arXiv (All)
open access
A Formation-Stage Bottleneck for Exomoons around Close-in Rocky Planets
Massive moons around rocky exoplanets are expected outcomes of giant impacts, yet no exomoon has been securely confirmed. We address this problem using meshless finite-mass simulations of giant impacts between differentiated rocky planets that include stellar tidal and Coriolis forces in a local co-
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
- The EBLM project - XX. Absolute dynamical masses of five low-mass eclipsing binaries, and an evaluation of mass estimation methods#1343852
- The thermal emission of the young and massive planet CoRoT-2b at 4.5 and 8 µm#356970
- Mobility Challenges and Possible Solutions for Low-gravity Planetary Body Exploration#291266
- Increased maximum carbon release offsets half of the growth trend in annual land carbon sink#1218669
- Giant impacts preferentially remove low-mass atmospheres: a generalised scaling law for impact-driven atmospheric loss#1202496
Record · ID 1412862
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