Astronomers determine an asteroid's distance from the sun by assessing its intrinsic brightness, which requires multiple observations to refine its orbit and position. Initial observations record key parameters such as time, elevation, azimuth, range, and range rate, with the latter two often measured by bouncing signals off the asteroid. If direct measurements aren't possible, estimates based on brightness and other factors are used. The accuracy of these measurements improves over time as more data is collected, allowing for a clearer trajectory to be plotted. This process explains why early warnings about potential asteroid impacts can later be retracted as trajectories are refined.