List of the most distant astronomical objects explained

This article documents the most distant astronomical objects discovered and verified so far, and the time periods in which they were so classified.

For comparisons with the light travel distance of the astronomical objects listed below, the age of the universe since the Big Bang is currently estimated as 13.787±0.020 Gyr.^[1]

Distances to remote objects, other than those in nearby galaxies, are nearly always inferred by measuring the cosmological redshift of their light. By their nature, very distant objects tend to be very faint, and these distance determinations are difficult and subject to errors. An important distinction is whether the distance is determined via spectroscopy or using a photometric redshift technique. The former is generally both more precise and also more reliable, in the sense that photometric redshifts are more prone to being wrong due to confusion with lower redshift sources that may have unusual spectra. For that reason, a spectroscopic redshift is conventionally regarded as being necessary for an object's distance to be considered definitely known, whereas photometrically determined redshifts identify "candidate" very distant sources. Here, this distinction is indicated by a "p" subscript for photometric redshifts.

The proper distance provides a measurement of how far a galaxy is at a fixed moment in time. At the present time the proper distance equals the comoving distance since the cosmological scale factor has value one:

. The proper distance represents the distance obtained as if one were able to freeze the flow of time (set in the FLRW metric) and walk all the way to a galaxy while using a meter stick.^[2] For practical reasons, the proper distance is calculated as the distance traveled by light (set in the FLRW metric) from the time of emission by a galaxy to the time an observer (on Earth) receives the light signal. It differs from the “light travel distance” since the proper distance takes into account the expansion of the universe, i.e. the space expands as the light travels through it, resulting in numerical values which locate the most distant galaxies beyond the Hubble sphere and therefore with recession velocities greater than the speed of light c.^[3]    

Most distant spectroscopically-confirmed objects

Most distant astronomical objects with spectroscopic redshift determinations

Image	Name	Redshift (z)	Light travel distance§ (Gly)[4] [5] [6] [7]	Proper distance(Gly)	Type	Notes
	JADES-GS-z14-0	z =			Galaxy	Lyman-break galaxy, detection of the Lyman break with JWST/NIRSpec.[8]
	JADES-GS-z14-1	z =			Galaxy	Lyman-break galaxy, detection of the Lyman break with JWST/NIRSpec.[9]
	JADES-GS-z13-0	z =	13.576 / 13.596 / 13.474 / 13.473	33.6	Galaxy	Lyman-break galaxy, detection of the Lyman break with JWST/NIRSpec.[10]
	UNCOVER-z13	z =	13.51	32.56†	Galaxy	Lyman-break galaxy, detection of the Lyman break with JWST/NIRSpec.[11]
	JADES-GS-z12-0	z =	13.556 / 13.576 / 13.454 / 13.453	32.34†	Galaxy	Lyman-break galaxy, detection of the Lyman break with JWST/NIRCam and JWST/NIRSpec, and CIII] line emission with JWST/NIRSpec. Most distant spectroscopic redshift from emission lines; most distant detection of non-primordial elements (C, O, Ne).
	UNCOVER-z12	z =	13.48	32.21†	Galaxy	Lyman-break galaxy, detection of the Lyman break with JWST/NIRSpec.
	GLASS-z12	z =	13.536 / 13.556 / 13.434 / 13.433	33.2	Galaxy	Lyman-break galaxy discovered by JWST/NIRCam, confirmed by ALMA detection of [O III] emission[12]
	UDFj-39546284	z =	13.512 / 13.532 / 13.410 / 13.409	31.77†	Galaxy	Lyman-break galaxy, detection of the Lyman break with JWST/NIRSpec.
	CEERS J141946.36+525632.8 (Maisie's Galaxy)[13]	z	13.4	31.69†	Galaxy	Lyman-break galaxy discovered by JWST
	CEERS2 588 [14]	z	13.45	31.45†	Galaxy	Lyman-break galaxy discovered by JWST
	GN-z11	z = 10.6034 ± 0.0013	13.481 / 13.501 / 13.380 / 13.379	31.18†	Galaxy	Lyman-break galaxy; detection of the Lyman break with HST at 5.5σ[15] and carbon emission lines with Keck/MOSFIRE at 5.3σ.[16] Conclusive redshift by JWST in February 2023[17]
	JADES-GS-z10-0 UDFj-39546284	z =	13.449 / 13.469 / 13.348 / 13.347	31.04†	Galaxy	Lyman-break galaxy, detection of the Lyman break with JWST/NIRSpec
	JD1	z =	13.409 / 13.429 / 13.308 / 13.307	30.12†	Galaxy	Lyman-break galaxy, detection of the Lyman break with JWST/NIRSpec[18]
	Gz9p3	z=9.3127 ± 0.0002	13.277	30.27†	Galaxy	A galaxy merger with a redshift estimated from [OII], Ne and H emission lines detected with JWST.[19]
	MACS1149-JD1	z =	13.361 / 13.381 / 13.261 / 13.260	30.37	Galaxy	Detection of hydrogen emission line with the VLT, and oxygen line with ALMA[20]
	EGSY8p7	z =	13.325 / 13.345 / 13.225 / 13.224	30.05	Galaxy	Lyman-alpha emitter; detection of Lyman-alpha with Keck/MOSFIRE at 7.5σ confidence[21]
	SMACS-4590	z = 8.496	13.308 / 13.328 / 13.208 / 13.207	29.71†	Galaxy	Detection of hydrogen, oxygen, and neon emission lines with JWST/NIRSpec[22] [23] [24] [25]
	A2744 YD4	z = 8.38	13.297 / 13.317 / 13.197 / 13.196	29.50†	Galaxy	Lyman-alpha and [O III] emission detected with ALMA at 4.0σ confidence[26]
	MACS0416 Y1	z =	13.290 / 13.310 / 13.190 / 13.189	29.44†	Galaxy	[O III] emission detected with ALMA at 6.3σ confidence[27]
	GRB 090423	z =	13.282 / 13.302 / 13.182 / 13.181	30	Gamma-ray burst	Lyman-alpha break detected[28]
	RXJ2129-11002	z =	13.175	29.31†	Galaxy	[O III] doublet, Hβ, and [O II] doublet as well as Lyman-alpha break detected with JWST/NIRSpec prism[29]
	RXJ2129-11022	z =	13.174	29.30†	Galaxy	[O III] doublet and Hβ as well as Lyman-alpha break detected with JWST/NIRSpec prism
	EGS-zs8-1	z =	13.228 / 13.248 / 13.129 / 13.128	29.5	Galaxy	Lyman-break galaxy[30]
	SMACS-6355	z = 7.665	13.221 / 13.241 / 13.121 / 13.120	28.83	Galaxy	Detection of hydrogen, oxygen, and neon emission lines with JWST/NIRSpec
	z7_GSD_3811	z =	13.221 / 13.240 / 13.121 / 13.120	28.83†	Galaxy	Lyman-alpha emitter[31]
	SMACS-10612	z = 7.658	13.221 / 13.241 / 13.120 / 13.119	28.83†	Galaxy	Detection of hydrogen, oxygen, and neon emission lines with JWST/NIRSpec
	QSO J0313–1806	z =	13.218 / 13.238 / 13.119 / 13.118	30	Quasar	Lyman-alpha break detected[32]
	ULAS J1342+0928	z =	13.206 / 13.226 / 13.107 / 13.106	29.36	Quasar	Redshift estimated from [C II] emission[33]
	z8_GND_5296	z = 7.51	13.202 / 13.222 / 13.103 / 13.102	30.01	Galaxy	Lyman-alpha emitter[34]
	A1689-zD1	z =	13.201 / 13.221 / 13.102 / 13.101	30	Galaxy	Lyman-break galaxy[35]
	GS2_1406	z =	13.195 / 13.215 / 13.096 / 13.095	28.62†	Galaxy	Lyman-alpha emitter[36]
	GN-108036	z = 7.213	13.164 / 13.184 / 13.065 / 13.064	29	Galaxy	Lyman alpha emitter
	SXDF-NB1006-2		13.164 / 13.184 / 13.065 / 13.064	29	Galaxy	[O III] emission detected[37]
	BDF-3299	z =	13.149 / 13.169 / 13.051 / 13.050	28.25	Galaxy	Lyman-break galaxy[38]
	ULAS J1120+0641	z =	13.146 / 13.166 / 13.048 / 13.047	29.85	Quasar	Redshift estimated from Si III]+C III] and Mg II emission lines[39]
	A1703 zD6	z =	13.140 / 13.160 / 13.042 / 13.041	29	Galaxy	Gravitationally-lensed Lyman-alpha emitter[40]
	BDF-521	z =	13.135 / 13.155 / 13.037 / 13.036	28.43†	Galaxy	Lyman-break galaxy
	G2_1408	z =	13.130 / 13.150 / 13.032 / 13.030	28.10†	Galaxy	Lyman-alpha emitter[41]
	IOK-1	z = 6.965	13.129 / 13.149 / 13.030 / 13.029	28.09†	Galaxy	Lyman-alpha emitter[42]
	LAE J095950.99+021219.1	z = 6.944	13.126 / 13.146 / 13.028 / 13.027	28.07†	Galaxy	Lyman-alpha emitter[43]
	SDF-46975	z = 6.844	13.111 / 13.131 / 13.013 / 13.012	27.95†	Galaxy	Lyman-alpha emitter
	PSO J172.3556+18.7734	z =	13.107 / 13.127 / 13.010 / 13.009	27.93†	Quasar (astrophysical jet)	Redshift estimated from Mg II emission[44]
§ The tabulated distance is the light travel distance, which has no direct physical significance. See discussion at distance measures and Observable Universe † Numeric value obtained using Wright (2006) with H0 = 70, \OmegaCM = 0.30, \OmegaDE = 0.70.

Candidate most distant objects

Since the beginning of the James Webb Space Telescope's (JWST) science operations in June 2022, numerous distant galaxies far beyond what could be seen by the Hubble Space Telescope (z = 11) have been discovered thanks to the JWST's capability of seeing far into the infrared.^[45] Previously in 2012, there were about 50 possible objects z = 8 or farther, and another 100 candidates at z = 7, based on photometric redshift estimates released by the Hubble eXtreme Deep Field (XDF) project from observations made between mid-2002 and December 2012.^[46] Some objects included here have been observed spectroscopically, but had only one emission line tentatively detected, and are therefore still considered candidates by researchers.^[47]

Notable candidates for most distant astronomical objects

Name	Redshift (z)	Light travel distance§ (Gly)	Type	Notes
F200DB-045	zp = or or	13.725 / 13.745 / 13.623 / 13.621	Galaxy	Lyman-break galaxy discovered by JWST NOTE: The redshift value of the galaxy presented by the procedure in one study may differ from the values presented in other studies using different procedures.[48] [49]
F200DB-175	zp =	13.657 / 13.677 / 13.555 / 13.554	Galaxy	Lyman-break galaxy discovered by JWST
S5-z17-1	or	13.653 / 13.673 / 13.551 / 13.550	Galaxy	Lyman-break galaxy discovered by JWST; tentative (5.1σ) ALMA detection of a single emission line possibly attributed to either [C II] (z =) or [O III] (z =).[50]
F150DB-041	zp = or	13.653 / 13.673 / 13.551 / 13.549	Galaxy	Lyman-break galaxy discovered by JWST
SMACS-z16a	zp = or	13.651 / 13.671 / 13.549 / 13.548	Galaxy	Lyman-break galaxy discovered by JWST[51] [52]
F200DB-015	zp =	13.648 / 13.668 / 13.546 / 13.545	Galaxy	Lyman-break galaxy discovered by JWST
F200DB-181	zp =	13.648 / 13.668 / 13.546 / 13.545	Galaxy	Lyman-break galaxy discovered by JWST
F200DB-159	zp =	13.648 / 13.668 / 13.546 / 13.545	Galaxy	Lyman-break galaxy discovered by JWST
F200DB-086	zp = or	13.639 / 13.659 / 13.537 / 13.536	Galaxy	Lyman-break galaxy discovered by JWST
SMACS-z16b	zp = or	13.637 / 13.657 / 13.535 / 13.534	Galaxy	Lyman-break galaxy discovered by JWST
F150DB-048	zp =	13.629 / 13.649 / 13.527 / 13.526	Galaxy	Lyman-break galaxy discovered by JWST
F150DB-007	zp =	13.619 / 13.639 / 13.517 / 13.516	Galaxy	Lyman-break galaxy discovered by JWST
F150DB-004	zp =	13.602 / 13.622 / 13.500 / 13.499	Galaxy	Lyman-break galaxy discovered by JWST
F150DB-079	zp =	13.596 / 13.616 / 13.494 / 13.493	Galaxy	Lyman-break galaxy discovered by JWST
F150DA-007	zp =	13.583 / 13.603 / 13.481 / 13.480	Galaxy	Lyman-break galaxy discovered by JWST
F150DA-053	zp =	13.583 / 13.603 / 13.481 / 13.480	Galaxy	Lyman-break galaxy discovered by JWST
F150DA-050	zp =	13.583 / 13.603 / 13.481 / 13.480	Galaxy	Lyman-break galaxy discovered by JWST
F150DA-058	zp =	13.583 / 13.603 / 13.481 / 13.480	Galaxy	Lyman-break galaxy discovered by JWST
F150DA-038	zp =	13.583 / 13.603 / 13.481 / 13.480	Galaxy	Lyman-break galaxy discovered by JWST
HD1	z =	13.579 / 13.599 / 13.477 / 13.476	Galaxy	Not yet spectroscopically confirmed. Guinness World Record of the most distant confirmed galaxy Lyman-break galaxy (5σ confidence) followed with a tentative ALMA detection of a single [O III] oxygen emission line only (4σ confidence)[53]
F150DA-010	zp =	13.562 / 13.582 / 13.460 / 13.459	Galaxy	Lyman-break galaxy discovered by JWST
S5-z12-1	zp =	13.553 / 13.573 / 13.452 / 13.451	Galaxy	Lyman-break galaxy discovered by JWST
CEERS-27535 4	zp =	13.553 / 13.573 / 13.452 / 13.451	Galaxy	Lyman-break galaxy discovered by JWST[54]
SMACS-1566	zp =	13.542 / 13.562 / 13.441 / 13.440	Galaxy	Lyman-break galaxy discovered by JWST
SMACS-z12b (F150DA-077)	zp = or	13.541 / 13.561 / 13.440 / 13.439	Galaxy	Lyman-break galaxy discovered by JWST
SMACS-z12a	zp =	13.539 / 13.559 / 13.437 / 13.436	Galaxy	Lyman-break galaxy discovered by JWST
CR2-z12-4	zp =	13.534 / 13.554 / 13.432 / 13.431	Galaxy	Lyman-break galaxy discovered by JWST
SMACS-10566	zp =	13.532 / 13.552 / 13.430 / 13.429	Galaxy	Lyman-break galaxy discovered by JWST
XDFH-2395446286	zp =	13.530 / 13.550 / 13.429 / 13.428	Galaxy	Lyman-break galaxy detected by JWST and Hubble[55]
CR2-z12-2	zp =	13.529 / 13.549 / 13.427 / 13.426	Galaxy	Lyman-break galaxy discovered by JWST
9-BUSCAR	zp =	13.527 / 13.547 / 13.425 / 13.424	Galaxy	Lyman-break galaxy discovered by JWST[56]
SMACS-8347	zp =	13.526 / 13.546 / 13.425 / 13.424	Galaxy	Lyman-break galaxy discovered by JWST
CEERS-26409 4	zp =	13.526 / 13.546 / 13.425 / 13.424	Galaxy	Lyman-break galaxy discovered by JWST
F150DB-069	zp =	13.522 / 13.542 / 13.420 / 13.419	Galaxy	Lyman-break galaxy discovered by JWST
XDFH-2334046578	zp =	13.522 / 13.542 / 13.420 / 13.419	Galaxy	Lyman-break galaxy detected by JWST and Hubble
CR2-z12-3	zp =	13.515 / 13.535 / 13.414 / 13.413	Galaxy	Lyman-break galaxy discovered by JWST
CR2-z12-1	zp =	13.514 / 13.534 / 13.413 / 13.412	Galaxy	Lyman-break galaxy discovered by JWST
F150DB-088	zp =	13.513 / 13.533 / 13.411 / 13.410	Galaxy	Lyman-break galaxy discovered by JWST
F150DB-084	zp =	13.513 / 13.533 / 13.411 / 13.410	Galaxy	Lyman-break galaxy discovered by JWST
F150DB-044	zp =	13.503 / 13.523 / 13.402 / 13.401	Galaxy	Lyman-break galaxy discovered by JWST
XDFH-2404647339	zp =	13.503 / 13.523 / 13.402 / 13.401	Galaxy	Lyman-break galaxy detected by JWST and Hubble
F150DB-075	zp =	13.503 / 13.523 / 13.402 / 13.401	Galaxy	Lyman-break galaxy discovered by JWST
F150DA-062	zp =	13.503 / 13.523 / 13.402 / 13.401	Galaxy	Lyman-break galaxy discovered by JWST
CEERS-127682	zp =	13.503 / 13.523 / 13.402 / 13.401	Galaxy	Lyman-break galaxy discovered by JWST
CEERS-5268 2	zp =	13.503 / 13.523 / 13.402 / 13.401	Galaxy	Lyman-break galaxy discovered by JWST
F150DA-060	zp =	13.503 / 13.523 / 13.402 / 13.401	Galaxy	Lyman-break galaxy discovered by JWST
F150DA-031	zp =	13.503 / 13.523 / 13.402 / 13.401	Galaxy	Lyman-break galaxy discovered by JWST
F150DA-052	zp =	13.503 / 13.523 / 13.402 / 13.401	Galaxy	Lyman-break galaxy discovered by JWST
F150DB-054	zp =	13.503 / 13.523 / 13.402 / 13.401	Galaxy	Lyman-break galaxy discovered by JWST
SMACS-z11d	zp = or		Galaxy	Lyman-break galaxy discovered by JWST
CEERS-77241	zp =		Galaxy	Lyman-break galaxy discovered by JWST
CEERS-6647	zp =		Galaxy	Lyman-break galaxy discovered by JWST
CEERS-622 4	zp =		Galaxy	Lyman-break galaxy discovered by JWST
SMACS-z11c	zp = or		Galaxy	Lyman-break galaxy discovered by JWST
SMACS-z11b	zp = or		Galaxy	Lyman-break galaxy discovered by JWST
F150DA-005	zp =		Galaxy	Lyman-break galaxy discovered by JWST
F150DA-020	zp =		Galaxy	Lyman-break galaxy discovered by JWST
CEERS-61486	zp =		Galaxy	Lyman-break galaxy discovered by JWST
SMACS-z11e (F150DA-081)	zp = or		Galaxy	Lyman-break galaxy discovered by JWST
SMACS-z11a	zp = or		Galaxy	Lyman-break galaxy discovered by JWST
CR3-z12-1	zp =		Galaxy	Lyman-break galaxy discovered by JWST
F150DA-026	zp =		Galaxy	Lyman-break galaxy discovered by JWST
F150DA-036	zp =		Galaxy	Lyman-break galaxy discovered by JWST
SMACS-z10e	zp = or		Galaxy	Lyman-break galaxy discovered by JWST
F150DB-040	zp =		Galaxy	Lyman-break galaxy discovered by JWST
EGS-14506	zp =		Galaxy	Lyman-break galaxy discovered by JWST[57]
MACS0647-JD	zp =		Galaxy	Gravitationally lensed into three images by a galaxy cluster; detected by JWST and Hubble[58] [59]
GLASS-z10 (GLASS-1698)	z = 10.38		Galaxy	Lyman-break galaxy discovered by JWST; tentative (4.4σ) ALMA detection of [O III] emission line only[60] [61]
EGS-7860	zp =		Galaxy	Lyman-break galaxy discovered by JWST
SPT0615-JD	zp =	13.419	Galaxy	[62]
A2744-JD	zp≅9.8	13.412	Galaxy	Galaxy is being magnified and lensed into three multiple images, geometrically supporting its redshift.[63] [64]
MACS1149-JD1	zp≅9.6	13.398[65]	Candidate galaxy or protogalaxy	[66]
GRB 090429B	zp≅9.4	13.383[67]	Gamma-ray burst	[68] The photometric redshift in this instance has quite large uncertainty, with the lower limit for the redshift being z>7.
UDFy-33436598	zp≅8.6	13.317	Candidate galaxy or protogalaxy	[69]
UDFy-38135539	zp≅8.6	13.317	Candidate galaxy or protogalaxy	A spectroscopic redshift of z = 8.55 was claimed for this source in 2010,[70] but has subsequently been shown to be mistaken.[71]
BoRG-58	zp≅8	13.258	Galaxy cluster or protocluster	Protocluster candidate[72]
§ The tabulated distance is the light travel distance, which has no direct physical significance. See discussion at distance measures and Observable Universe

List of most distant objects by type

Most distant object by type

Type	Object	Redshift (distance)	Notes
Any astronomical object, no matter what type	JADES-GS-z14-0	z = 14.32	Most distant galaxy with a spectroscopically confirmed redshift .
Galaxy or protogalaxy
Galaxy cluster	CL J1001+0220	z ≅ 2.506	As of 2016[73] See also: List of galaxy clusters.
Galaxy supercluster	Hyperion proto-supercluster	z = 2.45	This supercluster at the time of its discovery in 2018 was the earliest and largest proto-supercluster found to date.[74]
Galaxy protocluster	A2744z7p9OD	z = 7.88	This protocluster at the time of its discovery in 2023 was the most distant protocluster found and spectroscopically confirmed to date.[75] See also: List of galaxy groups and clusters.
Quasar	UHZ1	z ~ 10.0	See also: List of quasars.
Black hole
Star or protostar or post-stellar corpse (detected by an event)	Progenitor of GRB 090423	z = 8.2	[76] Note, GRB 090429B has a photometric redshift zp≅9.4,[77] and so is most likely more distant than GRB 090423, but is lacking spectroscopic confirmation. See also: List of gamma-ray bursts. Estimated an approximate distance of 13 billion lightyears from Earth
Star or protostar or post-stellar corpse (detected as a star)	WHL0137-LS (Earendel)	(12.9 Gly)	Most distant individual star detected (March, 2022).[78] [79] Previous records include SDSS J1229+1122[80] and MACS J1149 Lensed Star 1.[81]
Star cluster	The Sparkler	z = 1.378 (13.9 Gly)	Galaxy with globular clusters gravitationally lensed in SMACS J0723.3-7327[82]
System of star clusters
X-ray jet	PJ352–15 quasar jet	z = 5.831 (12.7 Gly)[83]	The previous recordholder was at 12.4 Gly.[84] [85]
Microquasar	XMMU J004243.6+412519	(2.5 Mly)	First extragalactic microquasar discovered[86] [87] [88]
Nebula-like object	Himiko	z = 6.595	Possibly one of the largest objects in the early universe.[89] [90]
Magnetic field	9io9	z = 2.554 (11.1 Gly)	Observations from ALMA has shown that the lensed galaxy 9io9 contains a magnetic field.
Planet	SWEEPS-11 / SWEEPS-04	(27,710 ly)	[91] An analysis of the lightcurve of the microlensing event PA-99-N2 suggests the presence of a planet orbiting a star in the Andromeda Galaxy.[92] A controversial microlensing event of lobe A of the double gravitationally lensed Q0957+561 suggests that there is a planet in the lensing galaxy lying at redshift 0.355 (3.7 Gly).[93] [94]

Most distant event by type

Type	Event	Redshift	Notes
Gamma-ray burst	GRB 090423	z = 8.2	Note, GRB 090429B has a photometric redshift zp≅9.4, and so is most likely more distant than GRB 090423, but is lacking spectroscopic confirmation. See also: List of gamma-ray bursts.
Core collapse supernova	SN 1000+0216	z = 3.8993	[95] See also: List of most distant supernovae.
Type Ia supernova	SN UDS10Wil	z = 1.914	[96] See also: List of supernovae.
Type Ia supernova	SN SCP-0401 (Mingus)	z = 1.71	First observed in 2004, it was not until 2013 that it could be identified as a Type-Ia SN.[97] [98] See also: List of supernovae.
Cosmic Decoupling	Cosmic Microwave Background Radiation creation	z~1000 to 1089	[99] [100]

Timeline of most distant astronomical object recordholders

Objects in this list were found to be the most distant object at the time of determination of their distance. This is frequently not the same as the date of their discovery.

Distances to astronomical objects may be determined through parallax measurements, use of standard references such as cepheid variables or Type Ia supernovas, or redshift measurement. Spectroscopic redshift measurement is preferred, while photometric redshift measurement is also used to identify candidate high redshift sources. The symbol z represents redshift.

Most Distant Object Titleholders (not including candidates based on photometric redshifts)

Object	Type	Date	Distance (z = Redshift)	Notes
JADES-GS-z14-0	Galaxy	2024–present	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	[101] [102] [103] [104]
Progenitor of GRB 090423 / Remnant of GRB 090423	Gamma-ray burst progenitor / Gamma-ray burst remnant	2009 − 2015	z = 8.2	[105]
IOK-1	Galaxy	2006 − 2009	z = 6.96	[106] [107] [108]
SDF J132522.3+273520	Galaxy	2005 − 2006	z = 6.597	[109]
SDF J132418.3+271455	Galaxy	2003 − 2005	z = 6.578	[110] [111] [112]
HCM-6A	Galaxy	2002 − 2003	z = 6.56	The galaxy is lensed by galaxy cluster Abell 370. This was the first non-quasar galaxy found to exceed redshift 6. It exceeded the redshift of quasar SDSSp J103027.10+052455.0 of z = 6.28[113] [114] [115] [116]
SDSS J1030+0524 (SDSSp J103027.10+052455.0)	Quasar	2001 − 2002	z = 6.28	[117] [118] [119] [120]
SDSS 1044–0125 (SDSSp J104433.04–012502.2)	Quasar	2000 − 2001	z = 5.82	[121] [122] [123] [124] [125] [126] [127]
SSA22-HCM1	Galaxy	1999 − 2000	z>=5.74	[128]
HDF 4-473.0	Galaxy	1998 − 1999	z = 5.60	[129]
RD1 (0140+326 RD1)	Galaxy	1998	z = 5.34	[130] [131] [132] [133]
CL 1358+62 G1 & CL 1358+62 G2	Galaxies	1997 − 1998	z = 4.92	These were the most remote objects discovered at the time. The pair of galaxies were found lensed by galaxy cluster CL1358+62 (z = 0.33). This was the first time since 1964 that something other than a quasar held the record for being the most distant object in the universe.[134] [135] [136]
PC 1247–3406	Quasar	1991 − 1997	z = 4.897	[137] [138] [139] [140] [141]
PC 1158+4635	Quasar	1989 − 1991	z = 4.73	[142] [143] [144] [145]
Q0051–279	Quasar	1987 − 1989	z = 4.43	[146] [147] [148] [149]
Q0000–26 (QSO B0000–26)	Quasar	1987	z = 4.11	[150]
PC 0910+5625 (QSO B0910+5625)	Quasar	1987	z = 4.04	This was the second quasar discovered with a redshift over 4.[151] [152]
Q0046–293 (QSO J0048–2903)	Quasar	1987	z = 4.01	[153] [154]
Q1208+1011 (QSO B1208+1011)	Quasar	1986 − 1987	z = 3.80	This is a gravitationally-lensed double-image quasar, and at the time of discovery to 1991, had the least angular separation between images, 0.45.[155] [156]
PKS 2000-330 (QSO J2003–3251, Q2000–330)	Quasar	1982 − 1986	z = 3.78	[157] [158]
OQ172 (QSO B1442+101)	Quasar	1974 − 1982	z = 3.53	[159]
OH471 (QSO B0642+449)	Quasar	1973 − 1974	z = 3.408	Nickname was "the blaze marking the edge of the universe".[160] [161] [162] [163]
4C 05.34	Quasar	1970 − 1973	z = 2.877	Its redshift was so much greater than the previous record that it was believed to be erroneous, or spurious.[164] [165] [166]
5C 02.56 (7C 105517.75+495540.95)	Quasar	1968 − 1970	z = 2.399	[167] [168]
4C 25.05 (4C 25.5)	Quasar	1968	z = 2.358	[169]
PKS 0237–23 (QSO B0237–2321)	Quasar	1967 − 1968	z = 2.225	[170] [171] [172]
4C 12.39 (Q1116+12, PKS 1116+12)	Quasar	1966 − 1967	z = 2.1291	[173]
4C 01.02 (Q0106+01, PKS 0106+1)	Quasar	1965 − 1966	z = 2.0990	[174] [175]
3C 9	Quasar	1965	z = 2.018	[176] [177] [178] [179] [180]
3C 147	Quasar	1964 − 1965	z = 0.545	[181] [182] [183] [184]
3C 295	Radio galaxy	1960 − 1964	z = 0.461	[185] [186] [187]
LEDA 25177 (MCG+01-23-008)	Brightest cluster galaxy	1951 − 1960	z = 0.2 (V = 61000 km/s)	This galaxy lies in the Hydra Supercluster. It is located at B1950.0 and is the BCG of the fainter Hydra Cluster Cl 0855+0321 (ACO 732).[188] [189] [190] [191] [192]
LEDA 51975 (MCG+05-34-069)	Brightest cluster galaxy	1936 –	z = 0.13 (V = 39000 km/s)	The brightest cluster galaxy of the Bootes Cluster (ACO 1930), an elliptical galaxy at B1950.0 apparent magnitude 17.8, was found by Milton L. Humason in 1936 to have a 40,000 km/s recessional redshift velocity.[193] [194]
LEDA 20221 (MCG+06-16-021)	Brightest cluster galaxy	1932 –	z = 0.075 (V = 23000 km/s)	This is the BCG of the Gemini Cluster (ACO 568) and was located at B1950.0 [195]
BCG of WMH Christie's Leo Cluster	Brightest cluster galaxy	1931 − 1932	z = (V = 19700 km/s)	[196] [197] [198]
BCG of Baede's Ursa Major Cluster	Brightest cluster galaxy	1930 − 1931	z = (V = 11700 km/s)	[199]
NGC 4860	Galaxy	1929 − 1930	z = 0.026 (V = 7800 km/s)	[200]
NGC 7619	Galaxy	1929	z = 0.012 (V = 3779 km/s)	Using redshift measurements, NGC 7619 was the highest at the time of measurement. At the time of announcement, it was not yet accepted as a general guide to distance, however, later in the year, Edwin Hubble described redshift in relation to distance, which became accepted widely as an inferred distance.[201] [202]
NGC 584 (Dreyer nebula 584)	Galaxy	1921 − 1929	z = 0.006 (V = 1800 km/s)	At the time, nebula had yet to be accepted as independent galaxies. However, in 1923, galaxies were generally recognized as external to the Milky Way.[203] [204] [205] [206]
M104 (NGC 4594)	Galaxy	1913 − 1921	z = 0.004 (V = 1180 km/s)	This was the second galaxy whose redshift was determined; the first being Andromeda – which is approaching us and thus cannot have its redshift used to infer distance. Both were measured by Vesto Melvin Slipher. At this time, nebula had yet to be accepted as independent galaxies. NGC 4594 was measured originally as 1000 km/s, then refined to 1100, and then to 1180 in 1916.[207]
Arcturus (Alpha Bootis)	Star	1891 − 1910	160 ly (18 mas) (this is very inaccurate, true=37 ly)	This number is wrong; originally announced in 1891, the figure was corrected in 1910 to 40 ly (60 mas). From 1891 to 1910, it had been thought this was the star with the smallest known parallax, hence the most distant star whose distance was known. Prior to 1891, Arcturus had previously been recorded of having a parallax of 127 mas.[208] [209] [210] [211]
Capella (Alpha Aurigae)	Star	1849–1891	72 ly (46 mas)	[212] [213] [214]
Polaris (Alpha Ursae Minoris)	Star	1847 – 1849	50 ly (80 mas) (this is very inaccurate, true=~375 ly)	[215]
Vega (Alpha Lyrae)	Star (part of a double star pair)	1839 – 1847	7.77 pc (125 mas)	[216]
61 Cygni	Binary star	1838 − 1839	3.48 pc (313.6 mas)	This was the first star other than the Sun to have its distance measured.[217] [218]
Uranus	Planet of the Solar System	1781 − 1838	18 AU	This was the last planet discovered before the first successful measurement of stellar parallax. It had been determined that the stars were much farther away than the planets.
Saturn	Planet of the Solar System	1619 − 1781	10 AU	From Kepler's Third Law, it was finally determined that Saturn is indeed the outermost of the classical planets, and its distance derived. It had only previously been conjectured to be the outermost, due to it having the longest orbital period, and slowest orbital motion. It had been determined that the stars were much farther away than the planets.
Mars	Planet of the Solar System	1609 − 1619	2.6 AU when Mars is diametrically opposed to Earth	Kepler correctly characterized Mars and Earth's orbits in the publication Astronomia nova. It had been conjectured that the fixed stars were much farther away than the planets.
Sun	Star	3rd century BC — 1609	380 Earth radii (very inaccurate, true=16000 Earth radii)	Aristarchus of Samos made a measurement of the distance of the Sun from the Earth in relation to the distance of the Moon from the Earth. The distance to the Moon was described in Earth radii (20, also inaccurate). The diameter of the Earth had been calculated previously. At the time, it was assumed that some of the planets were further away, but their distances could not be measured. The order of the planets was conjecture until Kepler determined the distances from the Sun of the five known planets that were not Earth. It had been conjectured that the fixed stars were much farther away than the planets.
Moon	Moon of a planet	3rd century BC	20 Earth radii (very inaccurate, true=64 Earth radii)	Aristarchus of Samos made a measurement of the distance between the Earth and the Moon. The diameter of the Earth had been calculated previously.

List of objects by year of discovery that turned out to be most distant

This list contains a list of most distant objects by year of discovery of the object, not the determination of its distance. Objects may have been discovered without distance determination, and were found subsequently to be the most distant known at that time. However, object must have been named or described. An object like OJ 287 is ignored even though it was detected as early as 1891 using photographic plates, but ignored until the advent of radiotelescopes.

Examples

Year of record		Object	Type	Detected using	First record by (1)
964	2.5[219]			naked eye	furthest object visible with the naked eye, but first recorded by Abd al-Rahman al-Sufi[220]
1654	3			refracting telescope	Giovanni Battista Hodierna[221]
1779	68[222]				Charles Messier[223]
1785	76.4[224]				William Herschel
1880s	206 ± 29[225]				Dreyer, Herschel
1959	2,400[226]				Maarten Schmidt, Bev Oke[227]
1960	5,000[228]				Rudolph Minkowski
2009	13,000[229]				Krimm, H. et al.[230]

See also

• Age of the universe
• List of largest cosmic structures
• List of exoplanet extremes
• Lists of astronomical objects
• List of most distant stars
• Timeline of knowledge about galaxies, clusters of galaxies, and large-scale structure

Notes and References

1. Planck Collaboration . 2020 . Planck 2018 results. VI. Cosmological parameters . Astronomy & Astrophysics . 641 . page A6 (see PDF page 15, Table 2: "Age/Gyr", last column) . 10.1051/0004-6361/201833910 . 1807.06209 . 2020A&A...641A...6P . 119335614.
2. Book: Guidry, Mike . Modern general relativity: black holes, gravitational waves, and cosmology . 2019 . Cambridge university press . 978-1-107-19789-3 . Cambridge New York.
3. Davis . Tamara M. . Lineweaver . Charles H. . 2004 . Expanding Confusion: Common Misconceptions of Cosmological Horizons and the Superluminal Expansion of the Universe . Publications of the Astronomical Society of Australia . en . 21 . 1 . 97–109 . 10.1071/AS03040 . astro-ph/0310808 . 2004PASA...21...97D . 13068122 . 1323-3580.
4. Web site: . UCLA Cosmological Calculator . 2015 . . 6 August 2022 . Light travel distance was calculated from redshift value using the UCLA Cosmological Calculator, with parameters values as of 2015: H₀=67.74 and Omega_M=0.3089 (see Table/Planck2015 at "Lambda-CDM model#Parameters")
5. Web site: . UCLA Cosmological Calculator . 2018 . . 6 August 2022 . Light travel distance was calculated from redshift value using the UCLA Cosmological Calculator, with parameters values as of 2018: H₀=67.4 and Omega_M=0.315 (see Table/Planck2018 at "Lambda-CDM model#Parameters")
6. Web site: . ICRAR Cosmology Calculator . 2022 . . 6 August 2022 . ICRAR Cosmology Calculator - Set H₀=67.4 and Omega_M=0.315 (see Table/Planck2018 at "Lambda-CDM model#Parameters")
7. Web site: Kempner . Joshua . KEMPNER Cosmology Calculator . 2022 . Kempner.net . 6 August 2022 . KEMP Cosmology Calculator - Set H₀=67.4, Omega_M=0.315, and Omega_Λ=0.6847 (see Table/Planck2018 at "Lambda-CDM model#Parameters")
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