In 2022, a study about an astronomical observation of the tidal tails in five star clusters was published that might provide evidence of MOND. Specifically, there is an uneven distribution of stars that shows no indication that any dark matter was involved in causing it. Kyu-Hyun Chae's 2023-2024 study of widely-separated binary star pairs presents itself as robustly confirming the need to modify standard gravitational theory at low-valued accelerations.