Laniakea Supercluster
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Summary
Laniakea Supercluster is a supercluster[1]. It ranks in the top 6% of supercluster entities by monthly Wikipedia readership (8,087 views/month).[2]
Key Facts
- Discoverer or inventor: R. Brent Tully[3], Hélène Courtois[4], Daniel Pomarède[5], Yehuda Hoffman[6]
- Constellation: Triangulum Australe[7]
- Site of astronomical discovery: National Radio Astronomy Observatory[8]
- Part of: Pisces–Cetus Supercluster Complex[9]
- Has part(s): Virgo Supercluster[10], Hydra-Centaurus Supercluster[11], Pavo-Indus Supercluster[12], Great Attractor[13]
- Time of discovery or invention: September 2014[14]
- Topic's main category: Category:Laniakea Supercluster[15]
- Redshift: 0.0708[16]
- Different from: Laniakea[17]
- Diameter: 500,000,000 light-year[18]
Why It Matters
Laniakea Supercluster has Wikipedia articles in 27 language editions, a strong signal of global cultural recognition.[19] It is known by 28 alternative names across languages and contexts.[20]