Local Hole: Difference between revisions

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{{Title notice|Local Hole|Talk:KBC Void#Improving the article}}
{{Short description|Large, comparatively empty region of space}}
{{Short description|Large, comparatively empty region of space}}
[[File:Kbc_void.png|thumb|Artist's conception of the KBC Void and the [[Galaxy_filament|filaments]] and walls that surround it.]]
[[File:Kbc_void.png|thumb|Artist's conception of the KBC Void and the [[Galaxy_filament|filaments]] and walls that surround it.]]

Revision as of 23:43, 4 March 2022

Artist's conception of the KBC Void and the filaments and walls that surround it.

The KBC Void (or Local Hole) is an immense, comparatively empty region of space, named after astronomers Ryan Keenan, Amy Barger, and Lennox Cowie, who studied it in 2013.[1] The existence of a local underdensity has been the subject of many pieces of literature and research articles.[2][3]

The underdensity is proposed to be roughly spherical, approximately 2 billion light-years (600 megaparsecs, Mpc) in diameter. As with other voids, it is not completely empty but contains the Milky Way, the Local Group, and a larger part of the Laniakea Supercluster. The Milky Way is within a few hundred million light-years of the void's center.[4]

The existence of supervoids have been shown to be consistent with the

MOND gravity rather than general relativity.[8]

See also

References

Further reading