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List of the most distant astronomical objects

Adapted from Wikipedia · Discoverer experience

A stunning image from the James Webb Space Telescope showing some of the earliest known galaxies in the universe, helping scientists study the early days of space and time.

This article lists the most distant astronomical objects discovered and verified so far, along with the time periods when they were recognized as such. These objects give us clues about the early universe and how it has changed over time.

MoM-z14 has a redshift of 14.44, making it the most distant known galaxy as of May 2025. This image represents the galaxy as it was less than 280 million years after the Big Bang.

The age of the universe is currently estimated to be about 13.787 billion years, but this number has changed as scientists have improved their methods of observation. For example, when the object IOK-1 was found in 2006, the estimated age of the universe was 13.66 billion years.

Measuring the distance to very far objects is tricky because they are usually very faint. Scientists often use a method called measuring the cosmological redshift of the object’s light. This means looking at how much the light from these objects has stretched to longer wavelengths. There are two ways to do this: using spectroscopy, which is more exact, and using a photometric redshift technique, which can sometimes be less accurate. Only objects with distances measured using spectroscopy are considered to have definitely known distances. The table in this article shows both types of measurements.

Most distant spectroscopically-confirmed objects

The universe is very old, and scientists have discovered objects that are very far away from us. These objects are some of the oldest things we know of, and they help us learn about how the universe began and grew. The age of the universe is estimated to be about 13.8 billion years old, but this number has changed as scientists have learned new things.

Most distant astronomical objects with spectroscopic redshift determinations
ImageNameRedshift
(z)
Years after the Big Bang (millions)Type
MoM-z14z = 14.44+0.02
−0.02
280Galaxy
JADES-GS-z14-0z = 14.1796+0.0007
−0.0007
290Galaxy
JADES-GS-z14-1z = 13.90+0.17
−0.17
300Galaxy
PAN-z14-1z = 13.53+0.05
−0.06
310Galaxy
JADES-GS-z13-0z = 13.20+0.04
−0.07
330Galaxy
UNCOVER-z13z = 13.079+0.014
−0.001
330Galaxy
JADES-GS-z13-1z = 13.0330Galaxy
JADES-GS-z12-0z = 12.63+0.24
−0.08
350Galaxy
UNCOVER-z12z = 12.393+0.004
−0.001
350Galaxy
GLASS-z12
(GHZ2)
z = 12.3327+0.0035
−0.0035
367Galaxy
UDFj-39546284z = 11.58+0.05
−0.05
380Galaxy
CEERS J141946.36+525632.8
(Maisie's Galaxy)
z = 11.44+0.09
−0.08
390Galaxy
CEERS2-588
z = 11.04410Galaxy
GN-z11z = 10.6034 ± 0.0013430Galaxy
JADES-GS-z10-0
(UDFj-38116243)
z = 10.38+0.07
−0.06
450Galaxy
JD1z = 9.793±0.002480Galaxy
Gz9p3z = 9.3127 ± 0.0002510Galaxy
MACS1149-JD1z = 9.1096±0.0006500Galaxy
EGSY8p7 (CEERS_1019)z = 8.683+0.001
−0.004
570Galaxy
SMACS-4590z = 8.496Galaxy
A2744 YD4z = 8.38600Galaxy
MACS0416 Y1z = 8.3118±0.0003600Galaxy
GRB 090423z = 8.23+0.06
−0.07
630Gamma-ray burst
RXJ2129-11002z = 8.16±0.01613Galaxy
RXJ2129-11022z = 8.15±0.01Galaxy
EGS-zs8-1z = 7.7302±0.0006670Galaxy
SMACS-0723-6355z = 7.665Galaxy
z7_GSD_3811z = 7.6637±0.0011Galaxy
SMACS-0723-10612z = 7.658Galaxy
QSO J0313–1806z = 7.6423±0.0013670Quasar
ULAS J1342+0928z = 7.5413±0.0007690Quasar
z8_GND_5296z = 7.51700Galaxy
A1689-zD1z = 7.5±0.2700Galaxy
GS2_1406z = 7.452±0.003Galaxy
GN-108036z = 7.213750Galaxy
SXDF-NB1006-2z = 7.2120±0.0003800Galaxy
BDF-3299z = 7.109±0.002800Galaxy
ULAS J1120+0641z = 7.085±0.003770Quasar
A1703 zD6z = 7.045±0.004Galaxy
BDF-521z = 7.008±0.002Galaxy
IOK-1z = 6.965780Galaxy
GDS_1408
(G2_1408)
z = 6.82±0.1Galaxy

Candidate most distant objects

Since the James Webb Space Telescope began its science work in June 2022, many faraway galaxies have been found. These galaxies are much farther than what the Hubble Space Telescope could see. The JWST can see deep into the infrared, which helps scientists spot these distant objects.

Before 2022, around 2012, there were about 50 possible objects that were very far away, and about 100 more candidates. Some of these objects have been studied closely, but only one light signal was found, so they are still considered possible candidates by scientists.

This list changes over time and may never be fully complete. You can help by updating the page with information from trusted sources.

Notable candidates for most distant astronomical objects
NameRedshift
(z)
Type
H-ATLAS J143740.9+021731z = 33.79Galaxy
Capotauro
(CEERS U-100588 )
z ~ 32Galaxy
MIDIS-z25-3zp = 25.6+1.5
−1.6
Galaxy
F200DB-045zp = 20.4+0.3
−0.3
or 0.70+0.19
−0.55 or 0.40+0.15
−0.26
Galaxy
GLIMPSE 70467zp = 16.4+1.8
−1.8
Galaxy
F200DB-175zp = 16.2+0.3
−0.0
Galaxy
S5-z17-1z = 16.0089±0.0004
or 4.6108±0.0001
Galaxy
F150DB-041zp = 16.0+0.2
−0.2
or 3.70+0.02
−0.59
Galaxy
SMACS-z16azp = 15.92+0.17
−0.15
or 2.96+0.73
−0.21
Galaxy
F200DB-015zp = 15.8+3.4
−0.1
Galaxy
F200DB-181zp = 15.8+0.5
−0.3
Galaxy
F200DB-159zp = 15.8+4.0
−15.2
Galaxy
GLIMPSE 72839zp = 15.8+0.8
−0.8
Galaxy
F200DB-086zp = 15.4+0.6
−14.6
or 3.53+10.28
−1.84
Galaxy
SMACS-z16bzp = 15.32+0.16
−0.13
or 15.39+0.18
−0.26
Galaxy
F150DB-048zp = 15.0+0.2
−0.8
Galaxy
F150DB-007zp = 14.6+0.4
−0.4
Galaxy

List of most distant objects by type

This section lists the farthest objects we have found in space, grouped by their type.

Most distant object by type
TypeObjectRedshift
(distance)
Any astronomical object, no matter what typeMoM-z14z = 14.4
Galaxy clusterCL J1001+0220z ≅ 2.506
Galaxy superclusterHyperion proto-superclusterz = 2.45
Galaxy protoclusterA2744z7p9ODz = 7.88
Galaxy or protogalaxyMoM-z14z = 14.4
QuasarUHZ1z ≅ 10.0
Black holeGN-z11z = 10.6034±0.0013
Star or protostar or post-stellar corpse
(detected by an event)
Progenitor of GRB 090423z = 8.26+0.07
−0.08
Star or protostar or post-stellar corpse
(detected as a star)
WHL0137-LS (Earendel)z = 6.2 ± 0.1
(12.9 Gly)
Star clusterThe Sparklerz = 1.378
(13.9 Gly)
System of star clusters
X-ray jetPJ352–15 quasar jetz = 5.831
(12.7 Gly)
MicroquasarXMMU J004243.6+412519(2.5 Mly)
Nebula-like objectHimikoz = 6.595
Magnetic field9io9z = 2.554 (11.1 Gly)
PlanetSWEEPS-11 / SWEEPS-04(27,710 ly)
Most distant event by type
TypeEventRedshift
Gamma-ray burstGRB 090423z = 8.26+0.07
−0.08
Supernova (any type)SN Eosz = 5.133±0.001
Core collapse supernovaSN 1000+0216z = 3.8993
Type Ia supernovaSN UDS10Wilz = 1.914

Timeline of most distant astronomical object recordholders

Objects on this list were the farthest known objects when scientists first measured how far away they were. This measurement date is often different from when the object was first found.

Scientists can figure out how far away stars and galaxies are by using special tools. They might look at how the object’s light changes over time, or they measure how much the light from the object has stretched out, called redshift. Redshift is shown with the symbol z.

Most distant object titleholders (not including candidates based on photometric redshifts)
ObjectTypeDateDistance
(z = Redshift)
MoM-z14Galaxy2025–presentz = 14.44
JADES-GS-z14-0Galaxy2024–2025z = 14.32
JADES-GS-z13-0Galaxy2022–2024z = 13.20
GN-z11Galaxy2016–2022z = 10.6
EGSY8p7Galaxy2015−2016z = 8.68
Progenitor of GRB 090423 / Remnant of GRB 090423Gamma-ray burst progenitor / Gamma-ray burst remnant2009–2015z = 8.2
IOK-1Galaxy2006 − 2009z = 6.96
SDF J132522.3+273520Galaxy2005 − 2006z = 6.597
SDF J132418.3+271455Galaxy2003 − 2005z = 6.578
HCM-6AGalaxy2002 − 2003z = 6.56
SDSS J1030+0524
(SDSSp J103027.10+052455.0)
Quasar2001 − 2002z = 6.28
SDSS 1044–0125
(SDSSp J104433.04–012502.2)
Quasar2000 − 2001z = 5.82
SSA22-HCM1Galaxy1999–2000z>=5.74
HDF 4-473.0Galaxy1998–1999z = 5.60
RD1 (0140+326 RD1)Galaxy1998z = 5.34
CL 1358+62 G1 & CL 1358+62 G2Galaxies1997 − 1998z = 4.92
PC 1247–3406Quasar1991 − 1997z = 4.897
PC 1158+4635Quasar1989 − 1991z = 4.73
Q0051–279Quasar1987 − 1989z = 4.43
Q0000–26
(QSO B0000–26)
Quasar1987z = 4.11
PC 0910+5625
(QSO B0910+5625)
Quasar1987z = 4.04
Q0046–293
(QSO J0048–2903)
Quasar1987z = 4.01
Q1208+1011
(QSO B1208+1011)
Quasar1986 − 1987z = 3.80
PKS 2000-330
(QSO J2003–3251, Q2000–330)
Quasar1982 − 1986z = 3.78
OQ172
(QSO B1442+101)
Quasar1974 − 1982z = 3.53
OH471
(QSO B0642+449)
Quasar1973 − 1974z = 3.408
4C 05.34Quasar1970 − 1973z = 2.877
5C 02.56
(7C 105517.75+495540.95)
Quasar1968 − 1970z = 2.399
4C 25.05
(4C 25.5)
Quasar1968z = 2.358
PKS 0237–23
(QSO B0237–2321)
Quasar1967 − 1968z = 2.225
4C 12.39
(Q1116+12, PKS 1116+12)
Quasar1966 − 1967z = 2.1291
4C 01.02
(Q0106+01, PKS 0106+1)
Quasar1965 − 1966z = 2.0990
3C 9Quasar1965z = 2.018
3C 147Quasar1964 − 1965z = 0.545
3C 295Radio galaxy1960 − 1964z = 0.461
LEDA 25177 (MCG+01-23-008)Brightest cluster galaxy1951 − 1960z = 0.2
(V = 61000 km/s)
LEDA 51975 (MCG+05-34-069)Brightest cluster galaxy1936 –z = 0.13
(V = 39000 km/s)
LEDA 20221 (MCG+06-16-021)Brightest cluster galaxy1932 –z = 0.075
(V = 23000 km/s)
BCG of WMH Christie's Leo ClusterBrightest cluster galaxy1931 − 1932z =
(V = 19700 km/s)
BCG of Baede's Ursa Major ClusterBrightest cluster galaxy1930 − 1931z =
(V = 11700 km/s)
NGC 4860Galaxy1929 − 1930z = 0.026
(V = 7800 km/s)
NGC 7619Galaxy1929z = 0.012
(V = 3779 km/s)
NGC 584
(Dreyer nebula 584)
Galaxy1921 − 1929z = 0.006
(V = 1800 km/s)
M104 (NGC 4594)Galaxy1913 − 1921z = 0.004
(V = 1180 km/s)
Arcturus
(Alpha Bootis)
Star1891 − 1910160 ly
(18 mas)
(this is very inaccurate, true=37 ly)
Capella
(Alpha Aurigae)
Star1849–189172 ly
(46 mas)
Polaris
(Alpha Ursae Minoris)
Star1847 – 184950 ly
(80 mas)
(this is very inaccurate, true=~440 ly)
Vega
(Alpha Lyrae)
Star (part of a double star pair)1839 – 18477.77 pc
(125 mas)
61 CygniBinary star1838 − 18393.48 pc
(313.6 mas)
UranusPlanet of the Solar System1781 − 183818 AU
SaturnPlanet of the Solar System1619 − 178110 AU
MarsPlanet of the Solar System1609 − 16192.6 AU when Mars is diametrically opposed to Earth
SunStar3rd century BC — 1609380 Earth radii (very inaccurate, true=16000 Earth radii)
MoonMoon of a planet3rd century BC20 Earth radii (very inaccurate, true=64 Earth radii)
z represents redshift, a measure of recessional velocity and inferred distance due to cosmological expansion
mas represents parallax, a measure of angle and distance that can be determined through trigonometry

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