Framed Print of Illustration of a supermassive black hole at the core of a young, star-rich galaxy

This artists conception illustrates one of the most primitive supermassive black holes known, at the core of a young, star-rich galaxy. The monstrous black holes are among the most distant known, and appear to be in the very earliest stages of formation, earlier than any observed so far. Unlike all other supermassive black holes probed to date, this primitive duo, called J0005-0006 and J0303-0019, lacks dust. As the illustration shows, gas swirls around a black hole in what is called an accretion disk. Usually, the accretion disk is surrounded by a dark doughnut-like dusty structure called a dust torus. But for the primitive black holes, the dust tori are missing and only gas disks are observed. This is because the early universe was clean as a whistle. Enough time had not passed for molecules to clump together into dust particles. Some black holes forming in this era thus started out lacking dust. As they grew, gobbling up more and more mass, they are thought to have accumulated dusty rings. This illustration also shows how supermassive black holes can distort space and light around them (see warped stars behind black hole). Stars from the galaxy can be seen sprinkled throughout, and distant mergers between other galaxies are illustrated in the background. Stocktrek Images specializes in Astronomy, Dinosaurs, Medical, Military Forces, Ocean Life, & Sci-Fi. © Stocktrek Images

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Media ID 13063105

Accretion Discs Astrophysics Black Holes Center Circumstellar Disks Core Cosmic Event Horizon Formation Galactic Galaxy Nucleus Planetesimal Protoplanetary Disks Quasar Radiant Spacetime Supermassive Black Holes Vibrant