arXiv (All)
open access
"Mega-Earths" are likely an artifact of stellar activity
Empirical relations and planet formation simulations suggest an upper mass limit for rocky planets of $\sim$10M$_{\oplus}$, as cores above this will almost certainly undergo runaway gas accretion. Nevertheless, a small number of planets appear to have densities consistent with rocky Earth-like compo
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
- Radiating Bondi Flows II: Giant Planet Accretion Models#1077873
- Effects of Outer Giant Planets on In Situ Formation of Inner Super-Earths#659039
- Effects of Outer Giant Planets on In Situ Formation of Inner Super-Earths#656903
- Beyond Pebble Isolation: Diverse Pathways to Giant Planet Formation Across Stellar and Orbital Scales#987135
- Probing Planet Formation within 10 au: Dust Substructures in Extremely Compact Protoplanetary Disks#1355317
Record · ID 1296607
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