| Laniakea Supercluster | |
|---|---|
A map of the Laniakea Supercluster and its component galaxy clusters
| |
| Observation data (Epoch J2000) | |
| Constellation(s) | Triangulum Australe and Norma (Great Attractor) |
| Right ascension | 10h32m |
| Declination | −46° 00′ |
| Number of galaxies | 100,000–150,000 |
| Parent structure | Pisces–Cetus Supercluster Complex |
| Major axis | 520 million ly (159 Mpc) h−1 67.80 ± 0.77 (H0 from Planck 2013) |
| Redshift | 0.0708 (center) |
| Distance | 250 million ly (77 Mpc) h−1 67.80 ± 0.077 (Great Attractor) (H0 from Planck 2013) |
| Binding mass | 1×1017[1] M☉ |
| Other designations | |
| Local Supercluster, Laniakea, Laniakea Supercluster, Laniakea Complex | |
| See also: Galaxy group, Galaxy cluster, List of galaxy groups and clusters | |
The Laniakea Supercluster (/ˌlɑːni.əˈkeɪ.ə/; Hawaiian for "open skies" or "immense heaven")[2] or the Local Supercluster (LSCorLS) is the galaxy supercluster that is home to the Milky Way and approximately 100,000 other nearby galaxies.
It was defined in September 2014, when a group of astronomers including R. Brent Tully of the University of Hawaiʻi, 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.[3][4] The new definition of the local supercluster subsumes the prior defined Virgo and Hydra-Centaurus Supercluster as appendages, the former being the prior defined local supercluster.[5][6][7][8][9]
Follow-up studies suggest that the Laniakea Supercluster is not gravitationally bound. It will disperse rather than continue to maintain itself as an overdensity relative to surrounding areas.[10]
The name laniākea ([ˈlɐnijaːˈkɛjə]) means 'immense heaven' in Hawaiian, from lani 'heaven', and ākea 'spacious, immeasurable'. The name was suggested by Nawaʻa Napoleon, an associate professor of Hawaiian language at Kapiolani Community College.[11] The name honors Polynesian navigators, who used knowledge of the sky to navigate the Pacific Ocean.[12]
The Laniakea Supercluster encompasses approximately 100,000 galaxies stretched out over 160 Mpc (520 million ly). It has the approximate mass of 1017 solar masses, or 100,000 times that of our galaxy, which is almost the same as that of the Horologium Supercluster.[3] It consists of four subparts, which were known previously as separate superclusters:
The most massive galaxy clusters of the Laniakea Supercluster are Virgo, Hydra, Centaurus, Abell 3565, Abell 3574, Abell 3521, Fornax, Eridanus, and Norma. The entire supercluster 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. Unlike its constituent clusters, Laniakea is not gravitationally bound and is projected to be torn apart by dark energy.[7]
Although the confirmation of the existence of the Laniakea Supercluster emerged in 2014,[3] early studies in the 1980s already suggested that several of the superclusters then known 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.[14]
The neighboring superclusters to the Laniakea Supercluster are the Shapley Supercluster, Hercules Supercluster, Coma Supercluster, and Perseus–Pisces Supercluster. The edges of the superclusters and Laniakea were not clearly known at the time of Laniakea's definition.[6] Since then, the study of the edges of the supercluster and of structures beyond them has substantially improved.[15][16]
Laniakea is itself a constituent part of the Pisces–Cetus Supercluster Complex, a galaxy filament.
Vimeo, "Laniakea Supercluster", Daniel Pomarède, 4 September 2014—video representation of the findings of the discovery paper YouTube, "Laniakea: Our Home Supercluster", Nature Video, 3 September 2014—Redrawing the boundaries of the cosmic map, they redefine our home supercluster and name it Laniakea.
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