Not exact matches
The project continues to detect waves from similar
events, offering new and incredible details about what happens when these
black holes crash and warp the spacetime
around them.
Meanwhile a project called the
Event Horizon Telescope aims to use radio observatories scattered
around Earth to image the supermassive
black hole at the center of the Milky Way.
The
event horizon is the sphere
around a
black hole from inside which nothing can escape its clutches.
Ordinarily, they don't stick
around long enough to be directly observed, but if a pair straddles the
event horizon, then one photon can fall into the
black hole, while the other escapes, carrying energy away as Hawking radiation.
This particular energy range offers astronomers a detailed look at what is happening near the
event horizon, the region
around a
black hole from which light can no longer escape gravity's grasp.
Based on data taken by NASA's Chandra X-ray Observatory, the model takes into account how energy flows between two regions
around the
black hole — an inner core close to the boundary beyond which light can not escape (the
event horizon) and an outer ring that extends far out and includes the massive young stars lurking near the
black hole.
This could allow scientists to peer into some of the more mysterious features of the cosmos, including
event horizons — gravitational points of no return
around black holes — and the blazing particle jets erupting from them.
«Our motive is not so much to establish that there is a hard surface,» Kumar said, «but to push the boundary of knowledge and find concrete evidence that really, there is an
event horizon
around black holes.»
Discovering that it was possible to take energy quickly out of a
black hole would be problematic for our understanding of how matter behaves
around the
event horizon.
By some estimates, the telescope could be used to image near the
black hole's
event horizon — the boundary
around which nothing can escape the
black hole's gravity.
They hope to find tiny stutters in these natural clocks caused by the gravitational wake of a massive
event, such as a
black hole in orbit
around another star.
The team plans to make an image of the
event horizon — the border
around a
black hole which light can enter, but not leave.
The team led by three principal investigators, Heino Falcke, Radboud University Nijmegen, Michael Kramer, Max - Planck - Institut für Radioastronomie, and Luciano Rezzolla, Goethe University in Frankfurt and Max - Planck - Institut für Gravitationsphysik, Potsdam, hopes to measure the shadow cast by the
event horizon of the
black hole in the center of the Milky Way, find new radiopulsars near this
black hole, and combine these measurements with advanced computer simulations of the behaviour of light and matter
around black holes as predicted by theories of gravity.
The image shall reveal the «shadow» of the
event horizon — the «one - way» membrane
around a
black hole that defines the boundary surrounding
black holes, through which light can enter, but never leave.
We used to think we might have a way
around it at the
event horizons of
black holes, but that turned out to be false.