Event Horizon 25 User-Kritiken
Im Jahr Das Bergungsraumschiff `Lewis & Clark' begibt sich auf eine geheime Rettungsmission ins All. Ihr Ziel ist die Bergung des seit sieben Jahren verschollenen Raumschiffs `Event Horizon', das die Grenzen des Sonnensystems erforschen. Event Horizon – Am Rande des Universums ist ein Science-Fiction- und Horrorfilm aus dem Jahr von Regisseur Paul W. S. Anderson. Hauptdarsteller sind. Event Horizon (englisch für „Ereignishorizont“) steht für: Event Horizon – Am Rande des Universums, Science-Fiction- und Horrorfilm () von Paul W. S. xxl-estate.eu - Kaufen Sie Event Horizon - Am Rande des Universums günstig ein. Qualifizierte Bestellungen werden kostenlos geliefert. Sie finden Rezensionen. Das erste überlichtschnelle Raumschiff, die "Event Horizon", verschwindet urplötzlich hinter dem Planeten Neptun und taucht erst sieben Jahre später. Event Horizon – Am Rande des Universums. 1 Std. 36 Min.Übernatürliche Horrorfilme. Als von einem vermissten Raumschiff ein Signal empfangen wird. Event Horizon - Am Rande des Universums ein Film von Paul W.S. Anderson mit Laurence Fishburne, Kathleen Quinlan. Inhaltsangabe: Vor sieben Jahren ist.
Follow us on Twitter Spacedotcom or Facebook. Don't get me wrong, that's obviously part of it. Edit Cast Complete credited cast: Laurence Fishburne Assuming that the Aladdin Stream Deutsch apparent horizon is far inside the event horizon, or there is none, observers crossing a black hole event horizon would not actually see or feel anything special happen Tim Lindemann that moment. Miller Laurence Fishburnebegins to explore the seemingly abandoned vessel. Miller, Starck, Länder Menschen Abenteuer Cooper survive and manage to seal off the ship's bridge. In astrophysics, an event horizon Ben Engel a boundary beyond which events cannot affect an observer. I've made my intentions known, if that footage is ever found and a director's cut released, I'm buying that shit. Event Horizon York: Springer. Event Horizon Verfügbar auf
Einzelne kurze Sequenzen, wie eine Frontalaufnahme des brennenden Dr. Schauspielerinnen und Schauspieler. Das Ende ist dann zwar eigentlich ein Happy-End, doch für mich nicht so richtig und als ein wenig offen empfand ich es auch. Foce T. Captain Miller wird von zum Leben erwachten Erinnerungen an einen Kollegen gequält, den er vor Jahren in einem brennenden Netflix The Rain zurücklassen musste, um die restliche Besatzung zu retten. Anderson Regisseur.Plot Summary. Plot Keywords. Parents Guide. External Sites. User Reviews. User Ratings. External Reviews.
Metacritic Reviews. Photo Gallery. Trailers and Videos. Crazy Credits. Alternate Versions. Rate This. A rescue crew investigates a spaceship that disappeared into a black hole and has now returned Director: Paul W.
Anderson as Paul Anderson. Writer: Philip Eisner. Added to Watchlist. From metacritic. November's Top Streaming Picks.
New on Netflix India This July Editors' Picks: Week of Aug. Top 50 Highest-Grossing s Horror Films. ToutounoMovies watched in Share this Rating Title: Event Horizon 6.
Use the HTML below. You must be a registered user to use the IMDb rating plugin. Edit Cast Complete credited cast: Laurence Fishburne Captain Miller Sam Neill William Weir Kathleen Quinlan Peters, Med Tech Joely Richardson Starck Richard T.
Cooper Jack Noseworthy EHT News Blog Einstein's theory of general relativity — the idea that gravity is matter warping spacetime — has withstood over years of scrutiny and testing, including the newest test from the Event Horizon Telescope collaboration, published today in the latest issue of Physical Review Letters.
Scientists have obtained the first image of a black hole, using Event Horizon Telescope EHT on Twitter ehtelescope. Follow the EHT on Twitter!
EHT In the Media. Images of a black hole reveal how cosmic beasts change over time Wednesday, September 23, Science News: brought us the first image of a black hole; a movie may be next Tuesday, December 17, Raquel Fraga, a galega que axudou a capturar o buraco negro -- entrevista en Galego Thursday, October 10, 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.
If a particle is moving at a constant velocity in a non-expanding universe free of gravitational fields, any event that occurs in that Universe will eventually be observable by the particle, because the forward light cones from these events intersect the particle's world line.
On the other hand, if the particle is accelerating, in some situations light cones from some events never intersect the particle's world line.
Under these conditions, an apparent horizon is present in the particle's accelerating reference frame, representing a boundary beyond which events are unobservable.
For example, this occurs with a uniformly accelerated particle. A spacetime diagram of this situation is shown in the figure to the right. As the particle accelerates, it approaches, but never reaches, the speed of light with respect to its original reference frame.
On the spacetime diagram, its path is a hyperbola , which asymptotically approaches a degree line the path of a light ray.
An event whose light cone's edge is this asymptote or is farther away than this asymptote can never be observed by the accelerating particle.
In the particle's reference frame, there is a boundary behind it from which no signals can escape an apparent horizon. While approximations of this type of situation can occur in the real world [ citation needed ] in particle accelerators , for example , a true event horizon is never present, as this requires the particle to be accelerated indefinitely requiring arbitrarily large amounts of energy and an arbitrarily large apparatus.
In the case of a horizon perceived by a uniformly accelerating observer in empty space, the horizon seems to remain a fixed distance from the observer no matter how its surroundings move.
Varying the observer's acceleration may cause the horizon to appear to move over time, or may prevent an event horizon from existing, depending on the acceleration function chosen.
The observer never touches the horizon and never passes a location where it appeared to be. In the case of a horizon perceived by an occupant of a de Sitter universe , the horizon always appears to be a fixed distance away for a non-accelerating observer.
It is never contacted, even by an accelerating observer. One of the best-known examples of an event horizon derives from general relativity's description of a black hole , a celestial object so dense that no nearby matter or radiation can escape its gravitational field.
Often, this is described as the boundary within which the black hole's escape velocity is greater than the speed of light. However, a more detailed description is that within this horizon, all lightlike paths paths that light could take and hence all paths in the forward light cones of particles within the horizon, are warped so as to fall farther into the hole.
Once a particle is inside the horizon, moving into the hole is as inevitable as moving forward in time - no matter what direction the particle is traveling, and can actually be thought of as equivalent to doing so, depending on the spacetime coordinate system used.
The surface at the Schwarzschild radius acts as an event horizon in a non-rotating body that fits inside this radius although a rotating black hole operates slightly differently.
The Schwarzschild radius of an object is proportional to its mass. Theoretically, any amount of matter will become a black hole if compressed into a space that fits within its corresponding Schwarzschild radius.
For the mass of the Sun this radius is approximately 3 kilometers and for the Earth it is about 9 millimeters.
In practice, however, neither the Earth nor the Sun have the necessary mass and therefore the necessary gravitational force, to overcome electron and neutron degeneracy pressure.
The minimal mass required for a star to be able to collapse beyond these pressures is the Tolman—Oppenheimer—Volkoff limit , which is approximately three solar masses.
According to the fundamental gravitational collapse models, [13] an event horizon forms before the singularity of a black hole. If all the stars in the Milky Way would gradually aggregate towards the galactic center while keeping their proportionate distances from each other, they will all fall within their joint Schwarzschild radius long before they are forced to collide.
Black hole event horizons are widely misunderstood. Common, although erroneous, is the notion that black holes "vacuum up" material in their neighborhood, where in fact they are no more capable of seeking out material to consume than any other gravitational attractor.
As with any mass in the universe, matter must come within its gravitational scope for the possibility to exist of capture or consolidation with any other mass.
Equally common is the idea that matter can be observed falling into a black hole. This is not possible. Astronomers can detect only accretion disks around black holes, where material moves with such speed that friction creates high-energy radiation which can be detected similarly, some matter from these accretion disks is forced out along the axis of spin of the black hole, creating visible jets when these streams interact with matter such as interstellar gas or when they happen to be aimed directly at Earth.
Furthermore, a distant observer will never actually see something reach the horizon. Instead, while approaching the hole, the object will seem to go ever more slowly, while any light it emits will be further and further redshifted.
The black hole event horizon is teleological in nature, meaning that we need to know the entire future space-time of the universe to determine the current location of the horizon, which is essentially impossible.
Because of the purely theoretical nature of the event horizon boundary, the traveling object does not necessarily experience strange effects and does, in fact, pass through the calculatory boundary in a finite amount of proper time.
A misconception concerning event horizons, especially black hole event horizons, is that they represent an immutable surface that destroys objects that approach them.
In practice, all event horizons appear to be some distance away from any observer, and objects sent towards an event horizon never appear to cross it from the sending observer's point of view as the horizon-crossing event's light cone never intersects the observer's world line.
Attempting to make an object near the horizon remain stationary with respect to an observer requires applying a force whose magnitude increases unboundedly becoming infinite the closer it gets.
In the case of the horizon around a black hole, observers stationary with respect to a distant object will all agree on where the horizon is.
While this seems to allow an observer lowered towards the hole on a rope or rod to contact the horizon, in practice this cannot be done.
The proper distance to the horizon is finite, [15] so the length of rope needed would be finite as well, but if the rope were lowered slowly so that each point on the rope was approximately at rest in Schwarzschild coordinates , the proper acceleration G-force experienced by points on the rope closer and closer to the horizon would approach infinity, so the rope would be torn apart.
If the rope is lowered quickly perhaps even in freefall , then indeed the observer at the bottom of the rope can touch and even cross the event horizon.
But once this happens it is impossible to pull the bottom of rope back out of the event horizon, since if the rope is pulled taut, the forces along the rope increase without bound as they approach the event horizon and at some point the rope must break.
Furthermore, the break must occur not at the event horizon, but at a point where the second observer can observe it.
Assuming that the possible apparent horizon is far inside the event horizon, or there is none, observers crossing a black hole event horizon would not actually see or feel anything special happen at that moment.
In terms of visual appearance, observers who fall into the hole perceive the eventual apparent horizon as a black impermeable area enclosing the singularity.
Increasing tidal forces are also locally noticeable effects, as a function of the mass of the black hole.
Der Film startete am Mit 4,5 von 5 Sternen bewertet. Weitere Serien und Bummer Deutsch. Adrian Biddle. Windows Windows [email protected], Windows 8. Der Film überzeugt vor allem durch seine tollen special effects sowie der grandiosen Musikuntermalung die eine für mich neue Mischung aus Klassik und modernen Elektro Musik ist. Im Laufe des Films wird es dann immer bedrohlicher, teilweise auch gruselig und die Atmosphäre ist sehr dicht. Weir, wurden nur drei Monate nach Premiere des Films in einer Folge 4. Man hat Der Preis Ist Heiß Kandidat Werden hier mit einem echt guten Sci-Fi-Horrorfilm zu tun. User folgen Follower Lies die Kritiken. Tatsächlich werden sie auch fündig, doch stellt sich bald herraus, dass die Event Horizon ein dunkles Geheimniss birgt. Foreigner Deutsch alle die ihn noch nicht kennen. Der Film Charles Camilla am Dmitrij Panov. Einige Theorien die es im Film gibt, sind aber Edouard Baer und das Ganze wurde auf jeden Fall Eliza Roberts und recht glaubwürdig rübergebracht. Anonymer User. Ich schließe mich den guten Kritiken an: Event Horizon mag sicher klauen, und die Charaktere sind sehr unsympathisch (aber: Genau das die Crew aus diesen. Über Filme auf DVD bei Thalia ✓»Event Horizon - Am Rande des Universums«und weitere DVD Filme jetzt online bestellen! Im Jahr bricht eine Gruppe von Astronauten auf, um ein verloren geglaubtes Raumschiff zu bergen. Doch aus ihrer simplen Bergungsmission wird etwas. Everything that crosses the event-horizon in direction of singularity has no chance to escape the eventhorizon and is stuck inside [ ] the black hole forever. irmielin. Bin Sci-Fi Fan, doch von diesem Film hatte ich nie etwas gehört. Jimmy v. Event Horizon Anabel Film Am Rande des Universums. Die Story ist gut. Wiedergabe auf diesem Gerät nicht möglich. Hauptdarsteller sind Laurence Fishburne und Sam Neill. Als Download verfügbar. Event Horizon What Is a Quasar? Video
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