Black holes & exotica

Phoenix A

A black hole possibly 100 billion times the Sun's mass, in a galaxy cluster that refuses to stop making stars

Mass uncertain Artist's impression · drag to rotate
Location centre of the Phoenix Cluster SPT-CL J2344-4243 [1]
Distance about 5.8 billion light-years light-travel distance [1]
Black hole mass up to about 10¹¹ Suns from a model, not measured directly [2]
Alternative estimate about 1.3 × 10¹⁰ Suns [2]
Cluster found 2010 South Pole Telescope [1]
Cluster mass about 2 × 10¹⁵ Suns [1]
Star formation about 740 Suns per year the Milky Way makes about 1 [3]

About the image. Drawn as a cluster of glowing galaxies around a giant central galaxy, with blue filaments of cooling gas flowing into it. The black hole itself is far too small to see at this scale; the arrangement of galaxies is imagined.

In the southern constellation Phoenix, about 5.8 billion light-years away, lies one of the most extreme clusters of galaxies known. It was found in 2010 by the South Pole Telescope, which detected the way its hot gas distorts the cosmic microwave background passing through it. The Phoenix Cluster holds about 2 × 10¹⁵ solar masses, and at its centre is a giant galaxy whose black hole may be the heaviest ever estimated: Phoenix A.

How heavy?

Phoenix A’s mass has never been measured from the orbits of stars or gas around it, the way the masses of black holes such as M87* were. Instead, in 2016 Michael Brockamp and colleagues estimated it from a model that treats the black hole as a “calorimeter”: the energy it must have pumped into the surrounding gas over billions of years implies how much it has grown. Their figure is of the order of 100 billion Suns.

Other estimates come out about eight times lower. Even at the lower figure Phoenix A would be among the most massive black holes known, but the exact number is uncertain, and it should not be treated as a measurement.

A cluster that will not cool quietly

The Phoenix Cluster is remarkable for another reason. In most giant clusters, the central black hole keeps the surrounding hot gas from cooling and forming stars. In 2012 Michael McDonald and colleagues reported that in the Phoenix Cluster gas is cooling at a very high rate and the central galaxy is forming stars at about 740 times the mass of the Sun every year. The Milky Way manages about one.

In 2025 a team led by Michael Reefe used the James Webb Space Telescope to map gas at temperatures of a few hundred thousand degrees in the cluster’s core, catching the gas in the act of cooling for the first time on large scales. The black hole, it seems, cannot quite keep up with the flood of cooling gas around it.

Gallery

A crowded band of golden galaxies with one bright, larger galaxy among them, an impression of the Phoenix Cluster, home of the black hole Phoenix A. AI-generated painting.
A black shadow at the heart of a glowing golden swirl of stars and gas, an impression of the supermassive black hole Phoenix A at the centre of its galaxy. AI-generated painting.
Phoenix A, 3D artist's impression, rendered from the interactive model.
Phoenix A, 3D artist's impression, from another angle, rendered from the interactive model.
Phoenix A, 3D artist's impression, close-up, rendered from the interactive model.

Timeline

  1. 2010 The South Pole Telescope discovers the Phoenix Cluster.
  2. 2012 A record starburst and cooling flow are reported in Nature.
  3. 2016 A model gives Phoenix A a mass of the order of 100 billion Suns.
  4. 2025 JWST maps the cooling gas in the cluster's core.

Questions people ask

Is Phoenix A the biggest black hole?

It may be, but its mass of up to 100 billion Suns comes from a model, not a direct measurement, and other estimates are about eight times lower.

How far away is Phoenix A?

About 5.8 billion light-years, in the constellation Phoenix.

Sources

  1. Wikipedia: Phoenix Cluster
  2. Wikipedia: List of most massive black holes
  3. McDonald et al. (2012), A massive, cooling-flow-induced starburst in the core of a luminous cluster of galaxies, Nature 488
  4. Brockamp et al. (2016), Supermassive black holes as giant calorimeters, A&A 585
  5. Reefe et al. (2025), Directly imaging the cooling flow in the Phoenix cluster, Nature 638