Classification of the galaxy Milky Way using variable precision rough sets technique

Astronomy image is regarded main source of information to discover outer space, therefore to know the basic contain for galaxy (Milky way), it was classified using Variable Precision Rough Sets technique to determine the CORDLESS CLIPPER different region within galaxy according different color in the image.From classified image we can determined the percentage for each class and then what is the Wafers percentage mean.In this technique a good classified image result and faster time required to done the classification process.