The discussion centers on the concept of whether the supermassive black hole at the center of the galaxy exhibits a "wobble" similar to the Sun's motion around the solar system's barycenter. It is suggested that while black holes can wobble due to gravitational influences, the massive black hole in the galaxy's core is likely stable due to the uniform distribution of mass around it. Observationally, detecting such a wobble could be challenging, but it might be measurable in stable accretion disks around black holes. The conversation also clarifies misconceptions about black holes, emphasizing that they are not created from small-scale events but from significant accumulations of mass. Overall, the dynamics of black holes and their interactions within their environments remain complex and intriguing.