New Scientist
Image: jurvetson
Geologists have used the Hubble Space Telescope to study minerals on the moon. It might be one small step for them, but it’s a giant leap towards building a lunar outpost.
Space scientists are keen to map the concentration of the titanium-dioxide-rich mineral ilmenite on the moon’s surface, says Jim Garvin of NASA’s Goddard Space Flight Center in Greenbelt, Maryland. “Oxygen production from TiO2-enhanced lunar soils could potentially make breathable oxygen and even oxidiser for rocket fuel.”
UV images of the lunar surface show patterns that correlate with the concentration of TiO2 measured in lunar samples collected by the Apollo missions, and so a map of the UV variations can be used to create a map of TiO2 abundance. However, Earth’s atmosphere interferes with UV readings, so the team used Hubble to take UV images of a small area of the lunar surface that included the landing sites of the Apollo 15 and 17 spacecraft.
When the team compared the UV data with the TiO2 levels from the Apollo sampled, they found that low-lying basaltic soil has 6 to 8 per cent TiO2 by weight, while the highland soils contain only 2 per cent (Geophysical Research Letters, vol 34, p L13203). “Our well-calibrated UV images will act as a pathfinder for mapping by NASA’s 2008 Lunar Reconnaissance Orbiter,” says Garvin.