Lunar craters with radar bright ejecta

Mathematics – Logic

Scientific paper

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Ejecta, Lunar Craters, Radar Imagery, Selenology, Infrared Photography, Lunar Surface, Radar Maps, Radar Signatures, Surface Properties, Apollo Missions, Imagery, Surface, Density, Catalogs, Comparisons, Data, Moon, Craters, Radar Observations, Brightness, Ejecta, Deposits, Origin, Impact Craters, Physical Properties, Wavelengths, Albedo, Remote Sensing, Distribution, Infrared, Photographs, Halos, Diameter, Optical Properties, Ages, Size, Maria

Scientific paper

The properties of the 3.8-cm radar-bright halos observed around certain lunar impact craters are compiled and compared with 70-cm radar, thermal infrared and photogeological data in order to address the nature of the halos. Diameters, positions, and radar and IR signal strengths are presented for 120 radar-bright ejecta regions of size greater than 20 km and twice the diameter of the crater. The 3.8-cm halos are noted to range in size up to 30 times that of the crater itself, although the strength of the signal from the crater and rim lies in a narrow range, while the IR halos are smaller in extent and variable in signal strength. The radar-bright ejecta are found to have a range of optical properties, and to be associated with fresh primary impact craters. Data are thus consistent with craters having radar-bright ejecta deposits having ages of less than 10 million to 1 billion years, with the radar and infrared signatures of the ejecta deposits produced by combinations of enhanced blockiness and roughness.

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