Quasar · black hole

TON 618

TON 618 in a Pan-STARRS survey image: just a single point
TON 618 in a Pan-STARRS survey image: just a single point
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TON 618 is an extremely luminous quasar in the constellation Canes Venatici. Its light travelled for about 10.4 billion years – we see it as it was when the universe was a little over 3 billion years old.

At its centre sits one of the most massive known black holes: roughly 40 to 66 billion solar masses depending on the measurement. Its event horizon would have a radius of about 1,300 astronomical units – over forty times Neptune's orbit, big enough to swallow our whole Solar System.

A quasar is the extremely bright core of a young galaxy: gas falls onto the black hole, forms a hot disc and radiates more brightly than hundreds of trillions of Suns.

In the sky TON 618 is just a single faint point (15.9 mag) and needs a large telescope. There is no photograph of the disc or the black hole itself: the pictures in the gallery are artist's impressions and do not show TON 618 itself.

Key facts

Distance (light travel)
≈ 10.4 billion light-years
Redshift
z ≈ 2.22
Black hole mass
≈ 40–66 billion solar masses
Horizon radius
≈ 1,300 AU (Neptune's orbit: 30 AU)
Luminosity
≈ 140 trillion Suns
Brightness
15.9 mag

Images

Artist's impression of a black hole with accretion disc
Artist's impression: Artist's impression of a black hole with accretion disc
Artist's impression of a quasar (ESO) – not TON 618 itself
Artist's impression: Artist's impression of a quasar (ESO) – not TON 618 itself
Artist's impression of a quasar (ESO) – not TON 618 itself
Artist's impression: Artist's impression of a quasar (ESO) – not TON 618 itself

More famous objects

Images: NASA, ESA, ESO, Event Horizon Telescope, Wikimedia Commons. Artist's impressions are labelled as such. Figures from published research, rounded.