Self-consistent-field method for triaxial differentiated bodies in hydrostatic equilibrium
By: C. Staelen, J.-M. Huré
Published: 2026-03-13
View on arXiv →#astro-ph.EP
Abstract
This research proposes a new numerical code, BALEINES, to study the hydrostatic shape of triaxial differentiated bodies. This method improves the modeling of planetary interiors and is crucial for accurately determining the physical properties and evolution of celestial objects, including Earth and other planets, impacting planetary science missions.