Global Ultraviolet through Visible Color Observations of the Moon with the Lunar Reconnaissance Orbiter Wide Angle Camera

during the β = 0° orbit (M109168446CE, 0° lat, 10.5° E lon). The 689, 604, and 415 nm bands are in red, green, and blue. The high reflectance streak is the opposition surge, which is at a slightly different position in each filter beacuse each filter has a different emission angle. Right: The phase, emission, and incidence angles of the 643 nm band in red, green, and blue. Phase and emission angles vary from 35° at the edges to 0° at the center, incidence angles range 0-3°. GLOBAL ULTRAVIOLET THROUGH VISIBLE COLOR OBSERVATIONS OF THE MOON WITH THE LUNAR RECONNAISSANCE ORBITER WIDE ANGLE CAMERA. B. W. Denevi, M. S. Robinson, B. W. Hapke, S. J. Lawrence, S. M. Wiseman, B. L. Jolliff, and the LROC Team. School of Earth and Space Exploration, Arizona State University, Tempe, AZ 85251, USA. Department of Geology and Planetary Science, University of Pittsburgh, Pittsburgh, PA 15260, USA. Department of Earth and Planetary Sciences, Washington University, St. Louis, MO 63130, USA.