HAL (France)
open access
Interior models suggest the presence of carbon inside Io and Europa
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
- Subduction-like process in Europa’s ice shell triggered by enhanced eccentricity periods#246919
- Impact of accretion variability on the CO emission of a disk around a very-low-mass star with JWST#1050509
- Long-term enhancing of Jupiter’s electrostatic waves as diagnostic of Io’s mass loading activity#322461
- The effect of the atmospheric C/O ratio on interiors of hot Jupiters#975329
- Inside the Eirenesphere: The Interplay of Porosity, Heat Flux and Mineralogy in Exoplanetary Aquable and Habitable Layers#1051773
Record · ID 482694
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