Lyman Alpha Mapping Project

LAMP Reveals Lunar Surface Features

New maps produced by the Lyman Alpha Mapping Project aboard NASA’s Lunar Reconnaissance Orbiter reveal features at the Moon’s northern and southern poles in regions that lie in perpetual darkness. LAMP, developed by Southwest Research Institute, uses a novel method to peer into these so-called permanently shadowed regions (PSRs), making visible the invisible. The LAMP maps show that many PSRs are darker at far-ultraviolet wavelengths and redder than nearby surface areas that receive sunlight. The darker regions are consistent with large surface porosities, indicating “fluffy” soils, while the reddening is consistent with the presence of water frost on the surface.
The LAMP team estimates that the loss of water frost is about 16 times slower than previously believed. In addition, the accumulation of water frost is also likely to be highly dependent on local conditions, such as temperature, thermal cycling and even geologically recent “impact gardening” in which micrometeoroid impacts redistribute the location and depth of volatile compounds. According to Dr. Kurt Retherford, a senior research scientist also in SwRI’s Space Science and Engineering Divisio an even more unexpected finding is that LAMP’s technique for measuring the lunar Lyman-alpha albedo indicates higher surface porosities within PSRs, and supports the long-postulated presence of tenuous ‘fairy-castle’ like arrangements of surface grains in the PSR soils. Comparisons with future LAMP maps created using data gathered from the Moon’s day side will prove helpful for revealing more about the presence of water frost, as well as the surface porosities of the darker surface features observed. The LAMP team is also eager to apply the Lyman-alpha technique elsewhere on the Moon and on other solar system objects such as Mercury. LRO’s findings are expected to be valuable to the future consideration of a permanent Moon base.