Report of the International Astronomical Union Division I Working Group on Precession and the Ecliptic - Archive ouverte HAL
Article Dans Une Revue Celestial Mechanics and Dynamical Astronomy Année : 2006

Report of the International Astronomical Union Division I Working Group on Precession and the Ecliptic

Résumé

The IAU Working Group on Precession and the Equinox looked at several solutions for replacing the precession part of the IAU 2000A precession nutation model, which is not consistent with dynamical theory. These comparisons show that the (Capitaine et al., Astron. Astrophys., 412, 2003a) precession theory, P03, is both consistent with dynamical theory and the solution most compatible with the IAU 2000A nutation model. Thus, the working group recommends the adoption of the P03 precession theory for use with the IAU 2000A nutation. The two greatest sources of uncertainty in the precession theory are the rate of change of the Earth's dynamical flattening, DeltaJ 2, and the precession rates (i.e. the constants of integration used in deriving the precession). The combined uncertainties limit the accuracy in the precession theory to approximately 2 mas cent-2.

Dates et versions

hal-03742144 , version 1 (02-08-2022)

Identifiants

Citer

James L. Hilton, Nicole Capitaine, Jean Chapront, Jose M. Ferrandiz, Agnès Fienga, et al.. Report of the International Astronomical Union Division I Working Group on Precession and the Ecliptic. Celestial Mechanics and Dynamical Astronomy, 2006, 94, pp.351-367. ⟨10.1007/s10569-006-0001-2⟩. ⟨hal-03742144⟩
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