Image of spiral galaxy ngc 4845, a flat and dust-mottled reddish-brown disk surrounding a bright orange galactic bulge.

NGC 4845

NGC 4845’s glowing center hosts a gigantic version of a black hole, known as a supermassive black hole. The presence of a black hole in a distant galaxy like this one can be inferred from its effect on the galaxy’s innermost stars; these stars experience a strong gravitational pull from the black hole and whizz around the galaxy’s center much faster than otherwise. From investigating the motion of these central stars, astronomers can estimate the mass of the central black hole; for NGC 4845 this is estimated to be hundreds of thousands times heavier than the sun. From investigating the motion of these central stars, astronomers can estimate the mass of the central black hole — for NGC 4845 this is estimated to be hundreds of thousands times heavier than the sun.

Credits: ESA/Hubble & NASA and S. Smartt (Queen's University Belfast)