NASA · ESA · Chandra · Hubble — Cosmic Record-Holders

Cosmic
ExtremesFour record-breaking objects

The most massive black hole ever measured. The hottest X-ray cluster. The largest galactic core. The biggest galaxy known. Four objects that push physics to its absolute limits.

⦿ TON 618 ◈ Phoenix Cluster ◎ Holm 15A* ⊞ IC 1101
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66B
M☉
TON 618 black hole
2.5Q
× Sun's mass
Phoenix Cluster total
40B
M☉
Holm 15A* black hole
100T
Stars
IC 1101 galaxy
NASA/JPL-Caltech · Artist's Impression
TON 618 — quasar · 10.4 billion light years · Canes Venatici
01
01
Ultramassive Quasar
TON 618
The most massive black hole directly measured
TON 618 is a hyperluminous, radio-loud quasar located 10.4 billion light-years away in the constellation Canes Venatici. At its core sits one of the most massive black holes ever directly measured, weighing in at 40–66 billion solar masses — so large that its event horizon alone is wider than our entire solar system.

The quasar's accretion disk blazes with the energy of 140 trillion Suns. Gas near the black hole moves at 10,500 km/s. It is surrounded by an enormous Lyman-alpha nebula stretching over 330,000 light-years. First catalogued in 1957 as a "faint blue star," its true nature as a quasar wasn't confirmed until 1970.
Black hole mass
40–66 billion M☉
Distance
10.4 billion ly
Luminosity
140 trillion L☉
Event horizon
Wider than solar system
Gas velocity
10,500 km/s
Nebula span
>330,000 ly
QuasarUltramassive BH AGNLyman-alpha BlobRadio-Loud
Chandra X-ray / Hubble · Composite
Phoenix Cluster SPT-CLJ2344-4243 · 5.7 billion light-years
02
02
Galaxy Cluster · Record-Holder
Phoenix
Cluster
Most X-ray luminous cluster ever discovered
The Phoenix Cluster (SPT-CLJ2344-4243) is located 5.7 billion light-years away in the constellation Phoenix. It holds the record for the most X-ray luminous galaxy cluster ever observed, radiating at 8.2 × 10⁴⁵ erg/s, and features the fastest-known cooling flow — over 3,800 solar masses of hot gas cooling per year.

This runaway cooling fuels an extraordinary starburst at the cluster's heart, forming stars at ~740 solar masses per year — the highest rate ever seen in a cluster core. Its central galaxy hosts a black hole 1,000× more massive than Sagittarius A*, and its total mass may be 2.5 quadrillion times the Sun.
Distance
5.7 billion ly
Total mass
2.5 quadrillion M☉
Cooling rate
3,800 M☉/yr
Star formation
~740 M☉/yr
X-ray luminosity
8.2×10⁴⁵ erg/s
Central BH
1,000× Sgr A*
Galaxy ClusterCooling Flow X-ray RecordStarburst CoreSPT Survey
ESO / VLT · Galaxy Core Observation
Holmberg 15A* — Abell 85 cluster · ~700 million light-years
03
03
Ultramassive Black Hole
Holm 15A*
Largest confirmed black hole by direct stellar dynamics
Holmberg 15A* is the central galaxy of the Abell 85 cluster, located about 700 million light-years away. It hosts one of the largest directly measured black holes: a mass of 40 billion solar masses, confirmed through stellar dynamics — earning it the informal designation "Holm 15A*" (echoing Sgr A*).

Its core is defined by a remarkably flat, depleted stellar density — the largest cored galaxy known — extending 15,000 light-years across. This core is thought to have been excavated by two merging supermassive black holes in the galaxy's past, creating a gravitational slingshot that ejected stars outward. Its velocity dispersion of ~320 km/s hints at an even larger dark matter halo.
Black hole mass
~40 billion M☉
Distance
~700 million ly
Core radius
15,000 ly (largest)
Host cluster
Abell 85
Vel. dispersion
~320 km/s
Core type
Depleted / flat γ=0
Ultramassive BHBCG Galaxy Abell 85Cored GalaxyBH Merger
Hubble Space Telescope · Abell 2029
IC 1101 — Abell 2029 · ~1.07 billion light-years · Virgo
04
04
Supergiant Elliptical Galaxy
IC 1101
One of the largest galaxies ever discovered
IC 1101 is the dominant galaxy of the Abell 2029 cluster, located about 1.07 billion light-years from Earth in Virgo. With a visible diameter of roughly 550,000 light-years and a diffuse stellar halo extending up to 4 million light-years, it is among the largest known galaxies.

Discovered by William Herschel on 19 June 1790, IC 1101 contains an estimated 100 trillion stars — 500× more than our Milky Way. It is a dying galaxy, depleted of star-forming gas by billions of years of collisions. At its centre sits a black hole of 50–100 billion solar masses. If placed at our galaxy's location, IC 1101 would swallow the Andromeda Galaxy and the entire Local Group.
Visible diameter
~550,000 ly
Halo extent
~4 million ly
Stars
~100 trillion
Distance
~1.07 billion ly
Central BH
50–100 billion M☉
Discovered
Herschel, 1790
Giant EllipticalAbell 2029 BCGDying Galaxy100 Trillion Stars