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astro-ph.EP2026

Planet formation in chemically diverse and evolving discs II. Chemical fingerprints in planetary atmospheres

E. Pacetti, D. Turrini, E. Schisano +13

Giant planets form in protoplanetary discs, where the coupled dynamical and chemical evolution of gas and solids determines the composition of the material they accrete. We investi…

astro-ph.EP2026

Substructures in Planet-Forming Disks with the SKAO

Yinhao Wu, Jessica Speedie, Sebastián Pérez +33

Disks of gas and dust orbiting young stars are the arenas and material reservoirs for planet formation. Over the past decade, multiwavelength observations, from infrared to radio,…

astro-ph.EP2026

The Origins of Planets for ArieL (OPAL) Key Science Project: the end-to-end planet formation campaign for the ESA space mission Ariel

Danae Polychroni, Diego Turrini, Romolo Politi +7

The growing body of atmospheric observations of exoplanets from space and ground-based facilities showcases how the great diversity of the planetary population is not limited to th…

astro-ph.EP2025

Planet formation in chemically diverse and evolving discs -- I. Composition of planetary building blocks

E. Pacetti, E. Schisano, D. Turrini +12

Protoplanetary discs are dynamic environments where the interplay between chemical processes and mass transport shapes the composition of gas and dust available for planet formatio…

astro-ph.EP2025

On Linking Planet Formation Models, Protoplanetary Disk Properties, and Mature Gas Giant Exoplanet Atmospheres

Adina D. Feinstein, Richard A. Booth, Jennifer B. Bergner +34

Measuring a single elemental ratio (e.g., carbon-to-oxygen) provides insufficient information for understanding the formation mechanisms and evolution that affect our observations…

astro-ph.EP2025

Planetesimal formation via the streaming instability in simulations of infall dominated young disks

L. -A. Hühn, C. P. Dullemond, U. Lebreuilly +7

Protoplanetary disks naturally emerge during protostellar core-collapse. In their early evolutionary stages, infalling material dominates their dynamical evolution. In the context…