Time Dilation & Visual Observation of Black Holes

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SUMMARY

The discussion centers on the effects of time dilation and gravitational influence on objects orbiting supermassive black holes, specifically regarding visual observations of stars near the event horizon. It is established that while objects in elliptical orbits accelerate as they approach their attractor, gravitational time dilation causes distant observers to perceive these objects as slowing down. The consensus is that stars orbiting the supermassive black hole at the center of the Milky Way are sufficiently far away that time dilation does not significantly impact observational calculations.

PREREQUISITES
  • Understanding of general relativity and gravitational time dilation
  • Familiarity with orbital mechanics and elliptical orbits
  • Knowledge of black hole physics, particularly event horizons
  • Basic principles of observational astronomy
NEXT STEPS
  • Research the effects of gravitational time dilation near event horizons
  • Study the dynamics of elliptical orbits in strong gravitational fields
  • Examine observational techniques for studying stars near black holes
  • Learn about the properties and behaviors of supermassive black holes
USEFUL FOR

Astronomers, astrophysicists, and students of physics interested in the dynamics of black holes and the effects of gravity on time and motion.

EskWIRED
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I'm under the impression that one sees clocks slow down when watching distant objects approaching strong sources of gravity, such black holes. And that objects in an elliptical orbit travel faster when they are near their attractor.

I can't quite figure out how these two phenomenon work together when an such an object travels close to a black hole.

If one were to watch a star orbiting a supermassive black hole, might it appear to slow down, rather than speed up at its closes approach, given sufficient time dilation close to the event horizon?
 
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EskWIRED said:
If one were to watch a star orbiting a supermassive black hole, might it appear to slow down, rather than speed up at its closes approach, given sufficient time dilation close to the event horizon?

There are no stable orbits inside a radius of three times the horizon radius, and no free-fall orbits at all, even unstable ones, inside one and a half times the horizon radius. Even the latter radius is not close enough to the horizon for gravitational time dilation to counteract increasing orbital speed.
 
Thanks.

Does time dilation need to be taken into account when observing or making calculations concerning stars orbiting the black hole at the center of the Milky Way? Or are they far enough away at all times that time dilation can be ignored?
 
EskWIRED said:
Does time dilation need to be taken into account when observing or making calculations concerning stars orbiting the black hole at the center of the Milky Way?

AFAIK, no. None of them are close enough for it to be a significant factor.
 

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