A Field Guide to Laniakea

The Local Universe Organized by Cosmic Web Topology

4 Superclusters·27 Structural Regions·128 Galaxy Groups·~500 Mly

Laniakea Basin — Elevation View
Laniakea Basin elevation view showing 122 galaxy groups across four superclusters plotted in supergalactic SGY vs SGZ coordinates

In 2014, Tully et al. defined Laniakea — a basin of attraction spanning approximately 500 million light-years that contains the Milky Way along with tens of thousands of other galaxies. Named "immeasurable heaven" in Hawaiian, Laniakea was mapped using velocity-watershed analysis of the Cosmicflows catalog: tracing how galaxies flow under gravity to identify dynamically coherent regions, much like mapping river drainage basins on Earth. The technique revealed that the Virgo Supercluster — long thought to be our home supercluster — constitutes only one lobe of a much larger structure.

This field guide proposes a hierarchical framework for organizing Laniakea's contents. The basin comprises four major supercluster lobes — Virgo, Hydra, Centaurus, and Pavo-Indus — each anchored by massive galaxy clusters, yet unified by convergent velocity flows toward a common gravitational core in the Norma-Centaurus region: the Great Attractor. The framework distinguishes basins of attraction (velocity-watershed-defined regions like Laniakea) from superclusters (the overdensity lobes within them), resolving a longstanding ambiguity in cosmographic terminology.

Rather than organizing galaxies by distance or brightness, the framework catalogs 128 galaxy groups containing approximately 718 galaxies into 27 structural regions defined by cosmic web topology — sheets, filaments, clusters, walls, streams, clouds, and void boundaries — prioritizing physical relationships and gravitational flow dynamics to reveal how structures relate within the flowing architecture of the cosmic web.

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Laniakea Basin — Top-Down View
Laniakea Basin top-down view showing 122 galaxy groups across four superclusters plotted in supergalactic SGY vs SGX coordinates

Laniakea's four superclusters exhibit convergent velocity flows toward the Great Attractor in the Norma-Centaurus region — the defining characteristic of the basin. The Virgo Supercluster flows southeastward toward this convergence point, Hydra and Centaurus contribute major flow streams from the south, and Pavo-Indus flows northward from the basin's far periphery. This convergent pattern, revealed through Cosmicflows velocity field analysis, demonstrates that these four superclusters are not independent structures but interconnected components of a unified dynamical system.

Virgo Supercluster

~0–110 Mly · ~1015 M · 10 Regions · 72 Galaxy Groups
The Virgo Cluster
The Virgo Cluster. Credit: RubinObs/NOIRLab/SLAC/NSF/DOE/AURA, CC BY 4.0
The nearest supercluster lobe and home to the Local Group, the Virgo Supercluster offers the most complete observational data within the Laniakea Basin. Its ten structural regions range from the remarkably flattened Local Sheet — an extremely thin disc just 750,000 light-years thick containing our own Milky Way — through the Local Filament bridging toward the massive Virgo Cluster at the supercluster's gravitational center. Outer concentrations including the Fornax Complex (containing the Fornax and Eridanus clusters) and the Leo Association complete the picture of matter converging from all directions onto this nearest great attractor, while sparse void boundaries mark transitions to the underdense regions between superclusters.
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Hydra Supercluster

~160 Mly · ~1015 M · 6 Regions · 18 Galaxy Groups
The Antlia Cluster
The Antlia Cluster. Credit: Dark Energy Survey/DOE/FNAL/DECam/CTIO/NOIRLab/NSF/AURAImage processing: R. Colombari & M. Zamani (NSF NOIRLab), CC BY 4.0
Centered approximately 160 million light-years distant, the Hydra Supercluster is characterized by prominent streams of galaxy groups feeding into two major clusters. The Antlia Stream serves as the primary structural feature, channeling matter into the Antlia Cluster and the Hydra Cluster (Abell 1060) before continuing as the Hydra-Centaurus Stream — a filamentary bridge flowing toward the basin's gravitational core. The twin-cluster morphology of Virgo and Hydra, connected by intermediate filaments, mirrors the hierarchical patterns observed at both supercluster and basin scales.
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Centaurus Supercluster

~170 Mly · ~1015–1016 M · 5 Regions · 16 Galaxy Groups
The Norma Cluster (Abell 3627)
The Norma Cluster (Abell 3627). Credit: DECaPS/Legacy Surveys/D. Lang (Perimeter Institute) & Meli Thev, CC BY 4.0
The Centaurus Supercluster features the massive Centaurus Wall and the Norma Complex — the region harboring the Great Attractor, the deepest gravitational potential well within Laniakea where flows from all four superclusters converge. The Norma Cluster (Abell 3627), heavily obscured by the Milky Way's Zone of Avoidance, sits at near-zero velocity in the cosmic microwave background rest frame — validation that Laniakea functions as a coherent basin of attraction, and that Norma marks the point where the basin's gravitational flows come to rest. What lies hidden behind the Milky Way's disc remains one of extragalactic astronomy's great open questions.
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Pavo-Indus Supercluster

~220 Mly · ~1015 M · 6 Regions · 20 Galaxy Groups
The most distant and least-characterized of Laniakea's four lobes, the Pavo-Indus Supercluster occupies the basin's southern extremity. Despite severe obscuration by the Zone of Avoidance, it exhibits a distinctive chain-like morphology — an elongated arc stretching from the dense Pavo-Indus Complex through the Telescopium Cloud and continuing as the Pavo-Indus Arch, a filamentary extension bounding the Local Void and connecting Laniakea to the neighboring Perseus-Pisces Basin. Unlike the twin morphology of Virgo and Hydra or the gravitationally consolidated Centaurus lobe, Pavo-Indus traces the basin's outer boundary — the frontier where Laniakea's influence gives way to the next great structure.
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Research Paper

A Hierarchical Framework for Organizing the Laniakea Basin

Bianchini, S.R. (2026)
Preprint · Not peer-reviewed

Abstract

This paper presents a hierarchical organizational framework for cataloging the contents of Laniakea, the basin of attraction containing the Milky Way and Local Group as defined by Tully et al. (2014). While the Laniakea Basin boundaries are well constrained through velocity field analysis, no comprehensive public catalog organizing its principal galaxy groups and structural regions by cosmic web topology has yet been published.

The framework organizes Laniakea's four major supercluster lobes (Virgo, Hydra, Centaurus, and Pavo-Indus) into structural regions defined by cosmic web topology: sheets, filaments, walls, clusters, streams, clouds, and void boundaries. This approach prioritizes physical relationships and gravitational flow dynamics over traditional distance-based or brightness-limited organization, creating an intuitive framework for understanding the large-scale structure of the universe.

Additionally, this work proposes standardized terminology for basin-scale structures and introduces hierarchical categories for organizing galaxy groups within each supercluster. The complete catalog contains ~128 galaxy groups and ~718 individual galaxies organized into 27 major structural regions across the four superclusters.

The framework serves multiple purposes: (1) as an educational tool for teaching cosmic web structure, (2) as an observational reference for amateur astronomers, (3) an organizational standard for future Laniakea studies, and (4) a template methodology for organizing other basins of attraction. The complete catalog is made freely available to enable community use and extension.

Bianchini_2026_Laniakea_Framework.pdf
PDF · 85 pages
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4 Superclusters
27 Structural Regions
~128 Galaxy Groups
~718 Galaxies Cataloged
86 References