Seeing the Unseen: Visualizing a Rotating Black Hole

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Black holes, particularly rotating ones known as Kerr black holes, have an ellipsoidal shape rather than being perfectly spherical. The event horizon's appearance varies based on the observer's position, with effects like gravitational lensing causing starlight to warp around it. For a boosted black hole, the event horizon may appear Lorentz contracted, altering its visual representation. The discussion emphasizes the complexities of visualizing black holes due to their unique geometrical and optical properties. Understanding these characteristics is crucial for comprehending the nature of black holes and their interactions with light.
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Of course one would suspect the title is quite odd because Black Holes don't allow anything with the velocity from 0 to c to escape once they pass the Event Horizon, excluding Bekenstein-Hawking Radiation but that is a concept that is irrelevant in this context. The trouble I'm having in visualizing a Black Hole is the apparent shape of the Event Horizon or the Black Hole itself, is it spherical as though it would appear similar from any observer dependant on their position around the Black Hole or is it a two dimensional circle then so from a front observer and opposite observer it would look "identical" but not to a side observer.

Thanks, Kevin
 
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A non-rotating black hole is spherical; rotating one is ellipsoidal.
 
Thanks, concise and the answer I was looking for. By a rotating black hole do you just mean a Kerr Black?
 
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Also, for a boosted black hole, you can imagine the event horizon simply appearing lorentz contracted, so that it pancakes perpendicular to the line of motion.
 
Kevin_Axion said:
Thanks, concise and the answer I was looking for. By a rotating black hole do you just mean a Kerr Black?

Yep, it would be a Kerr black hole. In that scenario Nabeshin's point would be pretty impressive too. Beyond the structure of the hole itself, you'd also have the effects of gravitational lensing of starlight behind and around the event horizon, warped and "squashed" into the ellipse of its rotation. This assumes no accretion disk to obscure the view.
 
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