Background

The existence of ice in the polar cold traps of the Moon has long been an intriguing possibility. The Clementine spacecraft conducted a radar bistatic experiment in 1994, which supported the idea of an ice deposit within Shackleton crater, near the south pole. However this result generated controversy and there is still disagreement whether observed polarization anomalies are due to ice, particularly from the Earth based radar community. However there is no argument related to the discovery by Lunar Prospector of enhanced hydrogen levels in the polar regions. The question is whether this hydrogen is in the form of water ice. Ice deposits would represent a significant potential resource for the manned human base that is to be set up at one of the Moon’s poles late in the next decade.

Solution

The Mini-RF, designed and built in collaboration with USRA’s Lunar and Planetary Institute, the U.S. Navy, and the Applied Physics Laboratory at Johns Hopkins University, is a miniature orbiting Single Aperture Radar imaging instrument capable of measuring signals at two different wavelengths. By mapping the dark areas near the poles and determining the backscattering properties of these surface materials, the Mini-RF will place firm constraints on the nature and occurrence of water ice deposits on the Moon.

Results

Mini-RF instruments are flying on India’s Chandrayaan-1 and NASA’s Lunar Reconnaissance Orbiter missions, both due for launch to the Moon in 2008.