After it was photographed by Mariner 9, it underwent a name change, likely because it is located 21 (*) kilometers above the surface of its planet, making it sufficiently high to avoid the frequent dust storms found there.
The Karzok and Pangboche craters are located on this body. The aureole surrounding it suggests development and resurfacing associated with glacial activity. Formed during the Amazonian epoch, it is located in the western end of Valles Marineris, in the Tharsis region. After it was photographed by Mariner 9, it underwent a name change, likely because it is located 21 (*) kilometers above the surface of its planet, making it sufficiently high to avoid the frequent dust storms found there. A lack of tectonic plates has been hypothesized as one of the reasons why this shield volcano, the size of Arizona, is three times larger than Mount Everest. With a six kilometer high scarp, FTP, name this body, located on Mars, the largest mountain in the solar system.
The Karzok and Pangboche craters are located on this body. The aureole surrounding it suggests development and resurfacing associated with glacial activity.
{Olympus Mons} (prompt on "{Mount Olympus"}. Accept "{Mars}" before "aureole", do not accept or prompt after)