File:Rainbows on the Moon (LROC241 - M109168446CE rainbow crop).png

English: With the Sun exactly overhead, the illumination conditions and viewing angles of the LROC WAC create a rainbow effect in this image. 689 nm filter in red, 643 nm filter in green, and 604 nm filter in blue, from image M109168446C. Scene from north to south covers ~120 km [NASA/GSFC/Arizona State University].

In past featured images, we've seen great examples of the huge effect lighting can have on how the lunar surface looks in NAC images. With the color images from LROC's Wide Angle Camera (WAC), the effects can be just as extreme, and the design of the camera can lead to some unusual and scientifically rich observations. This is the case in the image above, where the 689 nm, 643 nm, and 604 nm filters are displayed in red, green, and blue, respectively. This image was acquired as the Sun was exactly overhead, allowing us to observe the "opposition surge". This is a surge in brightness that occurs when the Sun is directly behind the observer because of two effects. First, there are no shadows seen on the surface, because each boulder and grain of soil's shadow is hidden directly beneath it. Second, as the light reflects back to the observer it constructively interferes with itself.

But why does the image above have a rainbow-like effect? You wouldn't actually see a rainbow with your naked eyes if you were orbiting overhead in a spacecraft. Because each WAC filter observes different pieces of the ground at different times, it observes the opposition surge at a slightly different time. When the observations from separate filters are combined to a single color image, this shifting bright spot is seen as a rainbow. When we make mosaics to look at color variations on the lunar surface, we use images where the Sun is a bit lower in the sky (around 30° from the vertical) where this extreme effect is no longer seen. But that doesn't mean these images aren't useful - they provide a huge new dataset for studying how light interacts with a particulate surface at different wavelengths. Perhaps an esoteric-sounding field of study, but this data can help us understand the reflectance images and spectra we have of the Moon and other bodies throughout the Solar System.