New Evidence Suggests Milky Way Is Part of a Larger Cosmic Web Tied to Shapley Concentration | Details Inside

New research has led to a new understanding of our galaxy’s position within the universe. The study suggests that the Milky Way may reside in a much larger “basin of attraction” than previously assume.

This discovery challenges what we know about our galactic surroundings, revealing that the supercluster which houses the Milky Way could be up to 10 times bigger than current estimates.

Basins of attraction (BOAs) are gravitational regions, where objects are drawn towards a massive centre.

These BOAs can be visualise as layers within layers.

For example, our Solar System is part of the Milky Way, which belongs to a group of galaxies call as the Local Group, which itself is within larger structures such as the Virgo Cluster and the Laniākea Supercluster.

As per the new study publish in Nature Astronomy, the Milky Way may be part of an even larger structure than Laniākea, potentially connect to the Shapley Concentration.

The Shapley Concentration is a massive cluster of galaxies that has long known but wasn’t previously to affect our galaxy.

This new research suggests that it might have a significant gravitational influence, extending far beyond what we have map so far.

Dr Noam Libeskind, Cosmologist at the Leibniz Institute for Astrophysics Potsdam, notes that expanding our knowledge of the universe reveals more connect and larger cosmic structures than we imagine.

The research team, led by scientists who initially discover Laniākea in 2014, estimates there is around a 60% chance that the Milky Way is part of this larger BOA.

Dr Ehsan Kourkchi, Astronomer at the University of Hawaii, highlight the challenges of cosmic surveys, stating that even the most advance tools might not be enough to capture the full picture of our universe.

ALSO READ  Hubble Uncovers Milky Way’s Gravitational Influence on Large Magellanic Cloud | Details Inside

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