Current radar technology can detect celestial objects over distances exceeding 1 billion kilometers, with Saturn and its moon Titan being notable examples. The effectiveness of radar detection depends on both the size of the object and the distance, as well as the ability to illuminate the target area. Radar reflections provide historical data, indicating that signals received are from a time in the past, such as Titan's reflection revealing conditions from 2.25 hours prior. The discussion also explores the theoretical potential of using gravitational phenomena, like black holes, as reflective surfaces for detecting light and signals from distant celestial bodies. While intriguing, the practicality of such methods remains limited due to the faintness of potential reflections and the fixed time delays involved.