The most massive black holes
TOP 23The largest black hole in this catalogue is TON 618, at 6.6×10¹⁰ M☉. Next are S5 0014+81 and SMSS J2157-3602.
Supermassive black holes sit at the centres of galaxies and scale with them: the bigger the galaxy, the bigger the hole. The largest here are billions of times the mass of the Sun, and the very heaviest have horizons wider than the whole planetary Solar System.
NAME
CLASS
MASS
DISTANCE
MAG
CONSTELLATION
TON 618★
Quasar
6.6×10¹⁰ M☉
56.78 Gly
—
Canes Venatici
S5 0014+81
Quasar
4×10¹⁰ M☉
94.16 Gly
—
Cepheus
SMSS J2157-3602
Quasar
3.4×10¹⁰ M☉
138.0 Gly
—
Piscis Austrinus
SDSS J0100+2802
Quasar
1.2×10¹⁰ M☉
196.9 Gly
—
Pisces
M87*★
Supermassive black hole
6.5×10⁹ M☉
53.50 Mly
—
Virgo
NGC 1277*
Supermassive black hole
4.9×10⁹ M☉
220.0 Mly
—
Perseus
SDSS J1148+5251
Quasar
3×10⁹ M☉
202.2 Gly
—
Ursa Major
ULAS J1120+0641
Quasar
2×10⁹ M☉
224.4 Gly
—
Leo
J0313-1806★
Quasar
1.6×10⁹ M☉
244.8 Gly
—
Eridanus
Pōniuāʻena
Quasar
1.5×10⁹ M☉
206.3 Gly
—
Pegasus
3C 273*★
Quasar
8.86×10⁸ M☉
2.451 Gly
—
Virgo
ULAS J1342+0928
Quasar
7.8×10⁸ M☉
241.1 Gly
—
Boötes
Sagittarius A*★
Supermassive black hole
4.3×10⁶ M☉
26 996 ly
—
Sagittarius
HLX-1
Intermediate-mass black hole
2×10⁴ M☉
290.0 Mly
—
Phoenix
ω Centauri IMBH
Intermediate-mass black hole
8200.00 M☉
17 700 ly
—
Centaurus
GW150914 remnant★
Stellar-mass black hole
62.00 M☉
1.300 Gly
—
—
Gaia BH3★
Stellar-mass black hole
32.70 M☉
1926 ly
—
Aquila
Cygnus X-1★
Stellar-mass black hole
21.20 M☉
7240 ly
—
Cygnus
GRS 1915+105★
Stellar-mass black hole
12.40 M☉
28 000 ly
—
Aquila
Gaia BH1★
Stellar-mass black hole
9.60 M☉
1560 ly
—
Ophiuchus
V404 Cygni
Stellar-mass black hole
9.00 M☉
7800 ly
—
Cygnus
A0620-00
Stellar-mass black hole
6.60 M☉
3300 ly
—
Monoceros
GW170817 remnant★
Stellar-mass black hole
2.70 M☉
130.0 Mly
—
Hydra
[
COMMON QUESTIONS
] 8 ANSWERED- How heavy do they get?
- The largest weighed so far run to tens of billions of solar masses, and they sit at the centres of the largest elliptical galaxies. That is around ten thousand times the mass of the hole at the centre of the Milky Way.
- Does more mass mean a bigger object?
- Yes, and in the simplest possible way: the horizon radius is proportional to the mass. Doubling the mass doubles the radius, so the heaviest holes here are wider than the orbit of Neptune while still being, in every other respect, the same shape as the lightest.
- How is a mass measured at that distance?
- By watching something else move. The orbit of a companion star, the speed of gas near the centre of a galaxy, or the waveform of a merger all fix the mass at the focus — nothing here is weighed directly, and every figure is the output of a model fitted to motion.
- How firm is the order?
- Less firm than a ranked list looks. Mass estimates for the heaviest objects carry uncertainties of tens of per cent, and two adjacent rows are often the same mass as far as the measurements can tell. The object's own page carries the error bar.
- Why are some black holes missing?
- Because no mass has been published for them. A mass needs a dynamical measurement, which needs something to watch, and most catalogued objects have never had one.
- Is there an upper limit?
- There appears to be one around fifty billion solar masses. Above roughly that, a disc of infalling gas fragments into stars instead of feeding the hole, so growth by accretion stalls — a hole can still gain mass by merging with another.
- How is such a mass measured?
- From the motion of what is nearby: individual stars where the galaxy is close enough to resolve them, otherwise the width of emission lines from gas orbiting the centre. Both are model-dependent, which is why the published figures for one object can differ by a factor of two.
- Is the biggest black hole the biggest thing in the universe?
- Not by size. The heaviest known are a couple of thousand astronomical units across — wider than the planetary part of the Solar System, and still millions of times smaller than the galaxy each one sits at the centre of. What a black hole holds is mass, not volume.