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Why Hollywood Fudged the Relativity-Based Wormhole Scenes In Interstellar

KentuckyFC writes: When Christopher Nolan teamed up with physicist Kip Thorne of Caltech to discuss the science behind his movie Interstellar, the idea was that Thorne would bring some much-needed scientific gravitas to the all-important scenes involving travel through a wormhole. Indeed, Thorne used the equations of general relativity to calculate the various possible shapes of wormhole and how they would distort the view through it. A London-based special effects team then created footage of a far away galaxy as seen through such a wormhole. It showed the galaxy fantastically distorted as a result, just as relativity predicts. But when it came to travelling through a wormhole, Nolan was disappointed with the footage.

The problem was that the view of the other side when travelling through a wormhole turns out to be visually indistinguishable from a conventional camera zoom and utterly unlike the impression Nolan wanted to portray, which was the sense of travelling through a shortcut from one part of the universe to another. So for the final cut, special effects artists had to add various animations to convey that impression. "The end result was a sequence of shots that told a story comprehensible by a general audience while resembling the wormhole's interior," admit Thorne and colleagues in a paper they have published about wormhole science in the film. In other words, they had to fudge it. Nevertheless, Thorne is adamant that the visualisations should help to inspire a new generation of students of film-making and of relativity.

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  1. Re:Well, if they wanted to make it more realistic. by Anonymous Coward · · Score: 4, Informative

    No they wouldn't. A supermassive black hole of the size mentioned in the movie has less gravitational tidal forces at the event horizon than what you have at the surface of the earth. You are being pulled apart right now more than you would be near that black hole. It's size makes the event horizon radius very large so the gravitational differences per length are small that far away from the point of the singularity.