# The INPOP10a planetary ephemeris and its applications in fundamental physics

@article{Fienga2011TheIP,
title={The INPOP10a planetary ephemeris and its applications in fundamental physics},
author={A. Fienga and Jacques Laskar and Petr Kuchynka and Herve Manche and Gregory Desvignes and Micka{\"e}l Gastineau and Ismael Cognard and Gilles Theureau},
journal={Celestial Mechanics and Dynamical Astronomy},
year={2011},
volume={111},
pages={363-385}
}
• Published 29 August 2011
• Physics
• Celestial Mechanics and Dynamical Astronomy
Compared to the previous INPOP versions, the INPOP10a planetary and lunar ephemeris has several improvements. For the planets of our Solar System, no big change was brought in the dynamics but improvements were implemented in the fitting process, the data sets used in the fit and in the selection of fitted parameters. We report here the main characteristics of the planetary part of INPOP10a like the fit of the product of the solar mass with the gravitational constant ($${{\rm GM}_{\odot… 101 Citations Gaia-DR2 asteroid observations and INPOP planetary ephemerides • Physics, Geology • 2022 We used the INPOP19a planetary ephemerides to perform the orbital adjustment of 14099 asteroids based on Gaia-DR2 observations, and compare for 23 of them the resulting orbits to radar data. As Development of planetary ephemerides EPM and their applications • Physics, Geology • 2014 This paper outlines the progress in development of the numerical planet ephemerides EPM—Ephemerides of Planets and the Moon. EPM was first created in the 1970s in support of Russian space flight Astrometric observations of Phobos and Deimos during the 1971 opposition of Mars • Physics • 2014 Abstract : Context. Accurate positional measurements of planets and satellites are used to improve our knowledge of their dynamics and to infer the accuracy of planet and satellite ephemerides. Aims. Numerical estimation of the sensitivity of INPOP planetary ephemerides to general relativity parameters • Physics • 2015 In this paper, are given numerical estimations of the sensitivity of the latest version of the INPOP planetary ephemerides (INPOP13c) to GR parameters: the PPN parameters$$\beta $$β,$$\gamma γ,
Relativistic effects and dark matter in the Solar system from observations of planets and spacecraft
• Physics, Geology
• 2013
The high precision of the latest version of the planetary ephemeris EPM2011 enables one to explore more accurately a variety of small effects in the solar system. The processing of about 678 thousand
Constraints on the location of a possible 9th planet derived from the Cassini data
• Geology, Physics
• 2016
To explain the unusual distribution of Kuiper belt objects, several authors have advocated the existence of a super-Earth planet in the outer solar system. It has recently been proposed that a 10 M⊕
Constraining the Angular Momentum of the Sun with Planetary Orbital Motions and General Relativity
The angular momentum of a star is an important astrophysical quantity related to its internal structure, formation, and evolution. Helioseismology yields \$S_{\odot}= 1.92\times10^{41}\ \mathrm{kg\
Observations of the Galilean satellites of Jupiter with Pulkovo Normal Astrograph during 2009–2011
The paper presents the results of observations of Jupiter and its Galilean moons, performed with the Normal Astrograph (D/F=0.33 m/3.5 m, CCD S2C, FOV 18′ × 16′) at Pulkovo observatory during
Current problems of dynamics of moons of planets and binary asteroids based on observations
The general approach to studying the dynamics of moons of planets and asteroids consists in developing more and more accurate models of motion based on observational data. Not only the necessary

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