  The MAGIC 17m-diameter Imaging Air Cherenkov Telescope (IACT) has been
commissioned beginning of 2005. The telescope has been designed to achieve the
lower detection energy threshold ever obtained with an IACT, about 50 GeV. A
new window in gamma-ray astronomy is being opened with great impact for
exciting new physics and new discoveries. Among the targets of MAGIC is the
indirect detection of Dark Matter (DM). We have considered different DM halo
models of high DM density objects like the center of the Milky Way, its closest
satellites and nearby galaxies (M31,M87). For each object, detection limits are
computed for different DM halo models in a mSUGRA scenario for supersymmetric
neutralino annihilation $\gamma$-ray production. Advantages and drawbacks of
these objects and plans for future observations are discussed.
