Discovery of an Inflated Hot Neptune and Its Formation from Jovian Mass Loss
Grant C. Weldon, Samuel W. Yee, Bradley M. S. Hansen, Smadar Naoz, Joel D. Hartman, Joshua N. Winn, R. Paul Butler, Jeffrey D. Crane, Phil Evans, Tianjun Gan, Steve B. Howell, Michelle Kunimoto, David Osip, David Rapetti, Stephen A. Shectman, Keivan G. Stassun, Johanna K. Teske, Roberto Zambelli, George Zhou, Carl Ziegler
astro-ph.EP
Submitted: 2026-07-01
Comments: 26 pages, 10 figures
Code: https://github.com/hpparvi/PyDE
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- The Neptunian ridge as a natural outcome of high-eccentricity tidal migration
- EXOFASTv2: A public, generalized, publication-quality exoplanet modeling code
- POSEIDON II: The Anti-Aligned Orbit of the Warm Neptune TOI-1710 A b
- The Densities of Planets and the Masses of Host Stars
- Revealing the Origin of Desert Dwellers via Stellar Obliquities
- POSEIDON I: The Dynamical Origins of Transiting Neptunes
- Possible Dynamical Pathways to the Misalignment of the VHS 1256-1257 System
- Do Super-Puffs Defy Core Accretion? Population-Wide Interior Structure Constraints
- Once a Triple, Not Always a Triple: The Evolution of Hierarchical Triples that Yield Merged Inner Binaries
- The Hot Jupiter Radius Anomaly and Stellar Connections
- Analytical models for secular descents in hierarchical triple systems
- Dynamical tide modified Roche limit in eccentric, asynchronous binaries
- Dynamical Tides during High-Eccentricity Migration produces the Hot Jupiter Pile-up, Neptune Ridge, and Neptune Desert
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