Hey Guys
What are the main diffences between ICRS (International Celestial Reference System) and the ITRS (International Terrestrial Reference System)
Regards
MAt
Hey Guys
What are the main diffences between ICRS (International Celestial Reference System) and the ITRS (International Terrestrial Reference System)
Regards
MAt
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Ty Olinghouse is definitely the guy to get deep with on this subject.. Ā He wrote a book once called "Redneck's Guide to Celestial Observation".. Ā just run a search on the network and you'll find him...just thought I'd put that out there...
The ITRS definition fulfills the following conditions:
See theĀ IERS Conventions (2010), especiallyĀ Ā Chapter 4Ā (pdf/661 KB), for a detailed description of the ITRS.
The ITRS is realized by estimates of theĀ coordinates and velocitiesĀ of a set of stations observed by VLBI, LLR, GPS, SLR, and DORIS. Its name is International Terrestrial Reference Frame (ITRF).
General documentation on terrestrial reference systems and frames is available at theĀ ITRS CentreĀ of the IERS.
The ITRS can be connected to theĀ International Celestial Reference SystemĀ (ICRS) by use of the IERSĀ Earth Orientation ParametersĀ (EOP).
Text provided by the former Central Bureau, modified.
The International Celestial Reference System (ICRS)
At its 23rd General Assembly in August 1997, the International Astronomical Union (IAU) decided that,Ā as from 1 January 1998, the IAU celestialĀ reference system shall be the International Celestial Reference System (ICRS), in replacement of the FK5 (Fricke et al. 1988).Ā
The consequences of this new situation for accuracy needs more stringent than 0.05" are summarized by Feissel and Mignard (1997).
By Reference System it is meant the set of prescriptions and conventions together with the modeling required to define at any time a triad of axes.
The ICRS is accessible by means of coordinates of reference extragalactic radio sources, theĀ International Celestial Reference FrameĀ (ICRF).
The ICRS complies with the conditions specified by theĀ 1991 IAU Recommendations. ItsĀ originĀ is located at the barycenter of the solar system through appropriate modelling ofĀ VLBIĀ observations in the framework of General Relativity. ItsĀ poleĀ is in the direction defined by the conventional IAU models for precession (Lieske et al., 1977) and nutation (Seidelmann, 1982). ItsĀ origin of right ascensionsĀ was implicitly defined by fixingĀ
the right ascension of 3C 273B to the Hazard et al. (1971) FK5 value transferred at J2000.0. See Arias et al. (1995) for more details.
TheĀ HipparcosĀ star positions and proper motions and theĀ JPL Solar System ephemeridesĀ are expressed in the ICRS.
The directions of the ICRSĀ pole and right ascensions originĀ are maintained fixed relative to the quasars within +/- 20 microarcseconds.Ā
Thanks to the fact that the Hipparcos catalogue includes all the FK5 stars, the location of the FK5 pole and right ascensions origin is known withĀ
an uncertainty of a few mas (Mignard and FroeschlĆ© 1997). Using a state of the art precession-nutation model, the analysis of long VLBI seriesĀ
of the observed motion of the celestial pole allows to derive the coordinates of the mean pole at J2000.0 in the ICRS: 17.3 +/- 0.2 mas in the direction 12 h and 5.1 +/- 0.2 mas in the direction 18 h.(IERS 1997). Comparing VLBI and LLR earth orientation and terrestrial reference frames, Folkner et al. (1994) estimated the frame tie between the IERS celestial system and the JPL planetary ephemeris, and concluded that the mean equinox of J2000.0 is shifted from the ICRS right ascension origin by 78 +/- 10 mas (direct rotation around the polar axis).
The ICRS is realized by VLBI estimates of equatorial coordinates of a set of extragalactic compact radio sources, theInternational CelestialĀ Reference FrameĀ (ICRF).
The ICRS can be connected to theĀ International Terrestrial Reference SystemĀ (ITRS) by use of theĀ IERS Earth Orientation ParametersĀ (EOP).