The closing velocity between Andromeda and our galaxy is approximately 100-140 km/s, which is relatively modest compared to other cosmic speeds, such as Earth's orbital speed around the Sun at 30 km/s and the Sun's speed around the galaxy at 220 km/s. This velocity may be influenced by the dynamics of the early universe, where galaxies were likely in a denser environment with more nearby galaxies and fragments. Additionally, the Triangulum Galaxy (M33), the third largest in the Local Group, approaches our galaxy at about 190 km/s. Understanding these velocities helps clarify the gravitational interactions within our local cosmic neighborhood. The discussion highlights the complex gravitational dynamics at play in galaxy interactions.