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The Seminar "Dark Matter in Galaxies" was delivered, within the Dark MatterAwareness Week (1-8 December 2010) at 140 institutes in 46 countries and it wasfollowed by 4200 people. A documentation of this worldwide initiative is athttp://www.youtube.com/watch?v=AOBit8a-1Fw. A reference presentation, preparedby a coordinated pool of leading scientists in the field, was available tospeakers. In response to feedbacks and suggestions, we upgraded it to a"Presentation Review" of which we provide here the Explanatory Notes, the linkto the .pptx file, and some image of the slides. This Presentation Review is aninnovative scientific product to meet the request of information about thephenomenology of the DM mystery at galactic scale. This Review concerns themass discrepancy phenomenon detected in galaxies, usually accounted bypostulating the presence of a non luminous non baryonic component. In thetheoretical framework of Newtonian Gravity we recall the properties of DarkMatter halos as emerging from the state-of-the-art of numerical simulationsperformed in the current $\Lambda CDM$ scenario. Then, the simple butmuch-telling phenomenology of the distribution of dark and luminous matter inSpirals, Ellipticals, and dwarf Spheroidals is reported. We show that acoherent observational framework emerges from reliable data of different largesamples of objects and it is obtained by different methods of investigation. Wethen highlight the impressive evidence that the distribution of dark andluminous matter are closely correlated and that have universal features. Hintson the cosmological role of this phenomenological scenario are then given.Finally, we discuss the constraints on the elusive nature of the dark particlethat the actual distribution of DM around galaxies pose on its direct andindirect searches.

DMAW 2010 LEGACY the Presentation Review: Dark Matter in Galaxies with its Explanatory Notes