
The left figure is a color composite of processed data that accentuates compositional differences in the moon's Orientale region. The image on the right contains significant thermal emission in the signal and is particularly sensitive to small variations in local morphology.
The Moon Mineralogy Mapper is the first instrument to provide highly uniform imaging of the lunar surface. Along with the length and width dimensions across a typical image, the instrument analyzes a third dimension - color.
A two-image figure, and other data from NASA's Moon Mineralogy Mapper Instrument, can be found HERE.
The composite image consists of a subset of Moon Mineralogy Mapper data for the Orientale region. The image strip on the left is a color composite of data from 28 separate wavelengths of light reflected from the moon. The blue to red tones reveal changes in rock and mineral composition, and the green color is an indication of the abundance of iron-bearing minerals such as pyroxene. The image strip on the right is from a single wavelength of light that contains thermal emission, providing a new level of detail on the form and structure of the region's surface.







