To launch a satellite into a circular orbit from the top of Mt. Everest, the horizontal velocity must be calculated using the relationship between centripetal force and gravitational force. The centripetal force can be expressed as F = mv²/R or F = 4π²mR/T², with the first formula being suitable for finding velocity. The gravitational force formula accounts for the mass of the Earth and the satellite, ensuring that the centripetal force equals the gravitational force for stable orbit. If the satellite's speed exceeds a certain threshold, the centripetal force will surpass gravitational pull, preventing it from maintaining orbit. Understanding these forces and their equations is crucial for determining the required launch velocity.