User login

Black Holes

Black hole at a Galaxy centre
Credit: : ESA V. Beckmann (NASA-GSFC)

Black Holes are very strange objects. They are formed when very massive stars come to the end of their lifetime, in a supernova event.

Everything that remains of the star is crushed down into an incredibly small, dense object. Close to the object, gravity is so strong that nothing can get away, not even light. This means that we cannot see anything within that region - hence the name black hole.

Simulation of a black hole distorting
an image of a galaxy
Credit: Alain r, Wikimedia

However, it is possible to see the effects of a black hole on the stars and material around it. Gas, dust and other stars close to a black hole can be sucked in by gravity - a bit like water going down a plughole. As material swirls around the black hole it crashes into each other, producing heat and light. Because this happens away from the black hole, the light can escape so that we can observe the activity.

Black holes can also distort the image of galaxies they pass in front of. The gravity of the black hole will bend the light we receive from the distant galaxy even though it is too far away for any material to be sucked into the black hole. This is called gravitational lensing (see the simulation on the right).

Once established, black holes can grow by consuming material, stars and even other black holes around them. Over time, super-massive black holes can develop, and it is thought that these lurk at the centre of galaxies.

ATTENTION

Please note that over the weekend of the 26-28th May 2017 we will be switching over to our brand new website - during this time there may be periods where the site is difficult to access, and users will be unable to request observations from the telescope. Please bear with us during this time. All should be back up and running by the 29th May 2017.