarycentricEcliptic(*args, copy=True, representation_type=None, differential_type=None, **kwargs)[source]¶ Bases:
astropy.coordinates.BaseEclipticFrameBarycentric ecliptic coordinates with custom obliquity. These origin of the coordinates are the barycenter of the solar system, with the x axis pointing in the direction of the mean (not true) equinox of J2000, and the xy-plane in the plane of the ecliptic tilted a custom obliquity angle.
The frame attributes are listed under Other Parameters.
Parameters: - data :
BaseRepresentationsubclass instance A representation object or
Noneto have no data (or use the coordinate component arguments, see below).- lon :
Angle, optional, must be keyword The ecliptic longitude for this object (
latmust also be given andrepresentationmust be None).- lat :
Angle, optional, must be keyword The ecliptic latitude for this object (
lonmust also be given andrepresentationmust be None).- distance :
Quantity, optional, must be keyword The distance for this object from the barycenter. (
representationmust be None).- pm_lon_coslat :
Angle, optional, must be keyword The proper motion in the ecliptic longitude (including the
cos(lat)factor) for this object (pm_latmust also be given).- pm_lat :
Angle, optional, must be keyword The proper motion in the ecliptic latitude for this object (
pm_lon_coslatmust also be given).- radial_velocity :
Quantity, optional, must be keyword The radial velocity of this object.
- representation_type :
BaseRepresentationsubclass, 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, zin most cases.- differential_type :
BaseDifferentialsubclass, 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 namesv_x, v_y, v_z.- copy : bool, optional
If
True(default), make copies of the input coordinate arrays. Can only be passed in as a keyword argument.
Attributes Summary
default_differentialdefault_representationframe_attributesframe_specific_representation_infonameobliquityAttributes Documentation
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default_differential¶
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default_representation¶
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frame_attributes= {'obliquity': <astropy.coordinates.attributes.QuantityAttribute object at 0x115295b38>}¶
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frame_specific_representation_info¶
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name= 'custombarycentricecliptic'¶
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obliquity= <Quantity 84381.448 arcsec>¶
- data :