We present an overview of the upcoming Microwave Anisotropy Probe (MAP)
mission, with an emphasis on those aspects of the mission that simplify the
data analysis. The method used to make sky maps from the differential
temperature data is reviewed and we present some of the noise properties
expected from these maps. An overview of the method we plan to use to mine the
angular power spectrum from the mega-pixel sky maps closes the paper.Comment: For the MAP Science Team. 11 pages, 5 figures, to appear in Mining
the Sky, ESO Astrophysics Symposia Serie