The nearest black holes to Earth
TOP 25The nearest black hole in this catalogue is Gaia BH1, 1560 ly away. Next are Gaia BH3 and A0620-00.
Every black hole here is far enough away to be harmless and close enough to study. The nearest ones were found the same way the first ones were — by watching a star orbit something that gives off no light.
NAME
CLASS
MASS
DISTANCE
MAG
CONSTELLATION
Gaia BH1★
Stellar-mass black hole
9.60 M☉
1560 ly
—
Ophiuchus
Gaia BH3★
Stellar-mass black hole
32.70 M☉
1926 ly
—
Aquila
A0620-00
Stellar-mass black hole
6.60 M☉
3300 ly
—
Monoceros
Cygnus X-1★
Stellar-mass black hole
21.20 M☉
7240 ly
—
Cygnus
V404 Cygni
Stellar-mass black hole
9.00 M☉
7800 ly
—
Cygnus
ω Centauri IMBH
Intermediate-mass black hole
8200.00 M☉
17 700 ly
—
Centaurus
Sagittarius A*★
Supermassive black hole
4.3×10⁶ M☉
26 996 ly
—
Sagittarius
GRS 1915+105★
Stellar-mass black hole
12.40 M☉
28 000 ly
—
Aquila
M87*★
Supermassive black hole
6.5×10⁹ M☉
53.50 Mly
—
Virgo
GW170817 remnant★
Stellar-mass black hole
2.70 M☉
130.0 Mly
—
Hydra
NGC 1277*
Supermassive black hole
4.9×10⁹ M☉
220.0 Mly
—
Perseus
HLX-1
Intermediate-mass black hole
2×10⁴ M☉
290.0 Mly
—
Phoenix
Markarian 231
Quasar
—
607.9 Mly
—
Ursa Major
GW150914 remnant★
Stellar-mass black hole
62.00 M☉
1.300 Gly
—
—
3C 273*★
Quasar
8.86×10⁸ M☉
2.451 Gly
—
Virgo
PDS 456
Quasar
—
2.907 Gly
—
Serpens
PHL 1811
Quasar
—
3.009 Gly
—
Capricornus
PG 1302-102
Quasar
—
4.633 Gly
—
Virgo
H1821+643
Quasar
—
4.990 Gly
—
Draco
3C 48
Quasar
—
6.442 Gly
—
Triangulum
4C +21.35
Quasar
—
7.725 Gly
—
Coma Berenices
3C 279
Quasar
—
9.977 Gly
—
Virgo
3C 147
Quasar
—
10.30 Gly
—
Auriga
3C 345
Quasar
—
11.28 Gly
—
Hercules
PKS 0637-752
Quasar
—
12.71 Gly
—
Mensa
[
COMMON QUESTIONS
] 8 ANSWERED- How close is close?
- Not close in any sense that matters. The nearest known black hole is thousands of light years away, which is far enough that its gravity has no measurable effect here and near enough that its companion star can be watched from the ground.
- How is a nearby one found?
- By the star going round it. A visible star on an orbit whose other focus holds nothing luminous gives away both the presence and the mass of the dark companion, and that is how the closest ones on this list were identified.
- How is the distance measured?
- By parallax where the object is near enough — the shift in its apparent position as the Earth crosses its orbit, which is geometry and needs no assumptions. Beyond that, distance is inferred from how bright something of known luminosity appears, and the further out the ladder goes the more the uncertainty grows.
- How firm is the order?
- Firmer at the top than at the bottom. Neighbouring rows often sit inside each other's error bars, so a swap between two adjacent entries is a revision rather than a correction. Each object's own page carries the figure with its uncertainty and the method it came from.
- Why are some black holes missing?
- Because this catalogue holds no distance for them. A row with an empty distance column cannot be ranked on it, so the list is the nearest of those measured rather than the nearest that exist.
- Could the nearest black hole ever reach us?
- No. It is bound to the galaxy on its own orbit, thousands of light years away, and nothing about a black hole makes it move towards anything — it falls the way any mass falls. At that separation its gravitational pull on the Solar System is smaller than that of many ordinary stars.
- Are there closer ones nobody has found?
- Almost certainly. A black hole with no companion to disturb and no gas to swallow gives off nothing at all, and the models suggest the galaxy holds a hundred million of them. Only the ones doing something detectable are on any list.
- Why do the distances change between publications?
- Because they are inferred from the companion star, and a revision to the star's distance or mass moves the black hole with it. Several entries here have shifted by tens of per cent since they were announced.