An independent Gaussian error model permits a bound Newtonian orbit for TYC 6382-243-1 and TYC 6382-241-1

We test whether the published measurements of 12 wide stellar pairs permit bound Newtonian states within a joint error region. The primary model uses independent Gaussian printed astrometric errors and a 40 m/s radial velocity calibration term for each star. For pair 11, TYC 6382-243-1 and TYC 6382-241-1, the minimum squared standardized change is 8.41. The nominal 95 percent joint limit for eight measurements is 15.51. An explicit finite ellipse has eccentricity 0.655, semimajor axis 57,068 AU, and change 13.12. Pair 11 also permits bound states with catalogue astrometric correlations and with a smaller 40 m/s differential radial velocity term. The result changes if the calibration errors are strongly shared. Conservative box bounds exclude bound states from the primary joint region for pairs 7 and 12. This is an error compatibility test. It does not show that pair 11 is bound or that gravity is anomalous. The package includes source data attribution, code, figures, numerical results, and reproduction instructions.

wide binaries · Newtonian orbits · radial velocity · Gaia · measurement errors · error covariance · reproducible astronomy