Black hole event horizon

Black hole event horizon

C026/4116 Rights Managed

Request low-res file

530 pixels on longest edge, unwatermarked

Request/Download high-res file

Uncompressed file size: 87.6MB

Downloadable file size: 3.5MB

Price image Pricing

Please login to use the price calculator


Credit: DAVID PARKER/SCIENCE PHOTO LIBRARY

Caption: Conceptual fractal illustration of material falling into a black hole, an object of extreme density, with such strong gravitational attraction that even light cannot escape from their grasp if it comes near enough. The theory of general relativity predicts that a sufficiently compact black hole can deform spacetime. Quantum field theory in curved spacetime predicts that event horizons emit Hawking radiation. Hawking radiation is black body radiation that is predicted to be released by black holes, due to quantum effects near the event horizon. In general relativity, an event horizon is a boundary in spacetime beyond which events cannot affect an outside observer. It is defined as "the point of no return", i.e., the point at which the gravitational pull becomes so great as to make escape impossible. Albert Einstein first predicted black holes in 1916 with his general theory of relativity.

Release details: Model release not required. Property release not required.

Keywords: abstract, albert einstein, astrophysical, astrophysics, big bang, black hole, blackbody, blackbody radiation, computer, cosmology, curved spacetime, early universe, energy, event horizon, explosion, fractal illustration, fractals, general relativity, gravitation, gravity, hawking radiation, illustration, light, mandelbrot set, microscopic black holes, particle physics, physics, quantum, relativity, spacetime, spiral, supersymmetry, susy, theory of relativity, vortex

Licence fees: A licence fee will be charged for any media (low or high resolution) used in your project.