Clusters

Galaxy groups and clusters are the largest known gravitationally boundobjects to have arisen thus far in the process of cosmic structure formation.They form the densest part of the large-scale structure of the Universe. In models for the gravitational formation of structure with cold dark matter, the smallest structures collapse first and eventually build the largest structures, clusters of galaxies. Clusters are then formed relatively recently between 10 billion years ago and now. Groups and clusters may contain ten to thousands of individual galaxies. The clusters themselves are often associated with larger, non-gravitationally bound, groups called superclusters.

Our own Galaxy, the Milky Way, is contained in the Local Group of more than 40 galaxies.


Local group

The Local Group is the galaxy group that includes the Milky Way. The Local Group comprises more than 54 galaxies, most of them dwarf galaxies. Its gravitational center is located somewhere between the Milky Way and the Andromeda Galaxy. The Local Group has a diameter of 10 Mly and has a binary distribution.


Virgo cluster

The Virgo Cluster is a cluster of galaxies whose center is 53.8 ± 0.3 Mly away in the constellation Virgo. Comprising approximately 1300 member galaxies, the cluster forms the heart of the larger Virgo Supercluster, of which the Local Group is an outlying member.
Distance to Earth: 65.23 million light years
Radius: 7.5 million light years
Number of galaxies: ~1500
Brightest member: Messier 49
Coordinates: RA 12h 27m 0s | Dec +12° 43′ 0″
Did you know: The Local Group is on the outskirts of the LS in a small filament extending from the Fornax Cluster to the Virgo Cluster

Virgo super cluster

The Virgo Supercluster or the Local Supercluster is a mass concentration of galaxies containing the Virgo Cluster and Local Group, which in turn contains the Milky Way and Andromeda galaxies. At least 100 galaxy groups and clusters are located within its diameter of 33 megaparsecs.
Did you know: The Virgo Supercluster’s volume is about 7000 times that of the Local Group or 100 billion times that of the Milky Way.

Laniekea supercluster

The Laniakea Supercluster is the galaxy supercluster that is home to the Milky Way and approximately 100,000 other nearby galaxies.
Radius: 250 million light years
Distance to Earth: 251.1 million light years
Number of clusters: 300–500
Coordinates: RA 10h 32m 0s | Dec -46° 0′ 0″
Binding mass: 1×1017 M
Did you know: The Laniakea Supercluster encompasses 100,000 galaxies stretched out over 160 megaparsecs (520 million light-years).

Observable universe

The observable universe is a spherical region of the Universe comprising all matter that can be observed from Earth at the present time, because electromagnetic radiation from these objects has had time to reach Earth since the beginning of the cosmological expansion.
Diameter: 8.8 m (×10^26)
Mass (ordinary matter): 4.5 x 10 51 kg