This document discusses specifying the position and orientation of rigid bodies using parameters. It explains that six degrees of freedom are required to fully specify the three-dimensional position and three-dimensional orientation of a rigid body. Rotation matrices are introduced as a way to represent the orientation of one coordinate system relative to another. Examples are provided to demonstrate how to determine the global coordinates of a point given its local coordinates, and how to calculate the position and orientation of one rigid body relative to another when the relationships between each body and an intermediate body are known.