This is Mons Mouton. It lies between the Nobile and Malapert craters in the lunar South Pole region. In the first image, north is at the top. The elevation is color-coded from lowest to highest as follows: blue, green, yellow, red, brown, and white. The south and southeast portions of Mons Mouton are the highest parts of the feature. Near these high points, it has a clear line of sight to Earth and receives full sunlight for a large percentage of the year. It offers gentle 3°–5° sloped pathways around the steeper, intermittent hills that have 10°–15° slopes—ideal terrain for exploration by rover. There are thousands of unnamed craters on the plateau itself that contain small Permanently Shadowed Regions (PSRs) which could hold water ice. These small craters should be explored before venturing into the larger, more dangerous PSRs at the lower elevations below the plateau. When deciding where to build on the plateau, one location stands out. It would lie on a line between the two largest PSRs on Mons Mouton. In fact, this route would be an excellent location for the first lunar road, and possibly the first lunar railway. The distance between the two PSRs is approximately 26 km. The largest PSR is located at -82.26, 42.29, and the second largest is at -84.46, 33.99. The second largest PSR is the most interesting to me because it features a small triangular area on its eastern rim that appears to be an ideal landing site. I have identified a triangle with nearly equal sides (about 1.25 km each) with a small PSR at each vertex. American astronauts landing anywhere inside this triangle would have a PSR just a short rover ride away; in fact, they could easily walk to one from the landing site. If the first site turns out to be a "dry hole," there are two other small craters and one very large one in close proximity to the landing site with PSRs.
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