Planetary science & exoplanets
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- TESS Pulsation Timing Reveals the JWST Calibration Star HD 158485 as a Double-pulsator Binary
- Towards a coupled activity-fallback model for comets I) 67P/Churyumov-Gerasimenko's water activity from a microphysics model with dynamic dust-depth
- Hydrogen Engulfment into Sub-Neptune Cores through Magma Ocean Convective Surface Renewal
- Assessing PLATO's Discovery Potential across Different Observing Strategies
- How long could volcanic plumes persist in the Venus atmosphere?
- The Hydrological Cycle and Circulation of Tidally-Locked Planets with a Finite Moisture Inventory
- Combination of multi-observatory photometry to determine asteroid rotation periods
- Detailed study of HD 219134: a benchmark K-dwarf with a compact planetary system
- Star Cluster Ecology VIII. -- Dynamically Forming S-Type and αCentauri-like Systems
- The Neptunian Final Parsec Problem: How Inertial Waves Enable Neptunes and Gas Giants to Survive Tidal Migration
- The GAPS Programme at TNG. LXXX. Characterisation of the 400 Myr old multi-planet system K2-233
- Glycine Partitions into Halite during Crystallization in Ceres Simulant Brines
- Radar Observations of Europa in 2011–2024: New Insights into Radar Scattering Properties
- Oxygen Ion Irradiation of Tholins: Implications for the Incorporation of Oxygen into Aerosols in Titan’s Atmosphere
- The Highly Unusual Behavior and Chemical Composition of Interstellar Comet 2I/Borisov
- Spectral Evolution of Ceres’ Surface and Implications for Space Weathering
- Radar Identification and Geomorphic Characterization of Distal Tycho Secondary Craters
- JWST Reveals the Kuiper Belt–like Compositions of the Uranian Rings and Small Moons
- A scaling law for stagnant-lid convection with composite visco-elasto-plastic rheology: application to Europa's ice shell
- The GAPS programme at TNG LXXXII. The first atmospheric investigation of the gas giant WASP-13b at high resolution with GIARPS
- Dust-driven vertical shear instability in an isothermal shearing box: I. Turbulence and gas dynamics without dust feedback
- The Fast & Fourier: Using neural operators to speed up radiative modeling of protoplanetary disks
- "Mega-Earths" are likely an artifact of stellar activity
- The accretionally heated atmospheres of protoplanets and brown dwarfs
- Longitudinal distribution of Io's dayside atmospheric density