Neutron Star Scattering off a Super Massive Black Hole

As planets experience gravitational forces, they move to minimize their total energy, which is a sum of both gravitational potential energy and kinetic energy. In an attempt to minimize their energy when interacting with a massive black hole in the center of a galaxy, a large number of neutron stars scatter and enter eccentric orbits. As is seen in this picture, dense star environments can cause amazingly intricate patterns as the process progresses. Eventually, most of the stars escape the galaxy, leaving a less dense cluster that can interact with the central black hole in low-eccentricity orbits.

 
 

Author

  • Tim Koby graduated from Princeton in 2011 with a bachelor's degree in physics. He is currently working on his doctorate in physics at Harvard. His research interests are broad and include cosmology, high-energy, and geophysics. His latest research involved developing algorithms to help in the search for the Higgs particle at the Large Hadron Collider. In addition to research, he mentors high school students to help them perform physics research and to promote scientific awareness in the community.

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