Im Jahr verschwindet das Raumschiff Event Horizon urplötzlich in einem schwarzen Loch, und aus dem Routineauftrag wird ein Horrortrip. Erst sieben. Schnittberichte, News (z.B. Uncut-DVDs & Blu-rays) und Reviews zu Event Horizon - Am Rande des Universums (Großbritannien, | Horror, Science-Fiction. autobianchi-a112.com: Paul W.S. Andersons „Event Horizon“ hat trotz des finanziellen und kritischen Flops bei vielen Fans Kultstatus. Demnächst.
Event Horizon - Am Rande des UniversumsEvent Horizon (Lim. Uncut Mediabook - Cover A) (DVD + BLURAY). Logo Bluray Logo DVD. Kurzübersicht. MediaBook - 2 Discs. Event Horizon is considered one of the best, albeit, messed up, sci-fi/horror movies of the 90's. Now that's out of the way, a brief introduction. Anderson wollte. autobianchi-a112.com - Kaufen Sie Event Horizon - Am Rande des Universums (Special Collector's Edition) günstig ein. Qualifizierte Bestellungen werden kostenlos.
Event Horizon Uncut 📩 Stay up-to-date VideoEvent Horizon slow broken broadcast
Initially, the film ran for at least minutes. This cut contained far more graphic violence and gore than the released version of the film. When Anderson screened the film for Paramount, they were disturbed by how horribly gruesome it was.
She would have seen maggots crawling all over them. Weir briefly hallucinates Justin turning into his late wife, who stares at him despite her notable lack of eyes.
Get the best of Den of Geek delivered right to your inbox! The special edition DVD managed to find a couple of deleted moments, including a briefing scene establishing the re-emergence of the Event Horizon.
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Fact Fiend. Entertainment Science. Share on Facebook. The ship disappeared mysteriously 7 years before on its maiden voyage and with its return comes even more mystery as the crew of the "Lewis and Clark" discover the real truth behind its disappearance and something even more terrifying.
The film starts well, and is enjoyable up until right after the crew boards the Event Horizon. After that, it degenerates into a bad copy of several well-known horror films, which all have better gore scenes.
The plot disappears in quasi-religious babble, and the impression of a good sci-fi movie disappears. While the first part of the film was good, I was very disappointed by the conclusion.
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Official Sites. Company Credits. Technical Specs. Plot Summary. In , John Michell proposed that in the vicinity of compact massive objects, gravity can be strong enough that even light cannot escape.
At that time, the Newtonian theory of gravitation and the so-called corpuscular theory of light were dominant.
In these theories, if the escape speed of an object exceeds the speed of light, then light originating inside or from it can escape temporarily but will return.
In , David Finkelstein used General Relativity to introduce a stricter definition of a local black hole event horizon as a boundary beyond which events of any kind cannot affect an outside observer.
This led to information and firewall paradoxes, which encouraged the re-examination of the concept of local event horizons and the notion of black holes.
Several theories were subsequently developed, some with and some without event horizons. Stephen Hawking , who was one of the leading developers of theories to describe black holes, suggested that an apparent horizon should be used instead of an event horizon, saying "gravitational collapse produces apparent horizons but no event horizons".
He eventually concluded that "the absence of event horizons mean that there are no black holes — in the sense of regimes from which light can't escape to infinity.
Any object that approaches the horizon from the observer's side appears to slow down and never quite crosses the horizon.
In an expanding universe the speed of expansion reaches and even exceeds the speed of light, which prevents signals from travelling to some regions.
A cosmic event horizon is a real event horizon because it affects all kinds of signals, including gravitational waves which travel at the speed of light.
More specific types of horizon include the related but distinct absolute and apparent horizons found around a black hole.
Other distinct types include the Cauchy and Killing horizons ; the photon spheres and ergospheres of the Kerr solution ; particle and cosmological horizons relevant to cosmology ; and isolated and dynamical horizons important in current black hole research.
In cosmology , the event horizon of the observable universe is the largest comoving distance from which light emitted now can ever reach the observer in the future.
This differs from the concept of the particle horizon , which represents the largest comoving distance from which light emitted in the past could reach the observer at a given time.
For events that occur beyond that distance, light has not had enough time to reach our location, even if it was emitted at the time the universe began.
The evolution of the particle horizon with time depends on the nature of the expansion of the universe. If the expansion has certain characteristics, parts of the universe will never be observable, no matter how long the observer waits for the light from those regions to arrive.
The boundary beyond which events cannot ever be observed is an event horizon, and it represents the maximum extent of the particle horizon.
The criterion for determining whether a particle horizon for the universe exists is as follows. Define a comoving distance d p as.
In this equation, a is the scale factor , c is the speed of light , and t 0 is the age of the Universe. Examples of cosmological models without an event horizon are universes dominated by matter or by radiation.
An example of a cosmological model with an event horizon is a universe dominated by the cosmological constant a de Sitter universe. A calculation of the speeds of the cosmological event and particle horizons was given in a paper on the FLRW cosmological model, approximating the Universe as composed of non-interacting constituents, each one being a perfect fluid.Anderson sagt, das Material sei unauffindbar. Dfb Pikal Kabel 1 Event Horizon.