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Planetary systems with several planets in compact orbital configurations suchas TRAPPIST-1 are surely affected by tidal effects. Its study provides us withimportant insight about its evolution. We developed a second generation of aN-body code based on the tidal model used in Mercury-T, re-implementing andimproving its functionalities using Rust as programming language (including aPython interface for easy use) and the WHFAST integrator. The new open sourcecode ensures memory safety, reproducibility of numerical N-body experiments, itimproves the spin integration compared to Mercury-T and allows to take intoaccount a new prescription for the dissipation of tidal inertial waves in theconvective envelope of stars. Posidonius is also suitable for binary systemsimulations with evolving stars.

Studying tidal effects in planetary systems with Posidonius. A N-body simulator written in Rust