
science & techESA/Hubble
A galaxy's spinning gas disc revealed the mass of its central black hole
NGC 4526 is a lenticular galaxy, a type that sits between spirals and ellipticals, and one of the brightest of its kind. It has a rapidly spinning disc of gas and stars at its centre that moves at more than 250 kilometres per second and reaches far out from the core. Measuring how fast that disc moves allowed astronomers to infer that the supermassive black hole at its centre has about 450 million times the Sun's mass. The method had not been used before to pin down a galaxy's central black hole. The galaxy is part of the Virgo cluster, and it has hosted two known supernovae, in 1969 and 1994.
Gas in the disc orbits the black hole, and its speed depends on how much mass is pulling at the centre. By measuring how fast the gas moves at different distances from the core, astronomers can calculate the mass inside, which is dominated by the black hole.
Black holes are invisible, so their masses have to be inferred from how nearby matter moves. Using a spinning gas disc as a measuring tool gives astronomers a new way to weigh black holes in galaxies that are otherwise hard to study.
