List of the most distant astronomical objects
Adapted from Wikipedia · Discoverer experience
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.
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.
| Image | Name | Redshift (z) | Years after the Big Bang (millions) | Type |
|---|---|---|---|---|
| MoM-z14 | z = 14.44+0.02 −0.02 | 280 | Galaxy | |
| JADES-GS-z14-0 | z = 14.1796+0.0007 −0.0007 | 290 | Galaxy | |
| JADES-GS-z14-1 | z = 13.90+0.17 −0.17 | 300 | Galaxy | |
| PAN-z14-1 | z = 13.53+0.05 −0.06 | 310 | Galaxy | |
| JADES-GS-z13-0 | z = 13.20+0.04 −0.07 | 330 | Galaxy | |
| UNCOVER-z13 | z = 13.079+0.014 −0.001 | 330 | Galaxy | |
| JADES-GS-z13-1 | z = 13.0 | 330 | Galaxy | |
| JADES-GS-z12-0 | z = 12.63+0.24 −0.08 | 350 | Galaxy | |
| UNCOVER-z12 | z = 12.393+0.004 −0.001 | 350 | Galaxy | |
| GLASS-z12 (GHZ2) | z = 12.3327+0.0035 −0.0035 | 367 | Galaxy | |
| UDFj-39546284 | z = 11.58+0.05 −0.05 | 380 | Galaxy | |
| CEERS J141946.36+525632.8 (Maisie's Galaxy) | z = 11.44+0.09 −0.08 | 390 | Galaxy | |
| CEERS2-588 | z = 11.04 | 410 | Galaxy | |
| GN-z11 | z = 10.6034 ± 0.0013 | 430 | Galaxy | |
| JADES-GS-z10-0 (UDFj-38116243) | z = 10.38+0.07 −0.06 | 450 | Galaxy | |
| JD1 | z = 9.793±0.002 | 480 | Galaxy | |
| Gz9p3 | z = 9.3127 ± 0.0002 | 510 | Galaxy | |
| MACS1149-JD1 | z = 9.1096±0.0006 | 500 | Galaxy | |
| EGSY8p7 (CEERS_1019) | z = 8.683+0.001 −0.004 | 570 | Galaxy | |
| SMACS-4590 | z = 8.496 | Galaxy | ||
| A2744 YD4 | z = 8.38 | 600 | Galaxy | |
| MACS0416 Y1 | z = 8.3118±0.0003 | 600 | Galaxy | |
| GRB 090423 | z = 8.23+0.06 −0.07 | 630 | Gamma-ray burst | |
| RXJ2129-11002 | z = 8.16±0.01 | 613 | Galaxy | |
| RXJ2129-11022 | z = 8.15±0.01 | Galaxy | ||
| EGS-zs8-1 | z = 7.7302±0.0006 | 670 | Galaxy | |
| SMACS-0723-6355 | z = 7.665 | Galaxy | ||
| z7_GSD_3811 | z = 7.6637±0.0011 | Galaxy | ||
| SMACS-0723-10612 | z = 7.658 | Galaxy | ||
| QSO J0313–1806 | z = 7.6423±0.0013 | 670 | Quasar | |
| ULAS J1342+0928 | z = 7.5413±0.0007 | 690 | Quasar | |
| z8_GND_5296 | z = 7.51 | 700 | Galaxy | |
| A1689-zD1 | z = 7.5±0.2 | 700 | Galaxy | |
| GS2_1406 | z = 7.452±0.003 | Galaxy | ||
| GN-108036 | z = 7.213 | 750 | Galaxy | |
| SXDF-NB1006-2 | z = 7.2120±0.0003 | 800 | Galaxy | |
| BDF-3299 | z = 7.109±0.002 | 800 | Galaxy | |
| ULAS J1120+0641 | z = 7.085±0.003 | 770 | Quasar | |
| A1703 zD6 | z = 7.045±0.004 | Galaxy | ||
| BDF-521 | z = 7.008±0.002 | Galaxy | ||
| IOK-1 | z = 6.965 | 780 | Galaxy | |
| GDS_1408 (G2_1408) | z = 6.82±0.1 | Galaxy |
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.
| Name | Redshift (z) | Type |
|---|---|---|
| H-ATLAS J143740.9+021731 | z = 33.79 | Galaxy |
| Capotauro (CEERS U-100588 ) | z ~ 32 | Galaxy |
| MIDIS-z25-3 | zp = 25.6+1.5 −1.6 | Galaxy |
| F200DB-045 | zp = 20.4+0.3 −0.3 or 0.70+0.19 −0.55 or 0.40+0.15 −0.26 | Galaxy |
| GLIMPSE 70467 | zp = 16.4+1.8 −1.8 | Galaxy |
| F200DB-175 | zp = 16.2+0.3 −0.0 | Galaxy |
| S5-z17-1 | z = 16.0089±0.0004 or 4.6108±0.0001 | Galaxy |
| F150DB-041 | zp = 16.0+0.2 −0.2 or 3.70+0.02 −0.59 | Galaxy |
| SMACS-z16a | zp = 15.92+0.17 −0.15 or 2.96+0.73 −0.21 | Galaxy |
| F200DB-015 | zp = 15.8+3.4 −0.1 | Galaxy |
| F200DB-181 | zp = 15.8+0.5 −0.3 | Galaxy |
| F200DB-159 | zp = 15.8+4.0 −15.2 | Galaxy |
| GLIMPSE 72839 | zp = 15.8+0.8 −0.8 | Galaxy |
| F200DB-086 | zp = 15.4+0.6 −14.6 or 3.53+10.28 −1.84 | Galaxy |
| SMACS-z16b | zp = 15.32+0.16 −0.13 or 15.39+0.18 −0.26 | Galaxy |
| F150DB-048 | zp = 15.0+0.2 −0.8 | Galaxy |
| F150DB-007 | zp = 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.
| Type | Object | Redshift (distance) |
|---|---|---|
| Any astronomical object, no matter what type | MoM-z14 | z = 14.4 |
| Galaxy cluster | CL J1001+0220 | z ≅ 2.506 |
| Galaxy supercluster | Hyperion proto-supercluster | z = 2.45 |
| Galaxy protocluster | A2744z7p9OD | z = 7.88 |
| Galaxy or protogalaxy | MoM-z14 | z = 14.4 |
| Quasar | UHZ1 | z ≅ 10.0 |
| Black hole | GN-z11 | z = 10.6034±0.0013 |
| Star or protostar or post-stellar corpse (detected by an event) | Progenitor of GRB 090423 | z = 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 cluster | The Sparkler | z = 1.378 (13.9 Gly) |
| System of star clusters | ||
| X-ray jet | PJ352–15 quasar jet | z = 5.831 (12.7 Gly) |
| Microquasar | XMMU J004243.6+412519 | (2.5 Mly) |
| Nebula-like object | Himiko | z = 6.595 |
| Magnetic field | 9io9 | z = 2.554 (11.1 Gly) |
| Planet | SWEEPS-11 / SWEEPS-04 | (27,710 ly) |
| Type | Event | Redshift |
|---|---|---|
| Gamma-ray burst | GRB 090423 | z = 8.26+0.07 −0.08 |
| Supernova (any type) | SN Eos | z = 5.133±0.001 |
| Core collapse supernova | SN 1000+0216 | z = 3.8993 |
| Type Ia supernova | SN UDS10Wil | z = 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.
| Object | Type | Date | Distance (z = Redshift) | |
|---|---|---|---|---|
| MoM-z14 | Galaxy | 2025–present | z = 14.44 | |
| JADES-GS-z14-0 | Galaxy | 2024–2025 | z = 14.32 | |
| JADES-GS-z13-0 | Galaxy | 2022–2024 | z = 13.20 | |
| GN-z11 | Galaxy | 2016–2022 | z = 10.6 | |
| EGSY8p7 | Galaxy | 2015−2016 | z = 8.68 | |
| Progenitor of GRB 090423 / Remnant of GRB 090423 | Gamma-ray burst progenitor / Gamma-ray burst remnant | 2009–2015 | z = 8.2 | |
| IOK-1 | Galaxy | 2006 − 2009 | z = 6.96 | |
| SDF J132522.3+273520 | Galaxy | 2005 − 2006 | z = 6.597 | |
| SDF J132418.3+271455 | Galaxy | 2003 − 2005 | z = 6.578 | |
| HCM-6A | Galaxy | 2002 − 2003 | z = 6.56 | |
| SDSS J1030+0524 (SDSSp J103027.10+052455.0) | Quasar | 2001 − 2002 | z = 6.28 | |
| SDSS 1044–0125 (SDSSp J104433.04–012502.2) | Quasar | 2000 − 2001 | z = 5.82 | |
| SSA22-HCM1 | Galaxy | 1999–2000 | z>=5.74 | |
| HDF 4-473.0 | Galaxy | 1998–1999 | z = 5.60 | |
| RD1 (0140+326 RD1) | Galaxy | 1998 | z = 5.34 | |
| CL 1358+62 G1 & CL 1358+62 G2 | Galaxies | 1997 − 1998 | z = 4.92 | |
| PC 1247–3406 | Quasar | 1991 − 1997 | z = 4.897 | |
| PC 1158+4635 | Quasar | 1989 − 1991 | z = 4.73 | |
| Q0051–279 | Quasar | 1987 − 1989 | z = 4.43 | |
| Q0000–26 (QSO B0000–26) | Quasar | 1987 | z = 4.11 | |
| PC 0910+5625 (QSO B0910+5625) | Quasar | 1987 | z = 4.04 | |
| Q0046–293 (QSO J0048–2903) | Quasar | 1987 | z = 4.01 | |
| Q1208+1011 (QSO B1208+1011) | Quasar | 1986 − 1987 | z = 3.80 | |
| PKS 2000-330 (QSO J2003–3251, Q2000–330) | Quasar | 1982 − 1986 | z = 3.78 | |
| OQ172 (QSO B1442+101) | Quasar | 1974 − 1982 | z = 3.53 | |
| OH471 (QSO B0642+449) | Quasar | 1973 − 1974 | z = 3.408 | |
| 4C 05.34 | Quasar | 1970 − 1973 | z = 2.877 | |
| 5C 02.56 (7C 105517.75+495540.95) | Quasar | 1968 − 1970 | z = 2.399 | |
| 4C 25.05 (4C 25.5) | Quasar | 1968 | z = 2.358 | |
| PKS 0237–23 (QSO B0237–2321) | Quasar | 1967 − 1968 | z = 2.225 | |
| 4C 12.39 (Q1116+12, PKS 1116+12) | Quasar | 1966 − 1967 | z = 2.1291 | |
| 4C 01.02 (Q0106+01, PKS 0106+1) | Quasar | 1965 − 1966 | z = 2.0990 | |
| 3C 9 | Quasar | 1965 | z = 2.018 | |
| 3C 147 | Quasar | 1964 − 1965 | z = 0.545 | |
| 3C 295 | Radio galaxy | 1960 − 1964 | z = 0.461 | |
| LEDA 25177 (MCG+01-23-008) | Brightest cluster galaxy | 1951 − 1960 | z = 0.2 (V = 61000 km/s) | |
| LEDA 51975 (MCG+05-34-069) | Brightest cluster galaxy | 1936 – | z = 0.13 (V = 39000 km/s) | |
| LEDA 20221 (MCG+06-16-021) | Brightest cluster galaxy | 1932 – | z = 0.075 (V = 23000 km/s) | |
| BCG of WMH Christie's Leo Cluster | Brightest cluster galaxy | 1931 − 1932 | z = (V = 19700 km/s) | |
| BCG of Baede's Ursa Major Cluster | Brightest cluster galaxy | 1930 − 1931 | z = (V = 11700 km/s) | |
| NGC 4860 | Galaxy | 1929 − 1930 | z = 0.026 (V = 7800 km/s) | |
| NGC 7619 | Galaxy | 1929 | z = 0.012 (V = 3779 km/s) | |
| NGC 584 (Dreyer nebula 584) | Galaxy | 1921 − 1929 | z = 0.006 (V = 1800 km/s) | |
| M104 (NGC 4594) | Galaxy | 1913 − 1921 | z = 0.004 (V = 1180 km/s) | |
| Arcturus (Alpha Bootis) | Star | 1891 − 1910 | 160 ly (18 mas) (this is very inaccurate, true=37 ly) | |
| Capella (Alpha Aurigae) | Star | 1849–1891 | 72 ly (46 mas) | |
| Polaris (Alpha Ursae Minoris) | Star | 1847 – 1849 | 50 ly (80 mas) (this is very inaccurate, true=~440 ly) | |
| Vega (Alpha Lyrae) | Star (part of a double star pair) | 1839 – 1847 | 7.77 pc (125 mas) | |
| 61 Cygni | Binary star | 1838 − 1839 | 3.48 pc (313.6 mas) | |
| Uranus | Planet of the Solar System | 1781 − 1838 | 18 AU | |
| Saturn | Planet of the Solar System | 1619 − 1781 | 10 AU | |
| Mars | Planet of the Solar System | 1609 − 1619 | 2.6 AU when Mars is diametrically opposed to Earth | |
| Sun | Star | 3rd century BC — 1609 | 380 Earth radii (very inaccurate, true=16000 Earth radii) | |
| Moon | Moon of a planet | 3rd century BC | 20 Earth radii (very inaccurate, true=64 Earth radii) | |
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