Link to full article

The Laniakea Supercluster (/ˌlæni.əˈkeɪ.ə/; Hawaiian for "open skies" or "immense heaven")[2] 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 local supercluster, the Virgo Supercluster, as an appendage.[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.