activity
20082019
most citedA pre-Caloris synchronous rotation for Mercury

66 citations · 298 across the 9 of their papers we have counts for

collaborators

9 papers

astro-ph.IM2019★ 8 cited

ESA Voyage 2050 white paper -- Faint objects in motion: the new frontier of high precision astrometry

F. Malbet, U. Abbas, J. Alves +28

Sky survey telescopes and powerful targeted telescopes play complementary roles in astronomy. In order to investigate the nature and characteristics of the motions of very faint ob…

astro-ph.EP2018★ 34 cited

Detectability of shape deformation in short-period exoplanets

B. Akinsanmi, S. C. C. Barros, N. C. Santos +4

Short-period planets suffer from extreme tidal forces from their parent stars causing them to deform and attain non-spherical shapes. The planet shapes, modeled here as triaxial el…

astro-ph.EP2016★ 8 cited

Coupled orbital and spin evolution of the CoRoT-7 two-planet system using a Maxwell viscoelastic rheology

Adrián Rodríguez Colucci, Nelson Callegari, Alexandre Correia

We investigate the orbital and rotational evolution of the CoRoT-7 two-planet system, assuming that the innermost planet behaves like a Maxwell body. We numerically resolve the cou…

astro-ph.EP2013★ 63 cited

On the equilibrium figure of close-in planets and satellites

Alexandre C. M. Correia, Adrian Rodriguez

Many exoplanets have been observed close to their parent stars with orbital periods of a few days. As for the major satellites of the Jovian planets, the figure of these planets is…

astro-ph.EP2013★ 19 cited

Tidal damping of the mutual inclination in hierachical systems

A. C. M. Correia, G. Boue, J. Laskar +1

Hierarchical two-planet systems, in which the inner body's semi-major axis is between 0.1 and 0.5 AU, usually present high eccentricity values, at least for one of the orbits. As a…

astro-ph.EP2012★ 62 cited

Dissipation in planar resonant planetary systems

J. -B. Delisle, J. Laskar, A. C. M. Correia +1

Close-in planetary systems detected by the Kepler mission present an excess of periods ratio that are just slightly larger than some low order resonant values. This feature occurs…