Calculating the mass of the Milky Way using only the speed of a planet in a circular orbit is not feasible without additional information, specifically the orbital radius. The relationship between centripetal force and gravitational force is established, but the radius is essential to solve for mass. Assumptions about typical trends in orbital speed and radius of stars can provide context, but they do not directly solve the problem. Without the radius or other relevant data, determining the Milky Way's mass from speed alone is impossible. Therefore, additional information or assumptions are necessary to approach this calculation effectively.