List of voids

This is a list of voids in astronomy. Voids are particularly galaxy-poor regions of space between filaments, making up the large-scale structure of the universe. Some voids are known as supervoids.

In the tables, z is the cosmological redshift, c the speed of light, and h the dimensionless Hubble parameter, which has a value of approximately 0.7 (the Hubble constant H0 = h × 100 km s−1 Mpc−1). Mpc stands for megaparsec.

The co-ordinates (right ascension and declination) and distance given refer to the approximate center of the region.

Voids and supervoids

Largest voids

Named voids

Name	Coordinates	Distance	Diameter	Notes
Local Void	18h 38m +18°	cz=2500 km/s	60 Mpc
Northern Local Supervoid		61 Mpc	104 Mpc	Virgo Supercluster, Coma Supercluster, Perseus–Pisces Supercluster, Ursa Major–Lynx Supercluster, Hydra–Centaurus Supercluster, Sculptor Supercluster, Pavo–Corona Australes Supercluster form a sheet between the Northern Local Supervoid and the Southern Local Supervoid. The Hercules Supercluster separates the Northern Local Void from the Boötes Void. The Perseus–Pisces Supercluster and Pegasus Supercluster form a sheet separating the Northern Local Void and Southern Local Void from the Pegasus Void.
Southern Local Supervoid		96 Mpc	112 Mpc
Giant Void	13h 01m +38.7°	z=0.116	300–400 Mpc	"Giant Void in NGH" or "AR-Lp 36"; NGH stands for "Northern Galactic Hemisphere"; discovered in 1988. It is the largest void in the NGH where z<0.14.
KBC Void			600 Mpc	Void containing the Milky Way and Local Group

Voids designated by their constellation

Name	Coordinates	Distance	Diameter	Notes
Boötes Void (Great Void)	14h 20m 26°	150 Mpc	100 Mpc	The Hercules Supercluster separates the Northern Local Void from the Boötes Void. The Hercules Supercluster thus forms part of the near edge of the Boötes Void.
Canis Major Void
Columba Void
Coma Void				Discovered in 1975, along with the Coma Supercluster, it lies in front of the Coma Cluster. It was the first void to be discovered and is approximately 1/3 as far away as the much larger Boötes Void.
Corona Borealis Void
Eridanus Void				This void is separated from the Sculptor void by a sheet of galaxies.
Eridanus Supervoid (Great Void)	03h 15m 05s −19° 35′ 02″	z=1	150 Mpc	The claimed Eridanus Supervoid or "Great Void", reported on 24 August 2007 by the NRAO from Very Large Array Sky Survey data. This void, if real, would be much larger than the others listed here (except the Giant Void), about 300 h−1 Mpc in diameter and 1800–3000 h−1 Mpc distant (where h is the dimensionless Hubble parameter). It would be associated with (and be the explanation of) a cold spot in the cosmic microwave background at the sky location. The evidence for such a "Great Void" is disputed by Smith and Huterer. They showed that the claims made of observational evidence for such a void from survey data neglected systematic effects and did not account for a posteriori choices made in analyzing data.
Southern Eridanus Void				The Southern Eridanus void is connected to the Eridanus void by a hole in the distribution of galaxies separating the two. A hole in the distribution of galaxies separating Sculptor and Southern Eridanus voids the size of (redshift) 1250 km/s appears to exist.
Fornax Void
Hercules Void	15.5h +30°	cz=7000 km/s		Discovered in 1979
Hydra Void				The Hydra Void lies beyond the Hydra–Centaurus Supercluster
Leo Void	11h 30m 0°	cz=4000 km/s
Microscopium Void				A hole in the distribution of galaxies separating Sculptor and Microscopium voids the size of (redshift) 1250 km/s appears to exist. This is roughly 1/2 of Microscopium's diameter.
Ophiuchus Void	near 17h −25°	< 5000 km/s (the outer limit)		25% of average universe density is the void density of matter. The far end of this void is defined by the Ophiuchus Supercluster.
Pegasus Void	22h +15°	cz=5500 km/s	40 Mpc	The Perseus–Pisces Supercluster and Pegasus Supercluster form a sheet separate the Northern Local Void and Southern Local Void from the Pegasus Void.
Perseus–Pisces Void	1h +10°	cz=8000 km/s		Discovered in 1980, it is also called the Perseus Void
Sagittarius Void
Sculptor Void	23h 48m −24° 39′		34.8 Mpc/h	Corresponds to SRSS1 Void 3 and SRSS2 Void 5 This void is separated from the Eridanus Void by a sheet of galaxies. A hole in the distribution of galaxies separating Sculptor and Southern Eridanus Voids the size of 1250 km/s appears to exist. The Sculptor Void lies next to the Southern Wall or Southern Great Wall.
Taurus Void			30 Mpc	The Taurus Void appears large and circular, and has walls of galaxies surrounding it. It lies next to the Perseus–Pisces Supercluster, and is the most visually identifiable. Several galaxies have been found to reside in the void, such as UGC 2627 and UGC 2629, both approximately 185 million light years away.

Other voids

Designation	Location	Coordinates	Distance	Diameter	Dimensions	Notes
Bahcall & Soneira 1982 void	z = 0.03 – 0.08				150 h−1 Mpc deep 300 h−1 Mpc wide 60 h−1 Mpc tall	This suspected void ranged 100 degrees across the sky, and has shown up on other surveys as several separate voids.

Voids by search or survey

Tully list

In 1985, Tully determined a local dominant supercluster plane, and found the Pisces–Cetus Supercluster Complex.

#	Coordinates	Distance	Diameter	Notes
(h−1 Mpc)
1	17.0h 80°	90	140
2	21.0h −7°	100	136
3	8.6h +13°	150	150
4	21.5h +5°	170	173
5	14.3h +52°	180	158	Boötes Void
6	23.0h −16°	190	171
7	12.8h +14°	190	174
8	10.0h +35°	250	170
9	2.6h −11°	280	229
10	8.7h +58°	310	243
11	16.8h +5°	310	270

B&B Abell-derived list

In a 1985 study of Abell clusters, 29 voids were determined, in the sphere z<0.1 around Earth.

#	Coordinates	Distance	Diameter	Notes
(h−1 Mpc)
1	0.0h +20°	293	100
2	0.3h 0°	276	100
3	0.7h +10°	284	100
4	2.0h −13°	275	150
5	8.0h +60°	300	100
6	9.0h +18°	220	100
7	9.0h +67°	180	120
8	9.2h +26°	137	140
9	9.5h +45°	262	200
10	9.8h 0°	285	110
11	9.8h +35°	219	110
12	10.8h −10°	293	120
13	12.0h +14°	206	110
14	12.3h 0°	276	100
15	12.4h −12°	272	150
16	12.5h +32°	237	100
17	12.9h +64°	105	110
18	13.6h +35°	154	200	Boötes Void
19	13.8h +20°	297	110
20	14.2h −4°	265	210
21	14.7h +70°	283	160
22	15.2h +42°	286	140
23	16.0h +7°	295	110
24	16.4h +41°	291	130
25	16.5h +59°	110	100
26	17.2h +58°	237	100
27	22.2h −2°	155	130
28	22.5h 5°	284	160
29	23.5h −7°	203	120

SSRS1 list

A redshift survey of galaxies in the southern sky in 1988, out to a distance of 120 Mpc/h, revealed some voids.

#	Coordinates	Distance (V)	Dimensions W × H × D (h−1 Mpc)	Constellation	Notes
1	1.5h −50°	3000 km/s	30 × 30 × 40	Phoenix/Eridanus	Located just behind the galaxy concentration in Eridanus-Fornax-Dorado
2	21h −25°	5000 km/s	30 × 30 × 30	Capricornus/Microscopium
3	23.5h −35°	6000 km/s	70 × 30 × 50	Sculptor/Grus
4	4h −40°	9000 km/s	50 × 100 × 50	Horologium/Eridanus

SSRS2 list

In 1994, a redshift survey in the southern sky identified 18 voids, 11 of which are major voids.

#	Coordinates	Distance (r)	Diameter (h−1 Mpc)	Constellation	Notes
1	1h 33m −16° 45′	85.7	54.3	Cetus	major void
2	3h 34m −28° 50′	99.7	56.2	Fornax	major void SRSS1 Void 4
3	22h 25m −14° 46′	107.2	60.8	Aquarius	major void
4	21h 43m −14° 40′	66.7	35.6	Capricornus	major void
5	23h 48m −24° 39′	53.0	34.8	Aquarius/Sculptor	major void SRSS1 Void 3 (Sculptor Void)
6	3h 56m −20° 11′	56.5	32.0	Eridanus	major void
7	3h 17m −11° 40′	77.2	25.5	Eridanus	major void
8	23h 20m −12° 32′	83.9	27.8	Aquarius	major void
9	3h 06m −13° 47′	114.6	39.0	Eridanus	major void
10	0h 26m −9° 17′	104.7	34.8	Cetus	major void
11	0h 21m −29° 43′	112.8	42.9	Sculptor	major void
12	23h 03m −32° 35′	74.8	25.0	Piscis Austrinus/Sculptor
13	1h 23m −19° 36′	31.0	22.1	Cetus	SRSS1 Void 1
14	21h 28m −29° 28′	87.2	21.3	Piscis Austrinus/Microscopium
15	21h 24m −33° 17′	116.1	27.3	Microscopium
16	21h 43m −18° 41′	36.5	20.3	Capricornus
17	3h 42m −21° 21′	32.1	19.0	Eridanus
18	4h 18m −8° 42′	85.9	21.1	Eridanus

1994 EEDTA Whole Sky Survey

A 1994 census lists a total of 27 supervoids within a cube of 740 Mpc a side, centered on us (z=0.1 distant sphere).

#	Coordinates (B1950.0)	Distance (Mpc/h)	Diameter (Mpc/h)	Notes
1	19.0° −57.1°	134	88
2	28.2° −12.3°	207	96
3	34.8° −61.9°	216	72
4	36.6° −33.5°	241	86
5	37.8° −36.1°	129	92
6	46.0° −21.4°	236	72
7	62.0° −8.0°	248	100
8	71.2° −38.3°	201	76
9	121.7° −1.5°	96	112	Southern Local Supervoid
10	130.0° +49.3°	246	144
11	140.4° +10.5°	160	92
12	146.9° +27.4°	227	106
13	153.1° −11.4°	246	94
14	159.9° +1.2°	167	68
15	161.6° −32.2°	241	98
16	167.4° +22.8°	222	74
17	186.9° −15.6°	216	94
18	196.8° +9.5°	119	102
19	204.8° +35.7°	119	108
20	214.6° +13.6°	216	78	Boötes Void (Great Void)
21	216.7° +56.5°	143	116
22	219.8° +57.9°	246	96
23	220.2° +33.9°	219	72
24	256.1° −4.8°	61	104	Northern Local Supervoid
25	353.0° −59.4°	198	74
26	356.6° +22.2°	246	80
27	358.9° −33.1°	241	70

Galactic Anti-Center IRAS search

In a 1995 study of IRAS data looking for large-scale structure in the Galactic Anticenter in the Zone of Avoidance, four voids were discovered.

#	Coordinates (B1950.0)	Distance (km/s)	Dimensions	Notes
V0	5.2h +18°	1000	96°×36°×2000 km/s
V1	3.5h +18°	3750	15°×36°×3500 km/s	V1 and V2 are connected, and block the Perseus–Pisces Supercluster from traversing the Zone of Avoidance.
V2	3.5h +29°	8000	25°×14°×2000 km/s	V1 and V2 are connected, and block the Perseus–Pisces Supercluster from traversing the Zone of Avoidance.
V3	8.0h +10°	7000	30°×20°×2000 km/s	This void lies in front of the CfA2 Great Wall.

IRAS list

Analysis of the IRAS redshift survey in 1997 revealed 24 voids, 12 of which were termed "significant"

#	Supergalactic Coordinates (r,X,Y,Z)	Diameter (h−1 Mpc)	Notes
1	(55.2,−10.4,−53.8,6.1)	51.0	significant void
2	(49.6,−25.3,31.4,−28.9)	43.8	significant void
3	(46.0,−24.8,26.7,28.1)	44.5	significant void
4	(46.5,8.7,24.7,38.4)	45.0	significant void (Local Void)
5	(32.0,−13.0,−23.9,−16.9)	36.0	significant void
6	(51.5,17.0,−32.2,36.4)	41.4	significant void
7	(57.1,31.2,44.9,16.5)	43.5	significant void
8	(60.4,−25.8,−22.7,−49.7)	39.5	significant void
9	(49.8,35.9,−25.6,−23.0)	36.0	significant void
10	(63.3,−48.0,−40.9,6.0)	33.6	significant void (Sculptor Void)
11	(48.6,11.8,46.6,−6.9)	32.0	significant void
12	(49.9,−15.6,−35.7,31.3)	31.5	significant void
13	(62.8,14.2,29.3,−53.7)	40.3
14	(19.0,0.7,−16.4,9.6)	28.8
15	(37.6,32.4,−17.0,8.6)	30.4	Perseus–Pisces Void