We discuss our current understanding of the interior structure and thermal evolution of giant
planets. This includes the gas giants, such as Jupiter and Saturn, that are primarily …

The interiors of giant planets remain poorly understood. Even for the planets in the Solar
System, difficulties in observation lead to large uncertainties in the properties of planetary …

To aid in the physical interpretation of planetary radii constrained through observations of
transiting planets, or eventually direct detections, we compute model radii of pure hydrogen …

Aims. We examine the uncertainties in current planetary models and quantify their impact on
the planet cooling histories and mass-radius relationships. Methods. These uncertainties …

We present the dayside thermal emission spectrum of WASP-77Ab from 2.8 to 5.2 μm as
observed with the NIRSpec instrument on the James Webb Space Telescope (JWST) …

We investigate a population of transiting planets that receive relatively modest stellar
insolation, indicating equilibrium temperatures< 1000 K, and for which the heating …

Context. Recent studies suggest that in comparison to their host star, many giant exoplanets
are highly enriched with heavy elements and can contain several tens of Earth masses of …

Treatise on Geophysics, Second Edition, Eleven Volume Set is a comprehensive and in-
depth study of the physics of the Earth beyond what any geophysics text has provided …

We monitor the star HD 149026 and its Saturn-mass planet at 8.0 μm over slightly more than
half an orbit using the Infrared Array Camera on the Spitzer Space Telescope. We find an …

Giant planets acquire gas, ices and rocks during the early formation stages of planetary
systems and thus inform us on the formation process itself. Proceeding from inside out …