Galaxy filament


In cosmology, galaxy filaments are the largest known structures in the universe, consisting of walls of galactic superclusters. These massive, thread-like formations can commonly reach 50 to 80 megaparsecs —with the largest found to date being Quipu, and possibly the still unconfirmed Hercules–Corona Borealis Great Wall at around in length—and form the boundaries between voids. Due to the accelerating expansion of the universe, the individual clusters of gravitationally bound galaxies that make up galaxy filaments are moving away from each other at an accelerated rate; in the far future they will dissolve.
Galaxy filaments form the cosmic web and define the overall structure of the observable universe.

Discovery

Discovery of structures larger than superclusters began in the late 1980s. In 1987, astronomer R. Brent Tully of the University of Hawaii's Institute of Astronomy identified what he called the Pisces–Cetus Supercluster Complex. The CfA2 Great Wall was discovered in 1989, followed by the Sloan Great Wall in 2003.
In January 2013, researchers led by Roger Clowes of the University of Central Lancashire announced the discovery of a large quasar group, the Huge-LQG, which dwarfs previously discovered galaxy filaments in size. In November 2013, using gamma-ray bursts as reference points, astronomers discovered the Hercules–Corona Borealis Great Wall, an extremely large filament measuring more than 10 billion light-years across.

Filaments

The filament subtype of filaments have roughly similar major and minor axes in cross-section, along the lengthwise axis.
FilamentDateMean distanceDimensionNotes
Coma FilamentThe Coma Supercluster lies within the Coma Filament. It forms part of the CfA2 Great Wall.
Perseus–Pegasus Filament1985Connected to the Pisces–Cetus Supercluster, with the Perseus–Pisces Supercluster being a member of the filament.
Ursa Major FilamentConnected to the CfA Homunculus, a portion of the filament forms a portion of the "leg" of the Homunculus.
Lynx–Ursa Major Filament 1999from 2000 km/s to 8000 km/s in redshift spaceConnected to and separate from the Lynx–Ursa Major Supercluster.
z=2.38 filament around protocluster ClG J2143-44232004z=2.38110 MpcA filament the length of the Great Wall was discovered in 2004. As of 2008, it was still the largest structure beyond redshift 2.

  • A short filament was proposed by Adi Zitrin and Noah Brosch—detected by identifying an alignment of star-forming galaxies—in the neighborhood of the Milky Way and the Local Group. The proposal of this filament, and of a similar but shorter filament, were the result of a study by McQuinn et al. based on distance measurements using the TRGB method.

Galaxy walls

The galaxy wall subtype of filaments have a significantly greater major axis than minor axis in cross-section, along the lengthwise axis.

WallDateMean distanceDimensionNotes
CfA2 Great Wall 1989z=0.03058251 Mpc long: 750 Mly long
250 Mly wide
20 Mly thick
This was the first super-large large-scale structure or pseudo-structure in the universe to be discovered. The CfA Homunculus lies at the heart of the Great Wall, and the Coma Supercluster forms most of the homunculus structure. The Coma Cluster lies at the core.
Sloan Great Wall 2003z=0.07804433 Mpc longThis was the largest known galaxy filament to be discovered, until it was eclipsed by the Hercules–Corona Borealis Great Wall found ten years later.
Sculptor Wall 8000 km/s long
5000 km/s wide
1000 km/s deep
The Sculptor Wall is "parallel" to the Fornax Wall and "perpendicular" to the Grus Wall.
Grus WallThe Grus Wall is "perpendicular" to the Fornax and Sculptor Walls.
Fornax WallThe Fornax Cluster is part of this wall. The wall is "parallel" to the Sculptor Wall and "perpendicular" to the Grus Wall.
Hercules–Corona Borealis Great Wall2013z≈23 Gpc long,
150 000 km/s deep
The largest known structure in the universe. This is also the first time since 1991 that a galaxy filament/great wall held the record as the largest known structure in the universe.

Large quasar groups

s are some of the largest structures known. They are theorized to be protohyperclusters/proto-supercluster-complexes/galaxy filament precursors.
LQGDateMean distanceDimensionNotes
Clowes–Campusano LQG
1991z=1.28
It was the largest known structure in the universe from 1991 to 2011, until U1.11's discovery.
U1.112011z=1.11
  • Was the largest known structure in the universe for a few months, until Huge-LQG's discovery.
    Huge-LQG2012z=1.27
  • It was the largest structure known in the universe, until the discovery of the Hercules–Corona Borealis Great Wall found one year later.