Deceased: 30 May 2011.
Far-ultraviolet reflectance properties of the Moon's permanently shadowed regions
Article first published online: 7 JAN 2012
© 2012 by the American Geophysical Union
Journal of Geophysical Research: Planets (1991–2012)
Volume 117, Issue E12, December 2012
How to Cite
2012), Far-ultraviolet reflectance properties of the Moon's permanently shadowed regions, J. Geophys. Res., 117, E00H04, doi:10.1029/2011JE003913., et al. (
- Issue published online: 7 JAN 2012
- Article first published online: 7 JAN 2012
- Manuscript Accepted: 30 OCT 2011
- Manuscript Revised: 17 OCT 2011
- Manuscript Received: 29 JUL 2011
- NASA. Grant Number: 00000
 Although of great interest for science and resource utilization, the Moon's permanently shadowed regions (PSRs) near each pole present difficult targets for remote sensing. The Lyman Alpha Mapping Project (LAMP) instrument on the Lunar Reconnaissance Orbiter (LRO) mission is able to map PSRs at far-ultraviolet (FUV) wavelengths using two faint sources of illumination from the night sky: the all-sky Ly α glow produced as interplanetary medium (IPM) H atoms scatter the Sun's Ly α emissions, and the much fainter source from UV-bright stars. The reflected light from these two sources produces only a few hundred events per second in the photon-counting LAMP instrument, so building maps with useful signal-to-noise (SNR) ratios requires the careful accumulation of the observations from thousands of individual LRO orbits. In this paper we present the first FUV albedo maps obtained by LAMP of the Moon's southern and northern polar regions. The results show that (1) most PSR regions are darker at all FUV wavelengths, consistent with their surface soils having much larger porosities than non-PSR regions (e.g., ∼70% compared to ∼40% or so), and (2) most PSRs are somewhat “redder” (i.e., more reflective at the longer FUV wavelengths) than non-PSR regions, consistent with the presence of ∼1–2% water frost at the surface.