To achieve a stable orbit, a satellite must reach a specific speed that balances gravitational force and centripetal acceleration. The gravitational force can be described using the equation F = G(m1m2/r²), while the centripetal acceleration is expressed as v²/r. The discussion highlights the importance of understanding that the net radial acceleration must equal zero for a circular orbit, meaning gravitational force must equal the centripetal force required to maintain the orbit. Participants express confusion about how to calculate the necessary orbital speed without knowing the mass of the satellite, emphasizing the need for a clear understanding of the forces at play. Ultimately, the conversation centers on the relationship between gravitational and centripetal forces in determining orbital speed.