What the movie Interstellar got right and wrong?

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    Interstellar Movie
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Discussion Overview

The discussion revolves around the scientific accuracy of concepts presented in the movie "Interstellar," particularly focusing on the effects of black holes on time dilation, the feasibility of habitable planets near black holes, and the implications of tidal forces. Participants explore theoretical scenarios and mathematical considerations related to these topics.

Discussion Character

  • Exploratory
  • Technical explanation
  • Debate/contested

Main Points Raised

  • Some participants discuss the possibility of a planet existing close to a black hole where time moves differently compared to Earth, questioning the mathematical framework to quantify this time difference.
  • There are assertions that if one were to orbit a black hole, the effects of time dilation would be significant, with potential differences in aging rates across a spacecraft due to gravitational gradients.
  • One participant suggests that a large black hole could allow for significant time dilation while minimizing tidal forces, making it theoretically possible for a planet to support human life.
  • Questions are raised about the habitability of such a planet, including the presence of an atmosphere and the physical conditions necessary for human survival.
  • Some participants note that the equations relevant to time dilation near a black hole are complex, especially for rotating black holes, and reference the need for specific mathematical derivations.
  • A participant expresses skepticism about the plausibility of the frozen “clouds” depicted in the movie, suggesting they may not be clouds but rather ice formations.

Areas of Agreement / Disagreement

The discussion contains multiple competing views regarding the feasibility of habitable planets near black holes and the implications of tidal forces and time dilation. Participants do not reach a consensus on these topics.

Contextual Notes

Participants acknowledge the complexity of the equations involved, particularly in scenarios with rotating black holes, and the limitations of existing references for deriving these equations. There is also uncertainty regarding the physical characteristics of the planet depicted in the movie.

RandyD123
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We all know that getting too close to the gravity well of a massive object like a black hole causes time to move more slowly for you than it would for people on Earth. But is it possible for a planet to exist close enough to a black hole and have a person actually stand on that planet? And if possible is there math that could be use to figure out how much time has passed on Earth vs. your time?
 
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If you get close enough for these effects to be relevant, I would expect the gradient of the fields to be great enough that one end of the ship would be getting older at a detectably different rate from the other end. Anyone could get into an orbit around a black hole and it would feel the same as the orbit around a star. . . . only you wouldn't see the central attractor.
Time dilation and other effects are detectable under pretty mild conditions, of course.
 
The idea is that the black hole is big, keeping tidal forces down, while providing significant time dilation. It's certainly possible to have hours on such a planet be years on Earth.

Hyperphysics has that equation:
http://hyperphysics.phy-astr.gsu.edu/hbase/Relativ/gratim.html

You wou'd want to select a maximum comfortable tidal acceleration and set the mass and distance parameters equal. I'd probably plug them into a spreadsheet and play with the parameters until I liked the result
 
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But can a human walk on that planet? And can that planet have atmosphere to support a human?
 
RandyD123 said:
But can a human walk on that planet? And can that planet have atmosphere to support a human?
There's no reason why it couldn't and it isn't clear to me what you think would happen. Remember, when you are in orbit, everything is in orbit together So orbiting the black hole while on a planet orbiting the black hole doesn't have a noticeable effect on you if the tidal force is low.
 
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sophiecentaur said:
If you get close enough for these effects to be relevant, I would expect the gradient of the fields to be great enough that one end of the ship would be getting older at a detectably different rate from the other end.

Not if the hole is large enough. The hole in Interstellar is supermassive (I believe a billion or so solar masses), so tidal gravity even very close to its horizon will be small.
 
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russ_watters said:
Hyperphysics has that equation

The equations on that page only apply to an observer hovering at rest above a non-rotating black hole's horizon. The situation in Interstellar is more complicated, because the hole is rotating and the planet is in a circular orbit. I can't find any online reference that gives the exact equation in question, but it should be fairly straightforward to derive it from the Kerr metric; if I have time later I'll try to do that.

Kip Thorne has published a book giving the detailed math that he worked out for the movie:

https://www.amazon.com/dp/0393351378/?tag=pfamazon01-20
 
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Slightly off topic, but what about the frozen “clouds” on the other planet. Seems implausible. I mean, unless they weren’t really clouds but were large ice mountains or something.
 

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