Introduction
Figure 1: Artist's
illustration of Sagittarius A*, the supermassive black hole at the center of
the Milky Way. The rendering highlights the surrounding accretion disk of hot
gas, gravitational light-bending effects, and energetic flaring hotspots
recently observed by the James Webb Space Telescope. Credit: Illustration -
NASA, ESA, CSA, Ralf Crawford (STScI)
The
Cosmic Window is a series dedicated to the
systematic exploration of astrophysical phenomena and cosmic objects - bridging
the frontier of observational astronomy with accessible scientific inquiry, one
chapter at a time.
Imagine a void so massive that an entire
Solar System would vanish inside it without a trace - a place where time itself
slows to a crawl and even light, the fastest thing in the universe, cannot
escape. These are not science fiction. They exist, they are real, and some of
them have been growing for over 13 billion years.
Black holes form when gravity wins its
ultimate battle. When a sufficiently massive star exhausts its nuclear fuel, no
outward pressure can resist the inward crush. The star implodes, forging a
singularity - a point of extreme density - wrapped in an event horizon, the invisible boundary beyond which nothing returns.
Supermassive black holes grow further by consuming gas, dust, and entire stars
across cosmic time. Our own Milky Way's central black hole, Sagittarius A*, weighs roughly 4
million solar masses - colossal by human reckoning, yet reduced to an
insignificant footnote by the five monsters below. Brace yourself: the numbers
that follow challenge the limits of imagination.
1. TON 618: ~66 Billion Solar Masses
Figure 2: Circled here is the supermassive
black hole TON 618, whose light has traveled over 10 billion years across
cosmic time to reach Earth. Credit: SDSS
Located ~10.4 billion light-years away in
Canes Venatici, TON 618 is a
hyperluminous quasar - its central black hole consuming surrounding matter so
voraciously that it outshines approximately 140 trillion Suns combined. Its mass of ~66 billion solar masses
gives it a Schwarzschild radius of roughly 1,300
AU, wider than our entire Solar System. Placed at the Sun's position, its
event horizon would engulf every planet out to well beyond Neptune.
Specialty:
The most massive black hole with a confirmed direct mass measurement (via
reverberation mapping). Its luminosity alone makes it visible from nearly the
edge of the observable universe - a beacon from a time when the cosmos was just
3 billion years old.
2. Holm 15A*: ~40 Billion Solar Masses
At the heart of elliptical galaxy Holm 15A, ~700 million light-years away
in the Abell 85 cluster, sits a black hole of ~40 billion solar masses. The surrounding stellar core is strikingly
faint and diffuse - a so-called core
deficit - caused by gravitational slingshot events as two massive black
holes spiralled inward over billions of years, ejecting stars outward as they
merged.
Specialty:
The largest directly measured black hole in the local universe, and its
ultra-depleted stellar core serves as fossilised evidence of a colossal black
hole merger - making it a unique laboratory for studying the final parsec
problem in astrophysics.
3. Abell 1201 BCG: ~32.7 Billion Solar Masses
~2.4 billion light-years away, the
brightest cluster galaxy of Abell 1201
hides a black hole of ~32.7 billion
solar masses - detected not by watching stars orbit, but by observing a
distant background galaxy whose light was bent and stretched into a luminous
arc as it passed this galaxy: strong
gravitational lensing.
Specialty:
The first ultramassive black hole of this scale discovered purely through
gravitational lensing (Nightingale et al., 2023). This technique does not
require resolving individual stellar orbits, meaning dozens of similarly
massive, previously invisible black holes may now be within reach of discovery
across the sky.
4. NGC 4889: ~21 Billion Solar Masses
The dominant galaxy of the Coma Cluster, ~320 million light-years
away, hosts a black hole with an estimated mass of roughly 21 billion solar masses under its highest-orbital-model scenario
(the observational range spans 6–37 billion M☉).
Its event horizon extends approximately 130
billion kilometres - about ten times the Sun-to-Pluto distance. Notably,
despite this immense scale, NGC 4889's black hole appears largely dormant today, no longer actively
accreting.
Specialty:
An early benchmark in ultramassive black hole science; its quiescent state
offers a rare window into the "quiet phase" of these giants after
billions of years of feeding - a glimpse of what TON 618 may one day become.
5. NGC 1600: ~17 Billion Solar Masses
Located ~200 million light-years away in
the constellation Eridanus, NGC 1600
hosts a black hole of ~17 billion solar
masses - yet it sits in a sparse, unremarkable galaxy group, not the rich
cluster environment typically associated with black holes of this scale.
Specialty:
Its existence fundamentally challenged models of black hole growth, suggesting
ultramassive black holes may be far more common - quietly lurking in ordinary
environments all across the cosmos, waiting to be found.
Comparison at a Glance
|
Black Hole |
Est. Mass |
Distance |
Host Environment |
Mass vs. Our Sun |
|
TON 618 |
~66 billion M☉ |
10.4 billion ly |
Quasar host |
66,000,000,000× |
|
Holm 15A* |
~40 billion M☉ |
~700 million ly |
Rich galaxy cluster |
40,000,000,000× |
|
Abell 1201 BCG |
~32.7 billion M☉ |
~2.4 billion ly |
BCG elliptical |
32,700,000,000× |
|
NGC 4889 |
~6–37 billion M☉† |
~320 million ly |
Rich galaxy cluster |
up to 37,000,000,000× |
|
NGC 1600 |
~17 billion M☉ |
~200 million ly |
Sparse galaxy group |
17,000,000,000× |
|
Sgr A* (Milky Way) |
~4 million M☉ |
~26,000 ly |
Spiral galaxy |
4,000,000× |
M☉
= solar masses. ly = light-years.
†NGC 4889 has a wide observational
uncertainty; ~21 billion M☉ reflects the tangentially-biased
orbital model (McConnell et al., 2011).
Video 1: Sizing Up the Universe’s Biggest Black Holes: A visual scale comparison tracking black holes from 100,000 solar masses up to TON 618’s staggering 66 billion solar masses, set against the orbital scale of our own Solar System. Credit: NASA Animation Sizes Up the Biggest Black Holes via NASA Goddard
Conclusion
These five black holes stand at the
outermost frontier of known mass - each billions of times heavier than our Sun,
making even our galaxy's own central black hole look negligible. Yet this
ranking is almost certainly provisional. Gravitational lensing surveys, the
Event Horizon Telescope, and upcoming missions such as LISA (Laser Interferometer
Space Antenna) are uncovering candidates at an accelerating pace. This list will be updated - and likely
overturned - as new discoveries arrive almost daily. The true upper limit
of black hole mass remains one of the most tantalising open questions in all of
science. The Cosmic Window series
will continue to chart these frontiers - turning next to other extraordinary
classes of objects that populate our universe.


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