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20182026
most citedForming Mercury by Giant Impacts

85 citations · 717 across the 35 of their papers we have counts for

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astro-ph.EP2026

Beyond Pebble Isolation: Diverse Pathways to Giant Planet Formation Across Stellar and Orbital Scales

Lorenzo Peerani, Sho Shibata, Ravit Helled

Context. Giant planet formation requires reaching crossover mass, i.e., when the mass of the gaseous envelope becomes equal to the mass of the core, within the disc's lifetime. The…

astro-ph.EP2026

The metallicity of giant exoplanets around low-mass stars and how Ariel can help

Ravit Helled, Sho Shibata, Shubham Kanodia +1

Giant planets orbiting low-mass stars represent a unique population of giant planets that can be studied to constrain planet formation theory. Surveys of transiting giant exoplanet…

astro-ph.EP2026

Composition gradients in sub-Neptunes: K2-18 b and TOI-270 d as case studies

Luca Morf, Ravit Helled

Structure models of sub-Neptunes commonly assume purely adiabatic interiors with distinct layers of homogeneous composition. We assess how allowing for more complex interiors with…

astro-ph.IM2026

The MegaWave Radio Surveyor

T. Joseph W. Lazio, Evgenya Shkolnik, James Aguirre +40

Several Decadal-level questions in astrophysics, exoplanets, astrobiology, and cosmology can be addressed only at low radio frequencies inaccessible from Earth. The MegaWave Radio…

astro-ph.EP2026

The atmospheric vertical structure of Uranus and Neptune from thermochemical models: the impact of model assumptions

Thomas Douçot, Ravit Helled, Daniel Kitzmann +2

The composition and temperature-pressure profile of the atmospheres of Uranus and Neptune are not well-determined. As observational data are limited, we often rely on chemical equi…

astro-ph.EP2026

Evolutionary tracks of giant planets formed by disk instability

Mirco Bussmann, Ravit Helled

The evolution of giant planets depends on their formation history. While several evolutionary models self-consistently link planet formation by core accretion to long-term evolutio…

astro-ph.EP2026

The influence of composition gradients on giant planet radii

Henrik Knierim, Ravit Helled

The radius of a giant planet is a key physical property. It encapsulates the outcome of its mass, composition, and thermal state, serving as a critical link between observations an…