
Light-toned layered deposits thought to be sandstones in West Candor Chasma, Mars. They may have formed in an ancient wet and potentially habitable environment.
CRISM's main purpose is to created detailed maps of the surface mineralogy of Mars. It can detect iron, oxides, phyllosilicates (clays,) and carbonates. All of these materials are indications that Mars was wet in the past, or is still wet now
Usually, CRISM images are paired with High Resolution Imaging Science Experiment (HiRISE) images of the same area. HiRISE is one of three cameras on the MRO, and the most powerful. In fact, HiRISE is a reflecting telescope, the largest ever carried on a deep space mission. It can image the surface of Mars in great detail, and NASA makes HiRISE images available on the website.















Comment: As noted above, the conservationists - opening up the land with controlled burning - have actually been doing the exact opposite to what the native peoples were doing. And this wouldn't be the first time ill-informed and biased conservation efforts, despite their best intentions, have run counter to what nature intends. It also reflects that, in the long term, man's impact is relatively insignificant: