Spectrographic data taken from an Ocean Optics spectrometer has helped Nasa confirm the presence of water ice on the moon.
The spectrometer, custom re-engineered for space duty by Aurora Design and Technology and dubbed 'Alice', was part of the scientific payload on Nasa's Lunar Crater Observation and Sensing Satellite (Lcross) mission.
The Lcross shepherding spacecraft (S-S/C) carrying Alice made spectroscopic measurement of the permanently shadowed crater Cabeus, near the lunar south pole, as the spacecraft's Centaur upper rocket stage impacted the floor of Cabeus.
The instruments on board the S-S/C monitored the emission caused by the Centaur impact, as well as the resulting two-part debris plume created by the impact.
Nasa scientists announced on 13 November that the signature of water was seen in both near-infrared and ultraviolet spectroscopic measurements taken during the mission.
Ocean Optics' Alice provided the ultraviolet measurements, confirming the findings of the near-infrared spectroscopic measurements.
From the data gathered, Nasa scientists were able to estimate that roughly 220lb of water was found by the instruments in the material excavated from the 20-30m wide crater formed by the Centaur impact.
It is hoped that water on the moon could set the stage for further space exploration by providing drinking water or even rocket fuel derived from its hydrogen and oxygen molecules.
Ocean Optics' highly sensitive QE65000 spectrometer was adapted to withstand the rigours of space - extreme temperature ranges, radiation, shock and vibration.
With a wavelength range of 270-650nm and an optical resolution of less than 1nm, Alice was designed to identify, with a high degree of accuracy, ionised water (visible at 619nm), OH radicals (visible at 308nm) and other organic molecules containing carbon.
Though the measurements were made from the ejecta reflecting sunlight scattered off of the crater walls, the unit's back-thinned detector was able to make the most of the available light.
Alice was developed in partnership with Aurora Design and Technology, which played a significant role in the mission, developing the optics that collected light from the impact and resulting ejecta plume for the mission.
Ocean Optics and Aurora Design and Technology have collaborated on other Nasa space projects, including the Chemcam Mars mission.
A unit designed around Ocean Optics' HR-Series spectrometers will be part of the mission to study rock and soil composition on the red planet, scheduled to launch in autumn 2011.
Aurora Design and Technology is also developing spectroscopic systems for Nasa's Ladee mission (based on Ocean Optics' QE65000) and O/Oreos mission (based on the USB2000+).
