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Scale of galaxies
kpc
Distance between galaxies
Mpc
Visible universe scale
Gpc
Messier catalogue
List of nebulae, galaxies and star clusters
The cosmological principle
The universe is homogeneous and isotropic
Dark matter
Missing mass
Virial theorem
2T + UG = 0
Percentage of dark matter in universe
85%
Percentage of dark matter + dark energy in universe
95%
MACHOs
Massive compact halo objects
WIMPs
Weakly interacting massive particles
“Cold” eg. in Cold dark matter
Short mean free path in the early universe
“Warm” eg. in Warm dark matter
Free streaming length comparable to a proto-dwarf in early universe
“Hot” eg. in Hot dark matter
Free streaming length much larger than the size of a proto-galazy
Dark matter rich regions
Galactic centres and halos