  In this paper we review the main theoretical and experimental achievements in
the field of Dark Matter from the Cosmological and Astrophysical point of view.
We revisit it from the very first surveys of local astrophysical matter, up to
the stringent constraints on matter properties, coming from the last release of
data on cosmological scales. To bring closer and justify the idea of dark
matter, we will go across methods and tools for measuring dark matter
characteristics, and in some cases a combination of methods that provide one of
the greatest direct proofs for dark matter, such as Bullet cluster.
