arXiv (All)
open access
Hybrid worlds are the commonest outcome among the M-dwarf sub-Neptunes characterised with JWST
The sub-Neptunes orbiting M dwarfs are usually assigned to one of two classes: rocky cores beneath primordial hydrogen, or volatile-rich bodies formed beyond the water-ice line. Bulk density cannot distinguish them, the two being degenerate in mass and radius once envelope evolution is modelled self
Conceptio Open Archive
Analyze & explore related research in Conceptio
Connect this record directly into your research workflow or AI agent. Explore citations across open repositories, query full text, and export structured proof bundles.
This document is indexed with metadata only: full text is not available in the archive for this record. Open the official source ↗
Related documents
- Structure, Phase Stability, and Transport in Hydrogen-Bearing Magma Oceans#996290
- Composition gradients in sub-Neptunes: K2-18 b and TOI-270 d as case studies#927614
- Ice Giants Revisited: Uranus and Neptune as Magma Ocean Worlds#971825
- Radiating Bondi Flows II: Giant Planet Accretion Models#1077873
- Most Rocky Sub-Neptunes are Molten: Mapping the Solidification Shoreline for Gas Dwarf Exoplanets#629880
Record · ID 1128897
Retrieved via Conceptio: every document is proof-bundled with source, license, and retrieval metadata.
Retrieved via Conceptio: every document is proof-bundled with source, license, and retrieval metadata.
Bring this data into your agent: Connect via MCP or API · 20 free credits to start · no card required
Read the Docs → · View CLI source on GitHub · Conceptio Open Knowledge Archive
Read the Docs → · View CLI source on GitHub · Conceptio Open Knowledge Archive