The star falls toward the black hole

As time progresses, the blue dot representing the location of the black hole remains fixed. However, the rate at which material from the nearby star falls toward the black hole can be observed varying over time.

Initially, there might be a gradual increase in the rate of material falling towards the black hole. This could result in an accretion disk forming around the black hole, where the material starts to swirl around it due to the immense gravitational pull.

Over time, the rate at which material falls towards the black hole might fluctuate. These variations can occur due to various factors such as the turbulence in the accretion disk, interactions with other celestial bodies, or even intense gravitational forces in the vicinity.

Observations over an extended period can help scientists understand the dynamics of the material falling into the black hole. Studying the rate at which material accretes onto the black hole gives insights into the black hole's mass, its behavior, and its surrounding environment
The blue dot indicates the location of the black hole. The rate at which material from the star falls toward the black hole can be seen over time.