The majority of hot Jupiters formed beyond the water ice line
Yaxing He, Bertram Bitsch, Adrien Houge, Joe Williams, Masahiro Ogihara
astro-ph.EP
Submitted: 2026-07-16
Comments: 8 pages, 5 figures, 2 tables. Accepted for publication in A&A Letters
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Related papers
- PDS 70 c and SR 12 c: Observational Constraints on Giant-Planet and Satellite Formation
- Two-stage disruption of resonant chains
- Detectability of resolved hydrogen lines from the accretion shock at gas giants and their CPDs
- Binary-lens Microlensing Degeneracy: Impact on Planetary Sensitivity and Mass-ratio Function
- Atmospheric escape fractionates secondary but not primary atmospheres
- The Occurrence Rate of Nearby Planetary Companions to Hot Jupiters