☰ Contents · Astronomy

Quasars, the expanding Universe and large-scale structure

Lessons 60–62 · 3 lessons · M. Mamadazimov. Astronomy Grade 11, 1st edition. DAVR NASHRIYOTI, Tashkent, 2018
62

The distribution of galaxies in the Universe

Textbook: pp. 132–133
GoalExplain the large-scale distribution of galaxies in clusters, superclusters, filaments and voids.
New words
galaxy cluster · galaktikalar to‘dasisupercluster · o‘ta to‘davoid · bo‘shliqcosmic web · kosmik to‘r
Explanation

Galaxies are not scattered evenly: they form groups (the Local Group, ≈ 80 galaxies) and clusters (the Virgo Cluster at ≈ 16.5 Mpc, ≈ 1300–2000 galaxies). Clusters join into superclusters: the Local Group belongs to the Virgo Supercluster, which lies within the still larger Laniakea Supercluster (≈ 160 Mpc across, ≈ 10¹⁷ M☉). On the largest scales galaxies lie along filaments and walls, between which are almost empty voids tens to hundreds of Mpc across – the cosmic web (the Great Wall, 1989). On scales larger than ≈ 100–300 Mpc the Universe is homogeneous and isotropic – the cosmological principle. Dark matter’s gravity was decisive in forming the web, whose seeds were tiny irregularities of ≈ 10⁻⁵ in the cosmic microwave background. 3D maps are made from galaxy redshifts (SDSS, DESI).

Worked examples
The Virgo Cluster at d ≈ 16.5 Mpc: 16.5 · 3.26 ≈ 54 million light-years; by Hubble’s law v ≈ 70 · 16.5 = 1155 km/s.
Across a 100 Mpc filament the Hubble flow differs by 70 km/s/Mpc · 100 Mpc = 7000 km/s – which is why distances can be mapped from redshifts.
Class activity

Structure model: think of a kitchen sponge, holes as voids and walls as filaments; sprinkle a safe fine material (salt) onto it and discuss how galaxies are distributed. Use safe materials only.

Practice
1
Which supercluster does the Local Group belong to?
2
A galaxy at 100 Mpc has v = 70 · 100 km/s. How many km/s is that?
3
What is the cosmological principle?
4
Why can galaxy maps be built from redshifts?