List of largest cosmic structures

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{{More citations needed|date=December 2022}}

{{multiple image

|image1 =Large-scale structure of light distribution in the universe.jpg

|caption1=Galaxy filaments form massive, thread-like structures on the order of millions of light-years. Computer simulation.

|image2 =2dfdtfe.gif

|caption2=The Sloan Great Wall, the Pisces–Cetus Supercluster Complex, the Horologium-Reticulum Supercluster and the Shapley Supercluster as seen in the 2dF Galaxy Redshift Survey

}}

This is a list of the largest cosmic structures so far discovered. The unit of measurement used is the light-year (distance traveled by light in one Julian year; approximately 9.46 trillion kilometres).

This list includes superclusters, galaxy filaments and large quasar groups (LQGs). The structures are listed based on their longest dimension.

This list refers only to coupling of matter with defined limits, and not the coupling of matter in general (such as, for example, the cosmic microwave background, which fills the entire universe). All structures in this list are defined as to whether their presiding limits have been identified.

There are some reasons to be cautious about this list:

  • The Zone of Avoidance, or the part of the sky occupied by the Milky Way, blocks out light from several structures, making their limits imprecisely identified.
  • Some structures are too distant to be seen even with the most powerful telescopes.
  • Some structures have no defined limits, or endpoints. All structures are believed to be part of the cosmic web, which is a conclusive idea.{{clarify|date=May 2023}} Most structures are overlapped by nearby galaxies, creating a problem of how to carefully define the structure's limit.
  • Interpreting the observational data requires assumptions about gravitational lensing, redshift, etc.

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List of largest structures

{{sticky header}}

class="wikitable sortable sticky-header"

|+List of the largest cosmic structures

style="background:#efefef; white-space:nobr;"| Structure name
(year discovered)

! style="background:#ffdead;"| Maximum dimension
(in light-years)

! class="unsortable"|Notes

Hercules–Corona Borealis Great Wall (2014){{cite journal|last1=Horvath|first1=Istvan|last2=Bagoly|first2=Zsolt|last3=Hakkila|first3=Jon|last4=Tóth|first4=L. Viktor|title=Anomalies in the GRB spatial distribution|journal=Proceedings of Science|pages=78|arxiv=1507.05528|bibcode = 2014styd.confE..78H |year=2014|doi=10.22323/1.233.0078 |doi-access=free }}9,700,000,000–10,000,000,000{{cite journal|last1=Horvath|first1=Istvan|last2=Hakkila|first2=Jon|last3=Bagoly|first3=Zsolt|date=2014|title=Possible structure in the GRB sky distribution at redshift two|journal=Astronomy & Astrophysics|volume=561|pages=id.L12|arxiv=1401.0533|bibcode=2014A&A...561L..12H|doi=10.1051/0004-6361/201323020|s2cid=24224684}}{{cite journal|last1=Horvath|first1=I.|last2=Hakkila|first2=J.|last3=Bagoly|first3=Z.|date=2013|title=The largest possible structure of the Universe, defined by Einstein in his Big Bang theory (1901).|journal=7th Huntsville Gamma-Ray Burst Symposium, GRB 2013: Paper 33 in EConf Proceedings C1304143|volume=1311|pages=1104|arxiv=1311.1104|bibcode=2013arXiv1311.1104H}}{{cite web|title=Universe's Largest Structure is a Cosmic Conundrum|url=http://news.discovery.com/space/galaxies/universes-largest-structure-is-a-cosmic-conundrum-131119.htm|last=Klotz|first=Irene|date=2013-11-19|publisher=discovery|url-status=dead|archive-url=https://web.archive.org/web/20150325183452/http://news.discovery.com/space/galaxies/universes-largest-structure-is-a-cosmic-conundrum-131119.htm|archive-date=2015-03-25|access-date=2013-11-22}}Discovered through gamma-ray burst mapping. Existence as a structure is disputed.{{Cite journal|last=Christian|first=Sam|date=2020-07-11|title=Re-examining the evidence of the Hercules–Corona Borealis Great Wall|url=https://academic.oup.com/mnras/article/495/4/4291/5843300|journal=Monthly Notices of the Royal Astronomical Society|language=en|volume=495|issue=4|pages=4291–4296|doi=10.1093/mnras/staa1448|doi-access=free |issn=0035-8711|arxiv=2006.00141|s2cid=219177572}}{{Cite journal|last1=Ukwatta|first1=T. N.|last2=Woźniak|first2=P. R.|date=2016-01-01|title=Investigation of redshift- and duration-dependent clustering of gamma-ray bursts|url=https://academic.oup.com/mnras/article/455/1/703/986230|journal=Monthly Notices of the Royal Astronomical Society|language=en|volume=455|issue=1|pages=703–711|doi=10.1093/mnras/stv2350|issn=0035-8711|doi-access=free|arxiv=1507.07117}}{{Cite journal|last1=Horvath|first1=I.|last2=Szecsi|first2=D.|last3=Hakkila|first3=J.|last4=Szabo|first4=A.|last5=Racz|first5=I.I.|last6=Toth|first6=L.V.|last7=Pinter|first7=S.|last8=Bagoly|first8=Z.|date=2020-08-22|title=The clustering of gamma-ray bursts in the Hercules-Corona Borealis Great Wall: the largest structure in the Universe?|url=https://academic.oup.com/mnras/article/498/2/2544/5895980|journal=Monthly Notices of the Royal Astronomical Society|language=en|volume=498|issue=2|pages=2544–2553|doi=10.1093/mnras/staa2460 |arxiv=2008.03679|issn=0035-8711|doi-access=free}}
Giant GRB Ring (2015){{cite journal |last1=Balazs |first1=L. G. |last2=Bagoly |first2=Z. |last3=Hakkila |first3=J. E. |last4=Horvath |first4=I. |last5=Kobori |first5=J. |last6=Racz |first6=I. I. |last7=Toth |first7=L. V. |date=2015-08-05 |title=A giant ring-like structure at 0.78 < z < 0.86 displayed by GRBs |journal=Monthly Notices of the Royal Astronomical Society |volume=452 |issue=3 |pages=2236–2246 |arxiv=1507.00675 |bibcode=2015MNRAS.452.2236B |doi=10.1093/mnras/stv1421 |s2cid=109936564 |doi-access=free}}5,600,000,000Discovered through gamma-ray burst mapping. Largest-known regular formation in the observable universe.
Huge-LQG (2012–2013)4,000,000,000{{cite journal|last=Aron|first=Jacob|title=Largest structure challenges Einstein's smooth cosmos|journal=New Scientist|volume=217|issue=2900|pages=13|url=https://www.newscientist.com/article/dn23074-largest-structure-challenges-einsteins-smooth-cosmos.html|access-date=14 January 2013|bibcode=2013NewSc.217...13A|year=2013|doi=10.1016/S0262-4079(13)60143-8|url-access=subscription}}{{cite web|title=Astronomers discover the largest structure in the universe|url=http://www.ras.org.uk/news-and-press/224-news-2013/2212-astronomers-discover-the-largest-structure-in-the-universe|publisher=Royal astronomical society|access-date=2013-01-13|archive-url=https://web.archive.org/web/20130114020821/http://www.ras.org.uk/news-and-press/224-news-2013/2212-astronomers-discover-the-largest-structure-in-the-universe|archive-date=2013-01-14|url-status=dead}}{{cite journal | arxiv=1211.6256 | bibcode=2013MNRAS.429.2910C | title=A structure in the early Universe at z ~ 1.3 that exceeds the homogeneity scale of the R-W concordance cosmology | date=2013-01-11 |last1=Clowes|first1=Roger |first2=Kathryn A. | last2=Harris|first3=Srinivasan | last3=Raghunathan|first4=Luis E. | last4=Campusano|first5=Ilona K. | last5=Söchting|first6=Matthew J. | last6=Graham | journal=Monthly Notices of the Royal Astronomical Society | volume=1211 | pages=6256 | doi=10.1093/mnras/sts497 | issue=4| doi-access=free | s2cid=486490 }}Decoupling of 73 quasars. Largest-known large quasar group and the first structure found to exceed 3 billion light-years.
"Giant Arc" (2021)3,300,000,000{{cite web | url =https://koliasa.com/giant-arc-stretching-1-3-billion-light-years-across-the-cosmos-shouldnt-exist/ | title =Giant arc stretching-1.3 billion light-years across the cosmos shouldn't exist | access-date =2021-06-16 | archive-date =2021-06-28 | archive-url =https://web.archive.org/web/20210628135533/https://koliasa.com/giant-arc-stretching-1-3-billion-light-years-across-the-cosmos-shouldnt-exist/ | url-status =dead }}Located 9.2 billion light years away.
U1.11 LQG (2011)2,500,000,000Involves 38 quasars. Adjacent to the Clowes-Campusano LQG.
Clowes–Campusano LQG (1991)2,000,000,000Grouping of 34 quasars. Discovered by Roger Clowes and Luis Campusano.
Sloan Great Wall (2003)1,380,000,000Discovered through the 2dF Galaxy Redshift Survey and the Sloan Digital Sky Survey.
South Pole Wall (2020)1,370,000,000{{cite journal |author=Pomarède, Daniel |display-authors=et al. |title=Cosmicflows-3: The South Pole Wall |date=10 July 2020 |journal=The Astrophysical Journal |volume=897 |number=2 |page=133 |doi=10.3847/1538-4357/ab9952 |arxiv=2007.04414 |bibcode=2020ApJ...897..133P |s2cid=220425419 |doi-access=free }}{{cite news |author=Pomerede |first=Daniel |display-authors=et al. |date=January 2020 |title=The South Pole Wall |work=Harvard University |pages=453.01 |bibcode=2020AAS...23545301P}}{{cite news |author= |title=Astronomers map massive structure beyond Laniakea Supercluster |url=https://www.hawaii.edu/news/2020/07/10/laniakea-supercluster-mapping/ |date=10 July 2020 |work=University of Hawaii |access-date=10 July 2020 }}{{cite news |last=Overbye |first=Dennis |author-link=Dennis Overbye |date=10 July 2020 |title=Beyond the Milky Way, a Galactic Wall – Astronomers have discovered a vast assemblage of galaxies hidden behind our own, in the "zone of avoidance" |url=https://www.nytimes.com/2020/07/10/science/astronomy-galaxies-attractor-universe.html |access-date=10 July 2020 |work=The New York Times}}{{cite news |last=Mann |first=Adam |title=Astronomers discover South Pole Wall, a gigantic structure stretching 1.4 billion light-years across |url=https://www.livescience.com/south-pole-wall-discovered-in-space.html |date=10 July 2020 |work=Live Science |access-date=10 July 2020 }}{{cite news |last=Starr |first=Michelle |title=A Giant 'Wall' of Galaxies Has Been Found Stretching Across The Universe |url=https://www.sciencealert.com/a-giant-wall-of-galaxies-has-been-found-stretching-across-the-universe |date=14 July 2020 |work=ScienceAlert.com |access-date=19 July 2020 }}The largest contiguous feature in the local volume and comparable to the Sloan Great Wall (see above) at half the distance. It is located at the celestial South Pole.
King Ghidorah Supercluster (2022)1,300,000,000Consists of at least 15 clusters plus other interconnected filaments. It is the most massive galaxy supercluster discovered so far.{{Cite journal|last1=Shimawaka|first1=Rhythm|last2=Okabe|first2=Nobuhiro|last3=Shirasaki|first3=Masat|last4=Tanaka|first4=Masayuki|date=22 November 2022|title=King Ghidorah Supercluster: Mapping the light and dark matter in a new supercluster at z = 0.55 using the subaru hyper suprime-cam|journal=Monthly Notices of the Royal Astronomical Society: Letters|volume=519|issue=1|pages=L45–L50|url=https://academic.oup.com/mnrasl/article-abstract/519/1/L45/6847752?redirectedFrom=fulltext|url-access=subscription|bibcode=2023MNRAS.519L..45S|doi=10.1093/mnrasl/slac150|doi-access=free |arxiv=2211.11970|s2cid=253761264|issn=1745-3933}}
Big Ring (2024)

|1,300,000,000

|Made up of galaxy clusters.

style="background:#efefef;"| (Theoretical limit)

| style="background:#efefef;"| 1,200,000,000

| style="background:#efefef;"| Structures larger than this size are incompatible with the cosmological principle according to all estimates. However, whether the existence of these structures itself constitutes a refutation of the cosmological principle is still unclear.{{Cite journal|last=Nadathur|first=Seshadri|date=10 July 2018|title=Seeing patterns in noise: Gigaparsec-scale 'structures' that do not violate homogeneity|journal=Monthly Notices of the Royal Astronomical Society|volume=434|issue=1 |pages=398–406|doi=10.1093/mnras/stt1028|doi-access=free |arxiv=1306.1700|bibcode=2013MNRAS.434..398N |s2cid=119220579}}

Ho'oleilana Bubble (2023)

|1,000,000,000

|Contains about 56,000 galaxies, located 820 million light years away.

BOSS Great Wall (BGW) (2016)1,000,000,000Structure consisting of 4 superclusters of galaxies. The mass and volume exceeds the amount of the Sloan Great Wall.{{Cite journal |author1=Lietzen |first=H. |author2=Tempel |first2=E. |author3=Liivamägi |first3=L. J. |date=20 March 2016 |title=Discovery of a massive supercluster system at z ~ 0.47 |journal=Astronomy & Astrophysics |volume=588 |page=L4 |arxiv=1602.08498 |bibcode=2016A&A...588L...4L |doi=10.1051/0004-6361/201628261 |s2cid=56126854}}
Perseus–Pegasus Filament (1985)1,000,000,000This galaxy filament contains the Perseus–Pisces Supercluster.
Pisces–Cetus Supercluster Complex (1987)1,000,000,000Contains the Milky Way, and is the first galaxy filament to be discovered. (The first LQG was found earlier in 1982.) A new report in 2014 confirms the Milky Way as a member of the Laniakea Supercluster.
CfA2 Great Wall (1989)750,000,000Also known as the Coma Wall.
Saraswati Supercluster652,000,000{{Cite web|url=http://www.iucaa.in/Saraswati-General.html|title=News {{pipe}} IUCAA|website=www.iucaa.in}}The Saraswati Supercluster consists of 43 massive galaxy clusters, which include Abell 2361 and ZWCl 2341.1+0000.
Boötes Supercluster620,000,000
Horologium-Reticulum Supercluster (2005)550,000,000Also known as the Horologium Supercluster.
Laniakea Supercluster (2014)520,000,000Galaxy supercluster in which Earth is located.
Komberg–Kravtsov–Lukash LQG 11500,000,000Discovered by Boris V. Komberg, Andrey V. Kravstov and Vladimir N. Lukash.{{cite journal | last1 = Komberg | first1 = Boris V. | last2 = Kravtsov | first2 = Andrey V. | last3 = Lukash | first3 = Vladimir N. | title = The search and investigation of the Large Groups of Quasars | journal = Monthly Notices of the Royal Astronomical Society | url =https://archive.org/details/arxiv-astro-ph9602090| page = 2090 |arxiv=astro-ph/9602090 | bibcode=1996MNRAS.282..713K| year = 1996 | volume = 282 | issue = 3 | doi = 10.1093/mnras/282.3.713 | doi-access = free | s2cid = 14700144 }}
Hyperion proto-supercluster (2018)489,000,000The largest and earliest known proto– supercluster.
Komberg–Kravtsov–Lukash LQG 12480,000,000Discovered by Boris V. Komberg, Andrey V. Kravstov and Vladimir N. Lukash.
Newman LQG (U1.54)450,000,000Discovered Peter R Newman{{cite thesis |last1=Newman |first1=Peter R. |title=Large groups of quasars in an ultraviolet-excess survey |date=1999 |publisher=University of Central Lancashire |url=http://doi.org/10.17030/uclan.thesis.00020658 |doi=10.17030/uclan.thesis.00020658 |bibcode=1999PhDT..........N}} et al.
Komberg–Kravtsov–Lukash LQG 5430,000,000Discovered by Boris V. Komberg, Andrey V. Kravstov and Vladimir N. Lukash.
Tesch–Engels LQG420,000,000
Shapley Supercluster400,000,000First identified by Harlow Shapley as a cloud of galaxies in 1930, it was not identified as a structure until 1989.
Komberg–Kravstov–Lukash LQG 3390,000,000Discovered by Boris V. Komberg, Andrey V. Kravstov and Vladimir N. Lukash.
U1.90380,000,000
Lynx–Ursa Major Filament (LUM Filament)370,000,000
Sculptor Wall370,000,000Also known as the Southern Great Wall.
Einasto Supercluster360,000,000{{Cite journal |last1=Sankhyayan |first1=Shishir |last2=Okabe |first2=Joydeep |last3=Tempel |first3=Elmo |last4=More |first4=Surhud |last5=Einasto |first5=Maret |last6=Dabhade |first6=Pratik |last7=Raychaudhury |first7=Somak |last8=Athreya |first8=Ramana |last9=Heinämäki |first9=Pekka |date=13 November 2023 |title=Identification of Superclusters and Their Properties in the Sloan Digital Sky Survey Using the WHL Cluster Catalog |journal=The Astrophysical Journal |volume=958 |issue=1 |page=62 |arxiv=2309.06251 |bibcode=2023ApJ...958...62S |doi=10.3847/1538-4357/acfaeb |doi-access=free }}
Pisces-Cetus Supercluster350,000,000
Komberg–Kravtsov–Lukash LQG 2350,000,000Discovered by Boris V. Komberg, Andrey V. Kravstov and Vladimir N. Lukash.
z=2.38 filament around protocluster ClG J2143-4423330,000,000
Webster LQG320,000,000First LQG (Large Quasar Group) discovered.R. G. Clowes. "Large Quasar Groups – A Short Review". 'The New Era of Wide Field Astronomy', ASP Conference Series, Vol. 232. 2001; Astronomical Society of the Pacific; {{ISBN|1-58381-065-X}}; {{bibcode|2001ASPC..232..108C}}.{{cite journal|last=Webster|first=Adrian|title=The clustering of quasars from an objective-prism survey|journal=Monthly Notices of the Royal Astronomical Society|date=May 1982|volume=199|issue=3|pages=683–705|bibcode=1982MNRAS.199..683W|doi=10.1093/mnras/199.3.683|doi-access=free}}
Komberg–Kravtsov–Lukash LQG 8310,000,000Discovered by Boris V. Komberg, Andrey V. Kravstov and Vladimir N. Lukash.
Komberg–Kravtsov–Lukash LQG 1280,000,000Discovered by Boris V. Komberg, Andrey V. Kravstov and Vladimir N. Lukash.
Komberg–Kravtsov–Lukash LQG 6260,000,000Discovered by Boris V. Komberg, Andrey V. Kravstov and Vladimir N. Lukash.
Komberg–Kravtsov–Lukash LQG 7250,000,000Discovered by Boris V. Komberg, Andrey V. Kravstov and Vladimir N. Lukash.
SCL @ 1338+27228,314,341One of the most distant known superclusters.
Komberg–Kravtsov–Lukash LQG 9200,000,000Discovered by Boris V. Komberg, Andrey V. Kravstov and Vladimir N. Lukash.
SSA22 Protocluster200,000,000Giant collection of Lyman-alpha blobs.
Ursa Major Supercluster200,000,000
nowrap="nowrap"| Komberg-Kravtsov-Lukash LQG 10180,000,000Discovered by Boris V. Komberg, Andrey V. Kravstov and Vladimir N. Lukash.
style="background:pink;" class="sortbottom"

| Virgo Supercluster

110,000,000A part of the Laniakea Supercluster (see above). It also contains the Milky Way Galaxy, which contains the Solar System where Earth orbits the Sun.
Listed here for reference.

{{Anchor|List of largest-known voids}}

List of largest voids

{{seealso|List of voids}}

Voids are immense spaces between galaxy filaments and other large-scale structures. Technically they are not structures. They are vast spaces which contain very few or no galaxies. They are theorized to be caused by quantum fluctuations during the early formation of the universe.

A list of the largest voids so far discovered is below. Each is ranked according to its longest dimension.

class="wikitable sortable sticky-header"

|+List of the largest voids

! style="background:#efefef; white-space:nobr;"| Void name/designation

! style="background:#ffdead;"| Maximum dimension
(in light-years)

! class="unsortable"|Notes

LOWZ North 13788 void2,953,000,000One of largest known voids, containing 109,066 known galaxies.{{Cite journal |arxiv = 1602.02771|doi = 10.3847/1538-4357/835/2/161|title = A Cosmic Void Catalog of SDSS DR12 BOSS Galaxies|year = 2017|last1 = Mao|first1 = Qingqing|last2 = Berlind|first2 = Andreas A.|last3 = Scherrer|first3 = Robert J.|last4 = Neyrinck|first4 = Mark C.|last5 = Scoccimarro|first5 = Román|last6 = Tinker|first6 = Jeremy L.|last7 = McBride|first7 = Cameron K.|last8 = Schneider|first8 = Donald P.|last9 = Pan|first9 = Kaike|last10 = Bizyaev|first10 = Dmitry|last11 = Malanushenko|first11 = Elena|last12 = Malanushenko|first12 = Viktor|journal = The Astrophysical Journal|volume = 835|issue = 2|page = 161|bibcode = 2017ApJ...835..161M|s2cid = 119098071 | doi-access=free }}
Local Hole2,000,000,000Proposed void containing the Milky Way galaxy and Local Group as an explanation for the discrepancy in the Hubble constant. Existence is still disputed.{{Cite journal|last1=Kenworthy|first1=W. D'Arcy|last2=Scolnic|first2=Dan|last3=Riess|first3=Adam|date=2019-04-24|title=The Local Perspective on the Hubble Tension: Local Structure Does Not Impact Measurement of the Hubble Constant|journal=The Astrophysical Journal|volume=875|issue=2|pages=145|doi=10.3847/1538-4357/ab0ebf|issn=1538-4357|arxiv=1901.08681|bibcode=2019ApJ...875..145K|s2cid=119095484 |doi-access=free }}{{Cite journal|title=The KBC void and Hubble tension contradict $\Lambda$CDM on a Gpc scale $-$ Milgromian dynamics as a possible solution|first1=Moritz|last1=Haslbauer|first2=Indranil|last2=Banik|first3=Pavel|last3=Kroupa|date=October 23, 2020|journal=Monthly Notices of the Royal Astronomical Society|volume=499|issue=2|pages=2845–2883|doi=10.1093/mnras/staa2348|doi-access=free |arxiv=2009.11292|bibcode=2020MNRAS.499.2845H }}
LOWZ North 4739 void1,846,000,000
LOWZ North 16634 void1,671,000,000
LOWZ North 11627 void1,663,000,000
LOWZ South 4653 void1,610,000,000
LOWZ North 13222 void1,515,000,000
Giant Void1,300,000,000Also known as Canes Venatici Supervoid
LOWZ North 14348 void1,277,000,000
LOWZ South 5589 void1,110,000,000
LOWZ North 13721 void1,095,000,000
LOWZ North 11918 void998,000,000
LOWZ North 5692 void984,000,000
nowrap="nowrap"| Bahcall & Soneira 1982 void978,000,000This suspected void ranged 100 degrees across the sky, and has shown up on other surveys as several separate voids.Bahcall, N. A.; Soneira, R. M. (1982) [http://articles.adsabs.harvard.edu/cgi-bin/nph-iarticle_query?1982ApJ...262..419B&data_type=PDF_HIGH&whole_paper=YES&type=PRINTER&filetype=.pdf "An approximately 300 MPC void of rich clusters of galaxies"] (PDF) Astrophysical Journal, Part 1, vol. 262, Nov. 15, 1982, p. 419-423. {{bibcode|1982ApJ...262..419B}} {{doi|10.1086/160436}}
LOWZ North 11446 void944,000,000
LOWZ North 15734 void938,000,000
LOWZ North 16394 void934,000,000
LOWZ North 8541 void917,000,000
LOWZ South 4775 void899,000,000
LOWZ North 12092 void891,000,000
LOWZ North 3294 void887,000,000
Tully-11 void880,000,000Catalogued by R. Brent Tully
CMASS South 7225 void865,000,000
LOWZ North 14775 void848,000,000
LOWZ South 6334 void846,000,000
LOWZ North 10254 void843,000,000
LOWZ North 13568 void841,000,000
LOWZ North 11954 void827,000,000
LOWZ North 3404 void812,000,000
LOWZ South 3713 void805,000,000
LOWZ South 4325 void804,000,000
CMASS South 5582 void796,000,000
Tully-10 void792,000,000Catalogued by R. Brent Tully
LOWZ North 6177 void789,000,000
Tully-9 void746,000,000Catalogued by R. Brent Tully
B&B Abell-20 void684,000,000
B&B Abell-9 void652,000,000
Tully-7 void567,240,000Catalogued by R. Brent Tully
Tully-4 void564,000,000Catalogued by R. Brent Tully
Tully-6 void557,460,000Catalogued by R. Brent Tully
Tully-8 void554,200,000Catalogued by R. Brent Tully
B&B Abell-21 void521,600,000
B&B Abell-28 void521,600,000
Eridanus Supervoid489,000,000
(most likely value)
A recent analysis of the Wilkinson Microwave Anisotropy Probe (WMAP) in 2007 has found an irregularity of the temperature fluctuation of the cosmic microwave background within the vicinity of the constellation Eridanus with analysis found to be 70 microkelvins cooler than the average CMB temperature. One speculation is that a void could cause the cold spot, with the possible size on the left. However, it may be as large as 1 billion light-years, close to the size of the Giant Void.
B&B Abell-4 void489,000,000
B&B Abell-15 void489,000,000
Tully-3 void489,000,000Catalogued by R. Brent Tully
1994EEDTAWSS-10 void469,440,000
Tully-1 void456,400,000Catalogued by R. Brent Tully
B&B Abell-8 void456,000,000
B&B Abell-22 void456,000,000
Tully-2 void443,360,000Catalogued by R. Brent Tully
B&B Abell-24 void423,800,000
B&B Abell-27 void423,800,000
CMASS North 4407 void414,000,000
B&B Abell-7 void391,200,000
B&B Abell-12 void391,200,000
B&B Abell-29 void391,200,000
1994EEDTAWSS-21 void378,160,000
Southern Local Supervoid365,120,000
B&B Abell-10 void358,600,000
B&B Abell-11 void358,600,000
B&B Abell-13 void358,600,000
B&B Abell-17 void358,600,000
B&B Abell-19 void358,600,000
B&B Abell-23 void358,600,000
CMASS North 11496 void342,000,000
1994EEDTAWSS-19 void342,100,000
Northern Local Supervoid339,000,000Virgo Supercluster, Coma Supercluster, Perseus–Pisces Supercluster, Ursa Major-Lynx Supercluster, Hydra–Centaurus Supercluster, Sculptor Supercluster, Pavo–Corona Australis 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 separate the Northern Local Void and Southern Local Void from the Pegasus Void.Einasto, Jaan; Einasto, Maret; Gramann, Mirt (1989) [http://cdsads.u-strasbg.fr/cgi-bin/nph-iarticle_query?1989MNRAS.238..155E&data_type=PDF_HIGH&whole_paper=YES&type=PRINTER&filetype=.pdf "Structure and formation of superclusters. IX – Self-similarity of voids"] (PDF). Royal Astronomical Society, Monthly Notices (ISSN 0035-8711), vol. 238, May 1, 1989, pp. 155–177. {{bibcode|1989MNRAS.238..155E}}.
Boötes Void330,000,000Also known as The Giant Nothing
1994EEDTAWSS-12 void328,000,000
CMASS North 15935 void252,000,000
SSRS1 4 void217,000,000
GACIRASS V0 void215,000,000
CMASS North 60 void210,000,000
SSRS2 3 void198,000,000
Local Void195,000,000The nearest void to the Milky Way.
SSRS2 1 void177,000,000
IRAS 1 void166,000,000
Sculptor void163,000,000
IRAS 3 void145,000,000
IRAS 2 void142,000,000
IRAS 7 void141,000,000
SSRS2 11 void139,000,000
IRAS 6 void135,000,000
IRAS 13 void131,000,000
Pegasus Void130,000,000S. A. Pustilnik (SAO), D. Engels (Hamburg), A. Y. Kniazev (ESO, SAO), A. G. Pramskij, A. V. Ugryumov (SAO), H.-J. Hagen (Hamburg) (2005). ["HS 2134+0400 – new very metal-poor galaxy, a representative of void population?"]. arXiv:astro-ph/0508255v1. {{bibcode|2006AstL...32..228P}} {{doi|10.1134/S1063773706040025}}. The Perseus–Pisces Supercluster and Pegasus Supercluster form a sheet separate the Northern Local Void and Southern Local Void from the Pegasus Void.
IRAS 8 void128,000,000
SSRS2 9 void127,000,000
IRAS 9 void117,000,000
IRAS 5 void117,000,000
SSRS2 4 void116,000,000
SSRS2 10 void113,000,000
SSRS1 1 void108,000,000Located just behind the galaxy concentration Eridanus-Fornax-Dorado.
IRAS 11 void104,000,000
SSRS2 6 void104,000,000
CMASS North 10020 void104,000,000
IRAS 12 void102,000,000
Perseus-Pisces void99,000,000
SSRS1 2 void97,000,000
IRAS 14 void93,000,000
SSRS2 8 void90,000,000
SSRS2 15 void89,000,000
GACIRASS V1 void83,000,000
SSRS2 7 void83,000,000
SSRS2 12 void81,000,000
GACIRASS V3 void81,000,000
SSRS2 14 void69,000,000
SSRS2 18 void68,000,000
SSRS2 16 void66,000,000
GACIRASS V2 void63,000,000
SSRS2 17 void61,000,000

See also

References

{{reflist|30em}}

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*

Structures, largest

Largest structures

cosmic structures