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Superclusters are large groups of smaller galaxy groups and clusters and are among the largest structures of the cosmos. They are so large that they are not gravitationally bound and, consequently, partake in the Hubble expansion.


The existence of superclusters indicates that the galaxies in our Universe are not uniformly distributed; most of them are drawn together in groups and clusters, with groups containing up to 50 galaxies and clusters up to several thousand galaxies. Those groups and clusters and additional isolated galaxies in turn form even larger structures called superclusters.

Once thought to be the largest structures in nature, superclusters are now understood to be subordinate to enormous walls or sheets, usually called "filaments", sometimes called "supercluster complexes", "walls" or "sheets", that can span a billion light-years in length, more than 5% of the observable universe. Superclusters themselves can span several hundred million light-years. The typical[clarification needed] speed of a galaxy is about 1000 km/s. Hubble's law implies that typical galaxies would only move about 30 million light-years at that speed in a Hubble time of 1/H, which is approximately the age of the universe. While this is a huge distance in human terms, it is much smaller than the size of superclusters. In an expanding universe, saying that the distance d an object has moved equals its present velocity v times the elapsed time t underestimates d when t is not small compared to 1/H. The calculation above still gives some idea of how long it would take the normal movements of galaxies to form or obliterate these structures, and thus indicates their great age. When we observe superclusters and larger structures today, we learn about the condition of the universe when these superclusters were created. The directions of the rotational axes of galaxies within superclusters also gives us insight into the formation process of galaxies early in the history of the Universe.[1]

According to some astronomers, no clusters of superclusters (“hyperclusters”) are known; the existence of structures larger than superclusters is debated (see Galaxy filament). Interspersed among superclusters are large voids of space in which few galaxies exist. Even though superclusters are the largest structures confirmed, the total number of superclusters leaves possibilities for structural distribution.

Superclusters are frequently subdivided into groups of clusters called galaxy clouds.

List of superclusters

Nearby superclusters

  • z=0.000 (0 light years away)
  • Length = 33 Mpc (110 million light years)
  • Hydra Supercluster
  • Centaurus Supercluster
  • 17h 10m -22°
  • cz=8500-9000 km/s (centre)
  • 18 Mpc x 26 Mpc

Distant superclusters

Far distant superclusters





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