According to a study published Wednesday in the Nature Journal, a distant supermassive quasar black hole is spinning at about 336 million miles (5.4 kilometers) per hour. They left their place, met and swallowed its neighbors. Its spin speed can tell the connection between the black hole itself and his host galaxy. The computer simulation model shows that the black hole's spin depends on a large amount of material for the consumption of the black hole itself.


Scientists have measured the spin rate of black holes before, but they have never been so far. The new measuring black hole is a quasar that is 60 billion light years from Earth. The black hole's space is very congested and its quality is light. Within its range of gravity, no photon can escape its attraction.
Calculated gases are combined by nearby galaxies to obtain a stable source of supply. For example, the rotational speed may be affected by the instability of material consumption or the surrounding galaxies. Astronomer Mark Reynolds of the University of Michigan said that the supermassive quasar black hole RXJ1131-1231 has a stable rotation speed, most likely to consume peripheral galaxies in sections, and consumes approximately 333,000 Earth masses a year. Scientists want to measure the spins of other more distant, supermassive black holes and investigate whether further spin conditions are different.

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