Bases: astropy.coordinates.BaseCoordinateFrame
A coordinate or frame in the Geocentric Celestial Reference System (GCRS).
GCRS is distinct form ICRS mainly in that it is relative to the Earth’s center-of-mass rather than the solar system Barycenter. That means this frame includes the effects of abberation (unlike ICRS). For more background on the GCRS, see the references provided in the See Also section of the documentation. (Of particular note is Section 1.2 of USNO Circular 179)
This frame also includes frames that are defined relative to the Earth, but that are offset (in both position and velocity) from the Earth.
This frame has three frame attributes:
The time at which the observation is taken. Used for determining the position of the Earth.
3-vector giving the position of the observer relative to the center-of-mass of the Earth, oriented the same as BCRS/ICRS. Defaults to 0, meaning “true” GCRS.
3-vector giving the celocity of the observer relative to the center-of-mass of the Earth, oriented the same as BCRS/ICRS. Defaults to 0, meaning “true” GCRS.
Parameters: | representation : BaseRepresentation or None
ra : Angle, optional, must be keyword
dec : Angle, optional, must be keyword
distance : Quantity, optional, must be keyword
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Attributes Summary
default_representation | |
frame_specific_representation_info | |
name | |
obsgeoloc | |
obsgeovel | |
obstime |
Attributes Documentation