Quasar · black hole
TON 618

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
.jpg?width=600)
.jpg?width=600)

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