Expressions for the Celestial Intermediate Pole and the Celestial Ephemeris Origin consistent with the IAU 2000A precession-nutation model

Nicole Capitaine (1, 2, 3) , Jean Chapront (1, 2, 3) , Sébastien Lambert (1, 2, 3) , Patrick Wallace

1 SYRTE - Systèmes de Référence Temps Espace
2 Rotation de la Terre et géodésie spatiale
3 Systèmes de référence célestes

Expressions for the position of the Celestial Intermediate Pole (CIP) and the Celestial Ephemeris Origin (CEO) in the Geocentric Celestial Reference System (GCRS) have been computed using the IAU 2000A precession-nutation. These expressions are for use in the new transformation between the GCRS and the International Terrestrial Reference System (ITRS) which is recommended by IAU Resolution B1.8. Various comparisons and numerical checks have been performed between the classical and the new transformations based on the IAU 2000A precession-nutation. These comparisons revealed necessary improvements to be applied to the classical form of the transformation in order to achieve the required level of accuracy. Once these improvements are applied, the consistency between the positions of the CIP in the GCRS corresponding to the classical and the new transformations is at a level of a few microarcseconds after one century. This work has demonstrated that the new method, in addition to providing an explicit separation between precession-nutation of the equator from Earth rotation, is more simple, compact and direct than the classical one, achieving accuracies at the level of a few microarcseconds with greatly reduced scope for accidental misuse. The resulting expressions for X, Y and s have been included in the IERS Conventions 2000. References for the numerical expressions are provided in Appendix C.

Domaines: Astrophysique [astro-ph]; Planète et Univers [physics]

Nicole Capitaine, Jean Chapront, Sébastien Lambert, Patrick Wallace. Expressions for the Celestial Intermediate Pole and the Celestial Ephemeris Origin consistent with the IAU 2000A precession-nutation model. Astronomy and Astrophysics - A&A, 2003, 400 (3), pp.1145-1154. ⟨10.1051/0004-6361:20030077⟩. ⟨hal-03801222⟩