Two X-ray house observatories, NASA's Nuclear spectroscopical Telescope Array (NuSTAR) and therefore the European house Agency's XMM-Newton, have teamed up to live definitively, for the primary time, the spin rate of a part.
The supermassive part lies at the dust- and gas-filled heart of a galaxy referred to as NGC 1365, and it's spinning nearly as quick as Einstein's theory of gravity can permit.
Shikoni Videon