TON 618 is one of the most massive known black holes, hosted by a distant quasar. It sits at the heart of an active galactic nucleus,
where gas and dust form an extremely luminous accretion flow as material spirals inward.
Type
Supermassive Black Hole (Quasar)
What you’re seeing here
Stylized accretion + polar structures (educational visualization)
Why it matters
A benchmark object for extreme SMBH growth and energetic feedback
Note: This scene is not to physical scale—it's designed to help visitors intuitively explore how rotation and inflow can shape
accretion structures around a supermassive black hole.
