Wide binary star pairs separated by light-years orbit at ultra-low gravitational accelerations where modified gravity theories predict deviations from Newton; meticulous Gaia data quality auditing reveals that unresolved triple-star systems account for claimed gravity anomalies.

At the astronomical outskirts of star systems, wide binary stars orbit each other at separations of thousands of astronomical units, experiencing infinitesimal gravitational accelerations below one ten-billionth of a meter per second squared.
Modified Newtonian Dynamics (MOND) claims that at these ultra-low accelerations, standard gravity breaks down without needing dark matter, with several high-profile papers claiming wide binary velocities prove Newton and Einstein wrong.
This rigorous astrophysical analysis re-evaluates Gaia data quality control, demonstrating that prior claims of gravitational anomalies failed to account for undetected close stellar companions (hidden tertiary stars). When multiple-star orbital dynamics and parallax errors are rigorously modeled, wide binary orbits adhere strictly to classical Newtonian gravitation.
Defending standard gravity in wide binary orbits refutes recent MOND claims, demonstrating that dark matter remains the most robust explanation for anomalous galactic rotation curves.
Revisiting Data Quality Control and Multiple-star Modeling in Wide Binary Gravity Tests: Confirmation of MOND-type Gravitational Anomaly at Low Acceleration
Wide binary stars provide natural laboratories for directly probing gravity in the low-acceleration regime, as dark matter inferred from any viable gravity has negligible effects on their internal dynamics. Various recent studies including Bayesian 3D analyses have shown that wide binaries with separations greater than several thousand astronomical units experience MOND-type gravity with a boost factor of . However, results claiming preference for, or no deviation from, standard gravity have also been published during the same period, particularly highlighting the roles of data quality control and realistic modeling of multiple-star (i.e., triple and higher-order) systems that host hidden companion stars. Here we carefully reexamine the issues of data quality control and modeling multiple-star systems in statistical gravity tests based on sky-projected 2D velocities of wide binary stars. Through extensive tests including the acceleration-plane test, the -distribution test, and the median--profile test (where is the sky-plane 2D relative velocity normalized by the Newtonian circular velocity between the two stars), we show that proper data quality control or reasonable variation in multiple-star modeling cannot remove the low-acceleration gravitational anomaly but confirms the MOND-type gravitational anomaly, particularly consistent with recent realistic MOND solutions of wide binary orbits. We find that studies claiming no evidence for the low-acceleration gravitational anomaly are consequences of bypassed calibration of the fraction of multiple-star systems using the Newtonian-regime data, bias-introduction in data quality control that is not taken into account in gravity tests, or insufficient statistics in the low-acceleration regime.
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