INPOP06: a new numerical planetary ephemeris

By Jacques Laskar, A. Fienga, H. Manche, Mickaël Gastineau. 2008

186 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Oceanography

View Paper: https://www.semanticscholar.org/paper/8cd110f45641e659f1d44c386cd54e99da8c3c19

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Citations in the corpus

INPOP08, a 4-D planetary ephemeris: from asteroid and time-scale computations to ESA Mars Express and Venus Express contributions (2009, methodology): “Such ephemerides as INPOP06, but also DE405, were only fitted to direct radar observations of the Venus surface (see Standish 1998b; Fienga et al. 2008) and to the VLBI data deduced from the tracking of the Venus mission Magellan in 1994.”
Density of asteroids (2012, background): “…Sun and the planets, the gravitational inﬂuence of several asteroids must be taken into account to properly describe the observed position of planets, satellites, and spacecrafts (see, Baer and Chesley, 2008; Baer et al., 2011; Fienga et al., 2008, 2009, 2010; Folkner et al., 2009, for details).”
La2010: a new orbital solution for the long-term motion of the Earth (2011, methodology): “We no longer average over the orbital motion of the planets, which allows a precise computation of the evolution of the Earth spin axis that can be compared to the most precise model adopted by the IAU (Soffel et al. 2003) (see Fienga et al. 2008).”
Phenomenology of the Lense-Thirring effect in the solar system (2010, background): “Third line: nominal values of the perihelion precessions due to the Sun’s oblateness for J 2 = 2×10 (Pireaux and Rozelot 2003; Pitjeva 2005a); the current level of uncertainty in it is about 10% (Fienga et al. 2008).”
Time scale controversy: Accurate orbital calibration of the early Paleogene (2012, methodology): “…the long-term ephemerides, the group of the Institut de Mécanique Céleste et de Calcul des Éphémérides (IMCCE) at Paris Observatory developed a new high precision planetary ephemeris called INPOP [Fienga et al., 2008, 2009, 2011] (Intégration Numérique Planétaire de l’Observatoire de Paris).”
Strong chaos induced by close encounters with Ceres and Vesta (2011, unknown): “These asteroids1 induce some perturbations of several km on the position of Mars (e.g., Kuchynka et al. 2010), and have long been taken into account in the elaboration of high-precision planetary ephemerides (Standish 1998; Fienga et al. 2008, 2009), valid over a few kyr.”