Consolidated Technical Report V.3.0: Hybrid Orbital Model and Gravitational Resonance Validation for TOI-561 f
Abstract
This consolidated technical report (Version 3.0) provides a refined orbital solution for the exoplanet candidate TOI-561 f. By synthesizing previous models with N-body gravitational simulations, the UCSU team identifies a stable 421.5-day period sustained by an 11:2 resonance with TOI-561 e. The report includes precise ephemeris for the April 03, 2026 transit window and predicts a measurable TTV shift of -6.4 minutes. Issued for the global astronomical community for real-time verification.
Fields of Study & Subjects
Stellar
planetary
and galactic studies
Astronomy and Astrophysical Research
Astro and Planetary Science
Publication details
- Journal / source
- Zenodo (CERN European Organization for Nuclear Research)
- Publication date
- 7 March 2026
- Language
- EN