Gravity around small black holes

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SUMMARY

The discussion centers on the gravitational effects around small black holes, specifically those with a mass similar to the Sun. It establishes that for a non-rotating black hole of one solar mass, the lowest stable orbit is approximately 9 kilometers from the event horizon, while the lowest circular orbit, where light can orbit, is at about 4.5 kilometers. The conversation highlights the significant relativistic effects that occur within 100 kilometers of such a black hole, contrasting it with the Sun's gravitational influence on nearby bodies. The discussion also notes that the radius concept becomes complex in the vicinity of a black hole.

PREREQUISITES
  • Understanding of general relativity and its implications on gravity
  • Familiarity with black hole physics and characteristics
  • Knowledge of orbital mechanics and stable orbits
  • Basic grasp of relativistic effects in astrophysics
NEXT STEPS
  • Research the properties of rotating black holes (Kerr black holes)
  • Study the concept of gravitational lensing and its effects near black holes
  • Explore the implications of perihelion precession in relativistic orbits
  • Learn about the Schwarzschild radius and its significance in black hole physics
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Astronomers, astrophysicists, and students of physics interested in black hole dynamics and gravitational effects in extreme environments.

Paul Katan
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If a black hole had a mass similar to the Sun (I know black holes tend to be at least three times larger but let's assume an unusual series of events) how far would the are of extremely distorted bent gravity around it be could it cause closely orbiting bodies to be pulled or pushed out of orbit around the black hole?
 
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A black hole has stable orbits around it in the same way all other objects have them. Even better: sun is a bit oblate due to its rotation, which has a notable influence on the perihelion precession of Mercury for example. A black hole is much smaller, so this effect gets much smaller as well.

Relativistic effects become strong very close to the black hole - for 1 solar mass, for distances below ~100 km. There are no orbits around the sun at that distance because sun is much larger, obviously. The lowest stable orbit depends on the spin of the black hole. If it is not rotating, the lowest stable orbit has a radius of about 9 kilometers. The lowest circular orbit is at about 4.5 kilometers (light can orbit here), and everything below that either falls into the black hole or escapes directly.
Note that "radius" is not a trivial concept close to a black hole.
 
Thanks
 

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