From tech to household and wellness products. This Time in History In these videos, find out what happened this month (or any month!) in history.#WTFact Videos In #WTFact Britannica shares some of the most bizarre facts we can find.Demystified Videos In Demystified, Britannica has all the answers to your burning questions.Britannica Explains In these videos, Britannica explains a variety of topics and answers frequently asked questions.Britannica Classics Check out these retro videos from Encyclopedia Britannica’s archives.“Does it have any profound significance? I don’t know,” says Hamilton. But whether it hints that a 2D view is more fundamental is not yet clear. “Close to the singularity, it appears that the entire three-dimensional universe is being crushed into a two-dimensional surface,” says Hamilton (see Our world may be a giant hologram). That’s where visualisations like this might just help. Somehow, different points in space seem to share the same states – but it’s not clear how. But along with other theorists, they suspect that this usual assumption, called locality, doesn’t work inside a black hole. To calculate total entropy, Hamilton and Polhemus assumed that you add up all the possible states that matter and energy could take at different points in space. The problem may be that we have a naive view of space, which breaks down inside the black hole. This is like a supercharged version of the old black hole information paradox, which pits the apparent destruction of objects – and information – that falls into a black hole against quantum mechanics, which states that quantum information can never be lost. Quantum calculations seem to show that there is too much complexity within a black hole – in earlier work, the researchers calculated that it should be possible to create much more entropy (a measure of disorder) inside the black hole than is measured by outside observers. This process might shed some light on a black hole puzzle. Eventually it gets red-shifted into nothingness, so your whole view will be squeezed into a horizontal ring. That would pull a real observer apart, and it also affects the light falling in around you – light from above your head is stretched out and shifted to the red end of the spectrum. If you’re falling in feet first, gravity at your head is much weaker than at your feet. So close to the centre of the black hole, you feel powerful tidal forces. The strangest sight is reserved for your last moments. The white grid that loops around you marks where distant observers would place the horizon – this is where you’d see other people falling in if they followed you through the horizon. And as you pass one Schwartzschild radius, another artificial visual aid pops up. Hamilton and Polhemus have painted a red grid on the horizon to help visualise it (as the horizon is spherical, the two circles on the grid represent the north and south “poles” of its central black hole). Even after you cross this radius, there is still a point in front of you where all light is swallowed, so from your point of view, you never reach the horizon. To distant observers, the horizon has a size of one Schwartzschild radius – about 15 million kilometres for this hole – but as you approach, it recedes from you. Light from stars directly behind the hole is swallowed by the horizon, while light from other stars is merely bent by the black hole’s gravity, forming a warped image around the hole. They follow the fate of an imaginary observer on an orbit that swoops down into a giant black hole weighing 5 million times the mass of the sun, about the same size as the hole in the centre of our galaxy.Īs you approach, a dark circle is bitten out of the galaxy containing the black hole, marking the event horizon – the point beyond which nothing can escape the black hole’s grip.
#JOUR EY INTO A BLACK HOLE CODE#
The research could help physicists understand the apparently paradoxical fate of matter and energy in a black hole.Īndrew Hamilton and Gavin Polhemus of the University of Colorado, Boulder, built a computer code based on the equations of Einstein’s general theory of relativity, which describes gravity as a distortion of space and time. A new simulation shows what you might see on your way towards the black hole’s crushing central singularity. Video: Falling into a black hole would be a one-off sightseeing trip, so this simulation, calculated by Andrew Hamilton and his team at the University of Colorado, Boulder, is a safer optionįalling into a black hole might not be good for your health, but at least the view would be fine.
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