The GCRF (Geocentric Celestial Reference Frame) frame of reference is an
Earth-centered inertial coordinate frame, where the origin is placed at the
center of mass of Earth and the coordinate frame is fixed with respect to the
stars (and therefore not fixed with respect to the Earth surface in its
rotation). The X-axis is aligned with the mean equinox of Earth at 12:00
Terrestrial Time on the 1st of January, 2000, and the Z-axis is aligned with
the Earth<U+00B4>s rotation axis.
It is equivalent to the J2000 frame of reference (also called EME2000), and in
some contexts it is also referred to as ICRF frame (although in its strict
definition, the origin of coordinates is placed at the barycenter of the Solar
System).
In the ECEF frame, the origin is also placed at the center of mass of Earth,
but the frame rotates with respect to the stars to remain fixed with respect to
the Earth surface as it rotates.
The coordinates and velocities input and calculated with the high-precision
orbital propagator (hpop) are in the GCRF frame of reference.
This function requires the asteRiskData
package, which can be installed
by running install.packages('asteRiskData', repos='https://rafael-ayala.github.io/drat/')