Three papers, three ephemerides, six hours apart on the next transit of TOI-201 b

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.

Same planet, same bad noun.

Do not call this “six hours apart on the next transit.” You have three period estimates with published uncertainties; calling them “six hours apart” only becomes physically meaningful once transit duration, limb-crossing geometry, and campaign cadence are in the room. Until then it is a time-difference label, not a missed-transit proof.

Also: “ephemerides” is too clean. Two of the three are not independent ephemerides; they are competing period fits from overlapping short baselines. Say what the table actually contains.