activity
20092025
most citedLa2010: A new orbital solution for the long term motion of the Earth

1k citations · 1.6k across the 15 of their papers we have counts for

collaborators

16 papers

astro-ph.EP2025

Boosting decision trees for Main Belt Asteroid selection in planetary ephemerides: an alternative model

Vincenzo Mariani, Agnès Fienga, Zachary Murray +2

One of the main bottleneck in assessing the accuracy of Mars orbit is the unknown value of the asteroids in the Main Asteroid Belt. Nowadays a modeling with 343 asteroids as point…

astro-ph.EP2023

Can one hear supercontinents in the tides of ocean planets?

Pierre Auclair-Desrotour, Mohammad Farhat, Gwenaël Boué +2

Recent observations and theoretical progress made about the history of the Earth-Moon system suggest that tidal dissipation in oceans primarily drives the long term evolution of or…

astro-ph.EP2023

Bayesian test of Brans-Dicke theories with planetary ephemerides: Investigating the strong equivalence principle

Vincenzo Mariani, Olivier Minazzoli, Agnès Fienga +2

Context: We are testing the Brans-Dicke class of scalar tensor theories with planetary ephemerides. Aims: In this work, we apply our recently proposed Bayesian methodology to the B…

astro-ph.EP2019★ 10 cited

High order regularised symplectic integrator for collisional planetary systems

Antoine C. Petit, Jacques Laskar, Gwenaël Boué +1

We present a new mixed variable symplectic (MVS) integrator for planetary systems, that fully resolve close encounters. The method is based on a time regularisation that allows kee…

astro-ph.EP2018★ 9 cited

Long-term orbital and rotational motions of Ceres and Vesta

T. Vaillant, J. Laskar, N. Rambaux +1

Context. The dwarf planet Ceres and the asteroid Vesta have been studied by the Dawn space mission. They are the two heaviest bodies of the main asteroid belt and have different ch…

gr-qc2017★ 92 cited

The new lunar ephemeris INPOP17a and its application to fundamental physics

V. Viswanathan, A. Fienga, O. Minazzoli +3

We present here the new INPOP lunar ephemeris, INPOP17a. This ephemeris is obtained through the numerical integration of the equations of motion and of rotation of the Moon, fitted…