TON 618

240 billion kmevent horizon diameter

Updated

240billion km
Visual creditscaleofspace.org / CC BY-NC 4.0

Details

TON 618 is a hyperluminous quasar powered by one of the most massive black holes known. We see it from a far younger universe, and the quasar is so overwhelmingly bright that the galaxy around it is largely lost in the glare.

TON 618 is a distant quasar whose broad emission lines imply a central black-hole mass of about 40.7 billion Suns. The estimate depends on the relation between the quasar’s luminosity, line widths and the unseen gas geometry, so it is less direct than a mass derived from resolved stellar orbits.

Its roughly 240-billion-kilometer event-horizon diameter is calculated from that mass. What telescopes detect is the exceptionally bright accretion flow around the black hole, which overwhelms the light of its host galaxy.

Key facts

Category
Black holes
Object class
Ultramassive black hole
Scale fact
240 billion kmevent horizon diameter
Mass
~40.7 billion solar masses
Embed

Size neighbors

Objects near TON 618 on the scale

On the logarithmic size axis, TON 618 falls between Holm 15A* and Phoenix A*. The band uses nearby Ultramassive black hole records.

Shared physical scale
184billion km
Holm 15A*236 billion km
TON 618240 billion km

Sources

References for TON 618

Measurements and descriptive context are compiled by the Scale of Space team from the references below. If you find an error, please let us know.

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