H
halman
Guest
Yevaud,<br /><br />I am not sure, but I believe that Earth-based radar was used in determining the rotational period of Mercury, sometime back in the 1960,s or 70's. This was possible because the exact location of the object was known, which meant that a tightly focused pulse could be transmitted to specific co-ordinates, and receiver sensitivity could be cranked way up without worrying about trying to determine if echoes were artifacts or actual echoes, because only echoes arriving in a window microseconds wide could be returns from Mercury. Everything else could be discarded.<br /><br />To scan a wide area, an extremely powerful pulse must be transmitted uniformly over a sector, and the sector carefully scanned for echoes. Then, the process must be repeated to insure that actual echoes are being registered, and not artifacts caused by circut noise, solar interference, etcetera. If we know where exactly to look, we can discern incredibly faint signals, as the Deep Space Tracking Network does routinely. But to search for an object, we have to examine every echo, and the more we increase receiver sensitivity, the more the noise floor will obscure extremely faint echoes. <div class="Discussion_UserSignature"> The secret to peace of mind is a short attention span. </div>