Laniakea Supercluster
(Laniakea, Local Supercluster)
(group of clusters including the Local Group)
The Laniakea Supercluster (considered the Local Supercluster)
is a supercluster
with 300-500 galaxy clusters, with 100,000 galaxies
including the Milky Way, stretched out over 160 megaparsecs,
with a mass of about 1017 solar masses.
It was defined as such in September 2014 based upon a study
of the velocities of the galaxies.
It combines four groups traditionally labeled superclusters:
A study has suggested it is not gravitationally bound, in which
case it is a matter of nomenclature whether it should be termed a
supercluster.
(galaxy supercluster,local,large scale structure)
Further reading:
https://en.wikipedia.org/wiki/Laniakea_Supercluster
https://www.nature.com/news/earth-s-new-address-solar-system-milky-way-laniakea-1.15819
https://ui.adsabs.harvard.edu/abs/2014Natur.513...71T/abstract
https://ui.adsabs.harvard.edu/abs/2015A%26A...575L..14C/abstract
Referenced by pages:
astronomical quantities
Coma Supercluster
Great Attractor
Hydra-Centaurus Supercluster
Pisces-Cetus Supercluster Complex
Sun
supercluster
Virgo Supercluster
Index