
| Pisces-Cetus Filament | The Pisces-Cetus Supercluster Complex is a galaxy filament that includes the Virgo Supercluster, to which our galaxy, the Milky Way, belongs. It is over 300 Mpc long, and nearly 50 Mpc wide. |
| Perseus-Pegasus Filament | Adjacent to the Pisces-Cetus filament, it includes the Perseus-Pisces Superclusters, and is, again, around 300 Mpc long. |
| Sloan Great Wall | The Sloan Great Wall was first identified in 2003 as part of the Sloan Digital Sky Survey, and is probably the largest structure in the known Universe. It is around 433 Mpc (c. 1.4 billion light years) long, and around 300 Mpc away, though estimates do vary. Some parts of it are not gravitationally bound together and and may never be, so in some ways, we should not really consider it as a single coherent structure. Nevertheless, it is impressive. Shown in the image to the right with the Shapley Supercluster, and parts of the Pisces-Cetus and Horologium-Reticulum Superclusters. |
| Great (Coma) Wall | Found in 1989, the Great Wall (also called the Coma Wall), is the next largest knownstructure in the Universe. It is a 250 Mpc long, 30 Mpc wide and 6 Mpc thick. It could extend much farther but the gas and dust in the Milky Way's zone of avoidance obscures what can be seen. |
| Centaurus Wall | Conjectural, but could contain the Great Attractor, the Norma Supercluster, the Virgo Supercluster (including the Milky Way and the Local Group of galaxies), as well as the Hydra-Centaurus Supercluster. |
| Sculptor Wall | The map to the right shows the position of the Sculptor Wall, the red curved line, in relation to the Milky Way, which is at the bottom. Courtesy HyperLeda (university of Lyon, France). Towards the bottom, and to the right of the Sculptor Wall, from approximately 100 to 300 light-years, there is a rectangular region with a very low density of galaxies. This is called the Sculptor Void. |