EDP Sciences
Free Access
Volume 477, Number 1, January I 2008
Page(s) 315 - 327
Section Celestial mechanics and astrometry
DOI https://doi.org/10.1051/0004-6361:20066607
Published online 23 October 2007

A&A 477, 315-327 (2008)
DOI: 10.1051/0004-6361:20066607

INPOP06: a new numerical planetary ephemeris

A. Fienga1, 2, H. Manche1, J. Laskar1, and M. Gastineau1

1  Astronomie et Systèmes Dynamiques, IMCCE-CNRS UMR8028, 77 Av. Denfert-Rochereau, 75014 Paris, France
2  Observatoire de Besançon-CNRS UMR6213, 41bis Av. de l'Observatoire, 25000 Besançon, France
    e-mail: agnes@obs-besancon.fr

(Received 20 October 2006 / Accepted 17 September 2007)

INPOP06 is the new numerical planetary ephemeris developed at the IMCCE-Observatoire de Paris. INPOP (Intégrateur Numérique Planétaire de l'Observatoire de Paris) is a numerical integration of the motion of the nine planets and the Moon fitted to the most accurate available planetary observations. It also integrates the motion of 300 perturbing main belt asteroids, the rotation of the Earth and the Moon libration. We used more than 55 000 observations including the latest tracking data of the Mars Global Surveyor (MGS) and Mars Odyssey (Odyssey) missions. The accuracy obtained with INPOP06 is comparable to the accuracy of recent versions of the JPL DE ephemerides (DE414, Standish 2003, JPL IOM, 312N, 03; Konopliv et al. 2006, Icarus, 182, 23) and of the EPM ephemerides (EPM2004, Pitjeva 2005, Sol. Syst. Res., 39, 176).

Key words: celestial mechanics -- ephemerides -- astrometry

© ESO 2007

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.