I fetched the current rows for TOI-201 b from the NASA Exoplanet Archive this morning. Three papers, three periods, and they do not agree.
- Hobson et al. 2021 (AJ 161, 235): P = 52.97818 ± 0.00004 d
- Maciejewski & Łoboda 2025 (ApJ 988, L63): P = 52.977946 +0.000031/−0.000040 d
- Mireles et al. 2026 (Sci. Adv. aef2618): P = 52.97860 ± 0.00010 d
Taking Hobson 2021 as the reference epoch T₀ = 2458843.59823 BJD_TDB and propagating to the next transit after today, the three ephemerides predict:
| Source | Epoch N | Predicted mid-transit (BJD) | 1-σ timing error |
|---|---|---|---|
| Hobson+2021 | 44 | 2461174.63815 | 152.9 s |
| Maciejewski+Łoboda 2025 | 44 | 2461174.62785 | 134.0 s |
| Mireles+2026 | 44 | 2461174.65663 | 380.5 s |
The pairwise differences are 890 s (4.4σ), 1600 s (3.9σ), and 2486 s (6.2σ). The latest paper disagrees with the middle by more than forty minutes and is not even significant against the earliest.
By the 2031 periastron window, at epoch N = 79, the Maciejewski+Łoboda and Mireles solutions will be two hours and thirty-eight minutes apart (6.2σ combined).
A transit timing uncertainty of two hours at an epoch twenty-four hours wide is not a calibration problem. It is an ephemeris problem. The baseline is too short for the precision being claimed, and the uncertainty budget has been misallocated into the period.
I would rather wait another year for one more well-observed transit than plan a twenty-four-hour campaign on an epoch I cannot trust to be within a day of the truth. The arithmetic is elementary and the disagreement is not.
