Fate of Galaxies: Will Stars be Pulled into Black Holes?

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SUMMARY

The discussion centers on the fate of stars in galaxies, particularly regarding their potential to be pulled into supermassive black holes. It is established that while the orbits of stars in the Milky Way are stable, gravitational radiation from the black hole can cause energy loss for nearby stars. Close interactions between stars can lead to some being ejected from the galaxy, while others may spiral closer to the black hole over time. Additionally, the formation of smaller stellar black holes and the theoretical concept of proton decay are mentioned as factors influencing the long-term fate of matter in the universe.

PREREQUISITES
  • Understanding of gravitational radiation and its effects on stellar orbits
  • Knowledge of supermassive black holes and their role in galaxies
  • Familiarity with stellar dynamics and interactions
  • Concept of proton decay in theoretical physics
NEXT STEPS
  • Research the mechanics of gravitational radiation and its impact on star orbits
  • Explore the role of supermassive black holes in galaxy evolution
  • Study stellar dynamics and the processes leading to star ejection from galaxies
  • Investigate the implications of proton decay in the context of cosmology
USEFUL FOR

Astronomers, astrophysicists, and anyone interested in the long-term evolution of galaxies and the dynamics of black holes.

pforeman
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In the far distant future, will all of the stars in a galaxy be pulled into one giant black hole in the center?
Are the arms of spiral galaxies like our milky way spiralling in or flying out?
Thanks
Paul
 
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That is still being debated. I seriously doubt 'all' stars will be absorbed by supermassive black holes, which seriously complicates any theory the universe will eventually achieve a state of perfect thermodynamic equilibrium.
 
pforeman said:
In the far distant future, will all of the stars in a galaxy be pulled into one giant black hole in the center?
Are the arms of spiral galaxies like our milky way spiralling in or flying out?
Thanks
Paul
For the most part, the orbits of stars in our galaxy are extremely stable. For objects close to the black hole, there is some gravitational radiation that causes the objects to lose orbital energy. But the magnitude of this radiation is extremely dependent upon distance, and is pretty negligible for objects even a short (in astrophysical terms) distance away.

Every once in a great while, there will be a close interaction between stars which transfers enough momentum to one star to kick it out of the galaxy. The galaxy loses one star, but the remaining stars have less orbital energy between them and are, after that interaction, on average a bit closer to the orbiting black hole. After many such interactions, more stars are liable to have fallen into the central black hole.

At the same time, matter within our galaxy is (occasionally) forming smaller stellar black holes which very slowly radiate away to nothing.

On extremely long time scales, matter itself is likely to decay through a process known as proton decay.

All of these processes are incredibly slow, and I couldn't tell you which will win out. But Wikipedia has a nice article on the subject:
http://en.wikipedia.org/wiki/Future_of_an_expanding_universe
 

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