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- Rose-Marie Baland (Royal Observatory of Belgium, Belgium), The obliquity of Mercury: Models and interpretation
- Konstantin Batygin (Caltech, USA), Towards a Unified Model of Planet Formation
- Giulio BaĆ¹ (University of Pisa, Italy), Alternative state representations for orbit prediction
- Emeline Bolmont (University of Geneva, Switzerland), A journey from planets to stars: improving tidal models in orbital evolution codes
- Alexandre Correia (University of Coimbra, Portugal), New methods to study the tidal evolution of planetary systems
- Jean-Baptiste Delisle (University of Geneva, Switzerland), Planetary systems in resonant chains
- Caroline Dorn (University of Zurich, Switzerland), Planet cores store majority of planetary water budgets
- Daniel Fabrycky (University of Chicago, USA), Resonant Chain Dynamics: Interpretation of Observations
- Catalin Gales (Alexandru Ioan Cuza University, Iasi, Romania), Dynamics modelling and stability analysis of satellites orbiting oblate bodies
- Mikael Granvik (University of Helsinki, Finland), Destruction mechanisms for near-Earth objects
- Man Hoi Lee (University of Hong-Kong, Hong-Kong), Dynamics of Circumstellar Planets in Binary Star Systems
- Anders Johansen (University of Copenhagen, Danemark), Forming planetary systems via pebble accretion
- Dong Lai (Cornell University, Ithaca, USA), Hot Jupiters and Super-Earths: Spin-Orbit Puzzles in Exoplanetary Systems
- Alessandro Morbidelli (OCA, Nice, France), Interdisciplinarity: an effective approach to comprehending the formation of planetary systems
- Antoine Petit (OCA, Nice, France), Long-term stability of compact planetary systems
- Cristobal Petrovich (Pontificia Universidad Catolica de Chile, Chile), Long-term evolution of exoplanet systems
- Nicolas Rambaux (IMCCE, Paris, France), Lunar reference system from science to MoonLight and LunaNet
- Aaron Rosengren (University of California, San Diego, USA), On the Multiscale Astrodynamics of Cislunar xGEO Space
- Daniel J. Scheeres (University of Colorado, USA), Binary Asteroids: A Pathway to Understanding the Morphological Evolution of Rubble Pile Asteroids