Time Dilation & Visual Observation of Black Holes

In summary, when watching distant objects approaching strong sources of gravity, such as black holes, their clocks may appear to slow down. This is also true for objects in elliptical orbits, which travel faster when they are near their attractor. However, when observing a star orbiting a supermassive black hole, it may appear to slow down rather than speed up at its closest approach, due to the significant time dilation close to the event horizon. However, there are no stable or free-fall orbits close enough to the horizon for gravitational time dilation to counteract increasing orbital speed. Therefore, time dilation does not need to be taken into account when observing or making calculations concerning stars orbiting the black hole at the center of the Milky Way,
  • #1
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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  • #2
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.
 
  • #3
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?
 
  • #4
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.
 

FAQ: Time Dilation & Visual Observation of Black Holes

1. What is time dilation?

Time dilation is a phenomenon where time appears to pass slower for an object in motion compared to an observer at rest. This is due to the effects of speed and gravity on the flow of time, as predicted by Einstein's theory of relativity.

2. How does time dilation relate to black holes?

In the vicinity of a black hole, the strong gravitational pull causes an extreme distortion of spacetime, resulting in a significant time dilation effect. This means that time appears to pass slower for an observer near a black hole compared to someone far away from it.

3. Can we observe time dilation near a black hole?

Yes, time dilation near a black hole can be observed through the phenomenon of gravitational lensing. This is when the intense gravitational pull of a black hole bends and distorts light, causing objects near the event horizon to appear elongated or distorted.

4. How does time dilation affect our perception of black holes?

The extreme time dilation near a black hole means that objects near the event horizon will appear frozen in time to an outside observer. This makes it difficult to observe and gather information about what is happening inside the black hole.

5. Is time dilation a proven concept?

Yes, time dilation has been proven through various experiments and observations, including the famous Hafele-Keating experiment and the observations of the behavior of atomic clocks on GPS satellites. It is also an integral part of Einstein's theory of general relativity, which has been extensively tested and confirmed by numerous experiments and observations.

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