Four quadrants. The upper two hold images of the galaxies NGC 3377 (left) and NGC 3379 (right). The bottom left quadrant holds and image of the galaxy NGC 4486B. The lower-right quadrant shows an expanded view of NGC 4486B's center. Each image holds a bright-yellow core surrounded by more diffuse a yellow, then orange, and later red glow.

Hubble Observes the Centers of Galaxies Looking for Black Holes

Combining images with data from Hubble’s spectrographs, researchers have peered into the center of many galaxies and established the existence of large black holes. These massive black holes surround themselves with luminous stars and gas, which are visible as bright knots. In a census performed by Hubble in the late 1990s, galaxies NGC 3379 and NGC 3377 were found to have black holes that “weighed in” at 50 million and over 100 million solar masses, respectively, and NGC 4486B was revealed to have a double nucleus at its core.

Credits: Karl Gebhardt (University of Michigan), Tod Lauer (NOAO) and NASA