The Science Potential of Characterizing Gas Giant Exoplanets with HWO
astro-ph.EP, astro-ph.IM
Submitted: 2026-09-18
Updated: 2026-09-18
Comments: 80 pages, 12 figures, accepted to Journal of Astronomical Telescopes, Instruments, and Systems "Habitable Worlds Observatory Pre-Formulation Science, Architecture Concepts, and Technology Maturation"
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