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Large Scale Structure of the Universe

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Wall

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Walls are large, sheet-like structures of galaxies found in the universe, separating different regions or voids.

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Dark Energy

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Dark energy is a hypothetical form of energy that permeates all of space and tends to accelerate the expansion of the universe. It is thought to be the driving force behind the accelerating universe.

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Galaxy Filament

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Galaxy filaments are the largest known structures in the universe, comprising thread-like formations made up of clusters and superclusters of galaxies.

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Supercluster

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A supercluster is a large group of smaller galaxy clusters or galaxy groups; it is among the largest known structures in the universe.

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Galaxy Cluster

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A galaxy cluster is a structure that consists of hundreds to thousands of galaxies bound together by gravity. They are often found at the intersections of cosmic filaments.

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Galaxy

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A galaxy is a massive, gravitationally bound system of stars, stellar remnants, interstellar gas, dust, and dark matter. The Milky Way is an example, containing our Solar System.

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Galaxy Group

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A galaxy group is a smaller number of galaxies, typically fewer than 50, that are gravitationally bound and often dominated by a single large galaxy.

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Void

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Voids are vast spaces between filaments (the largest-scale structures in the Universe) that contain very few, or possibly no, galaxies. They are a significant component of the large-scale structure of the universe.

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Cosmic Microwave Background (CMB)

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The CMB is the thermal radiation left over from the time of recombination in Big Bang cosmology, providing a snapshot of the oldest light in the universe.

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Dark Matter

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Dark matter is a form of matter thought to account for approximately 85% of the matter in the universe and about a quarter of its total energy density. Its presence is implied by gravitational effects on visible matter and radiation.

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