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In this short note we discuss recent observation of linear correlation onlog-log scale between distribution of dark and visible mass in gravitationallybound systems. The coefficient of such correlation appears to be essentiallythe same for various systems of dramatically different scales such as spiralgalaxies of different luminosities and galaxy clusters. We briefly touchpossible interpretations of this observation and implications for the mass ofdark matter particle.Comment: presented at the DPF2004 meeting in Riverside, CA; to be published in  a supplement in International Journal of Modern Physics

Exploring Properties of Dark and Visible Mass Distribution on Different Scales in the Universe