Laniakea Supercluster


The Laniakea Supercluster or Laniakea for short is the large-scale structure centered around the Great Attractor that is home to the Milky Way and approximately 100,000 other nearby galaxies. It was originally defined in September 2014 as a galaxy supercluster, when a group of astronomers, including R. Brent Tully of the University of Hawaiʻi at Mānoa, Hélène Courtois of the University of Lyon, Yehuda Hoffman of the Hebrew University of Jerusalem, and Daniel Pomarède of CEA Université Paris-Saclay published a new way of defining superclusters according to the relative velocities of galaxies as basins of attraction. The new definition of the Local Supercluster subsumes the then prior defined Virgo and Hydra-Centaurus Supercluster as appendages, the former being the historical local supercluster.
Follow-up studies suggest that the Laniakea is not gravitationally bound. It will disperse rather than continue to maintain itself as an overdensity relative to surrounding areas. In addition, some papers favored the traditional definition of superclusters as high-density regions of the cosmic web; basins of attraction including Laniakea were therefore proposed to be called "supercluster cocoons", containing smaller traditional superclusters, which evolve inside their parent cocoon.
The Laniakea is the inner part of the local superstructure, also known as Pisces–Cetus Supercluster Complex. Both are among the largest known cosmic structures in the observable universe. Latest observations of basins of attraction suggested a basin of attraction around Ophiuchus Cluster may be associated with Laniakea, and also have found both are moving toward the Shapley Concentration and may thus be part of this greater structure.

Name

The name laniākea means 'immense heaven' in Hawaiian],. The name was suggested by Nawaʻa Napoleon, an associate professor of Hawaiian language at Kapiʻolani Community College. The name honors Polynesian navigators, who used knowledge of the sky to navigate the Pacific Ocean.

Characteristics

The Laniakea supercluster encompasses approximately 100,000 galaxies stretched out roughly. It has the approximate mass of solar masses, or 100,000 times that of our galaxy, which is almost the same as that of the Horologium Supercluster. It consists of several previously defined subparts, including smaller superclusters based on their traditional defintion:
The most massive galaxy clusters of the Laniakea are Virgo, Hydra, Centaurus, Abell 3565, Abell 3656, Abell 2870, Abell 3581, Abell 3574, Abell 3521, Fornax, Eridanus, Ophiuchus, and Norma. The entire supercluster cocoon consists of approximately 300 to 500 known galaxy clusters and groups. The real number may be much larger because some of these are traversing the Zone of Avoidance, an area of the sky that is partially obscured by gas and dust from the Milky Way galaxy, making them essentially undetectable.
Superclusters are some of the universe's largest structures and have boundaries that are difficult to define, especially from the inside. Within a given supercluster, most galaxy motions will be directed inward, toward the center of mass. This gravitational focal point, in the case of Laniakea, is called the Great Attractor, and influences the motions of the Local Group of galaxies, where the Milky Way galaxy resides, and all others throughout the supercluster. The same study that confirmed the Laniakea proposed to define a supercluster as basins of attraction, rather than high-density regions such as the Virgo Supercluster. Unlike its constituent then-known superclusters, which would collapse in the far future, Laniakea is, however, not gravitationally bound and is projected to be torn apart by dark energy. Follow-up studies favored the traditional definition of superclusters as high-density regions, with referred to basins of attraction such as Laniakea as "supercluster cocoons" or "watershed superclusters". Because there is no community consensus on an agreed defintion of the term supercluster, other studies avoid calling any structure a supercluster, including Laniakea and Shapley, which were referred as simply basins of attraction.
Although confirmation of the existence of the Laniakea supercluster emerged in 2014, early studies in the 1980s already suggested that several of the then-known superclusters might be connected. For example, South African astronomer Tony Fairall stated in 1988 that redshifts suggested that the Virgo and Hydra–Centaurus superclusters may be connected. More recent observations using Cosmicflows-4 catalog have shown that a basin of attraction centered on the Ophiuchus Cluster might be associated with Laniakea, forming a "probabilistic Basin of Attraction".

Location

The neighboring superclusters to the Laniakea are the Shapley, Hercules, Coma, and Perseus–Pisces Superclusters. The edges of the superclusters and Laniakea were not clearly known at the time of Laniakea's definition. Since then, the study of the edges of superclusters and of structures beyond them has substantially improved. Because the Laniakea, Apus, and Coma superclusters are moving toward the Shapley Supercluster, they may be sub-basins part of this larger basin of attraction.
Laniakea is also a constituent part of a much larger local superstructure that has also been proposed by R. Brent Tully, referred to as the Pisces–Cetus Supercluster Complex, a galaxy filament.