Using powerful K-band radar signals to map rocky exoplanets is not feasible due to significant challenges in signal strength, resolution, and the lengthy time required for echoes to return. The immense power output needed would be astronomical, and the closest exoplanets are far enough away that radar signals would take decades to return. Additionally, the size of the necessary radar dish would be enormous, although interferometry could potentially reduce this size at a high cost. The radar cross-section of rocky planets, influenced by their reflectivity and orientation, further complicates detection, making it unlikely to receive any meaningful return signal. Overall, the technical and financial barriers render the idea of radar mapping distant rocky planets impractical.