aJohns Hopkins University Applied Physics Laboratory, Laurel, MD 20723, USA;bComputer Sciences Corporation, Lanham, MD 20706, USA;cDepartment of Terrestrial Magnetism, Carnegie Institution of Washington, Washington, DC 20015, USA
Abstract:
To illustrate the spatial resolution of measurements of Mercury's surface elemental composition by the Gamma-Ray Spectrometer on the MESSENGER spacecraft after one year of orbital observations, we have simulated a global coverage map of the 846-keV iron gamma-ray count rate. The simulated map suggests that distinct geologic units larger than 800 km in horizontal dimension will be discernable when the difference in Fe abundance between adjacent geologic units exceeds 4 wt%. These results imply that the MESSENGER Gamma-Ray Spectrometer dataset will provide useful information for regional geological studies of the surface of Mercury.