The discussion centers on the measurement of orbital velocities of various astronomical objects within the Milky Way, particularly focusing on the solar system's planets. Participants highlight the complexity of accurately determining these velocities due to the dynamic nature of celestial mechanics and the influence of numerous factors, including gravitational interactions and the presence of uncharted mass. They mention various software and models, such as SLALIB and the Gaia mission, which provide high-precision data for celestial positions and velocities. The conversation also touches on the challenges of mapping the Milky Way due to dust and other obstructions, as well as the ongoing efforts by NASA and ESA to improve data accuracy. Overall, the accuracy of current orbital speed predictions is noted to be within a range of +/- 1%, reflecting the inherent difficulties in celestial navigation and modeling.