Image de couverture de livre

The mass-radius relation of exoplanets, revisited

Fuente: arXiv

Enregistré dans:

Détails bibliographiques
Auteurs principaux:	Müller, Simon, Baron, Jana, Helled, Ravit, Bouchy, François, Parc, Léna
Format:	Preprint
Publié:	2023
Sujets:	Earth and Planetary Astrophysics
Accès en ligne:	Acceder al recurso
Tags:	Ajouter un tag Pas de tags, Soyez le premier à ajouter un tag!

Documents similaires

From super-Earths to sub-Neptunes: Observational constraints and connections to theoretical models
par: Parc, Léna, et autres
Publié: (2024)

Deep radiative zones affect the planetary cooling and internal structure: implications for exoplanet characterisation
par: Müller, Simon, et autres
Publié: (2026)

Giant exoplanet composition: Why do the hydrogen-helium equation of state and interior structure matter?
par: Howard, Saburo, et autres
Publié: (2024)

Origin and characterization of super-Earths and sub-Neptunes
par: Parc, Léna, et autres
Publié: (2026)

Unraveling the origin of giant exoplanets: Observational implications of convective mixing
par: Knierim, Henrik, et autres
Publié: (2025)

Can Jupiter's atmospheric metallicity be different from the deep interior?
par: Müller, Simon, et autres
Publié: (2024)

The bulk metallicity of giant planets around M stars
par: Müller, Simon, et autres
Publié: (2024)

Resizing the giants: How modelling adiabatic interiors impacts predicted planetary radii
par: Müller, Simon, et autres
Publié: (2026)

Ice Giants
par: Helled, Ravit
Publié: (2025)

Outstanding Questions in Giant Planet Theory
par: Helled, Ravit
Publié: (2026)

Giant planet formation via pebble accretion across different stellar masses
par: Shibata, Sho, et autres
Publié: (2025)

The interior of Uranus: Thermal profile, bulk composition and the distribution of rock, water and hydrogen and helium
par: Morf, Luca, et autres
Publié: (2024)

Evolution of Jupiter and Saturn with helium rain
par: Howard, Saburo, et autres
Publié: (2024)

Uranus' Complex Internal Structure
par: Neuenschwander, Benno A., et autres
Publié: (2024)

Icy or rocky? Convective or stable? New interior models of Uranus and Neptune
par: Morf, Luca, et autres
Publié: (2025)

Convective Mixing in Gas Giant Planets with Primordial Composition Gradients
par: Knierim, Henrik, et autres
Publié: (2024)

Giant planet interiors and atmospheres
par: Helled, Ravit, et autres
Publié: (2024)

The Evolution and Internal Structure of Neptunes and Sub-Neptunes: The importance of thermal conductivity in non-convective regions
par: Eberlein, Mark, et autres
Publié: (2025)

The fuzzy cores of Jupiter and Saturn
par: Helled, Ravit, et autres
Publié: (2024)

Giant Planet Evolution with MESA
par: Helled, Ravit, et autres
Publié: (2025)

How Internal Structure Shapes the Metallicity of Giant Exoplanets
par: Peerani, Lorenzo, et autres
Publié: (2025)

Disk and atmosphere composition of multi-planet systems
par: Eberlein, Mark, et autres
Publié: (2024)

Mind the Companion : Demographics of Transiting S-type Exoplanets
par: Messamah, Lina Y., et autres
Publié: (2026)

On the origin of Jupiter's fuzzy core: constraints from N-body, impact and evolution simulations
par: Meier, Thomas, et autres
Publié: (2025)

Accretion of primordial H-He atmospheres in mini-Neptunes: the importance of envelope enrichment
par: Lous, Marit Mol, et autres
Publié: (2024)

The Possibility of Hydrogen-Water Demixing in Uranus, Neptune, K2-18b and TOI-270d
par: Howard, Saburo, et autres
Publié: (2025)

The linear-mixing approximation in silica-water mixtures at planetary conditions
par: Darafeyeu, Valiantsin, et autres
Publié: (2024)

Towards an agnostic algorithm for sampling empirical structure models: The case of Uranus and Neptune
par: Wirth, Stefano, et autres
Publié: (2025)

Earth as an Exoplanet. III. Using Empirical Thermal Emission Spectra as an Input for Atmospheric Retrieval of an Earth-twin Exoplanet
par: Mettler, Jean-Noël, et autres
Publié: (2023)

The Outcome of Collisions between Gaseous Clumps formed by Disk Instability
par: Matzkevich, Yoav, et autres
Publié: (2024)

Beyond the mass-radius plane: Integrated radiative-convective and interior structure simulations of the exoplanet continuum
par: Nicholls, Harrison, et autres
Publié: (2026)

Further constraints on Jupiter's primordial structure
par: Knierim, Henrik, et autres
Publié: (2025)

Recent development in high-precision high-fidelity spectrographs for exoplanet research and characterization
par: Bouchy, François, et autres
Publié: (2026)

Recent advances in modelling of global-scale collisions using smoothed particle hydrodynamics
par: Reinhardt, Christian, et autres
Publié: (2026)

Giant Planet Formation by Disk Instability
par: Helled, Ravit, et autres
Publié: (2026)

The possibility of a giant impact on Venus
par: Bussmann, Mirco, et autres
Publié: (2025)

Studying the variability of the He triplet to understand the detection limits of evaporating exoplanet atmospheres
par: Mercier, Samson J., et autres
Publié: (2025)

On the road to the radius valley: distinguishing between gas dwarfs and water worlds with young transiting exoplanets
par: Rogers, James G.
Publié: (2025)

Fate of a remnant solid disk around an eccentric giant planet
par: Shibata, S., et autres
Publié: (2024)

Can radio occultations constrain Uranus or Neptune's internal rotation periods?
par: Mankovich, Christopher R., et autres
Publié: (2026)