August 31, 2017
Rooks, but not Rooked
Originally published February 14, 2008
image from Kaguya Image Gallery
Except for handheld Hasselblad photos, most images from lunar orbit look straight down on the lunar surface. But the high definition TV camera on Kaguya gives the oblique view that some younger visitors to LPOD may hope to see themselves someday. In this recently released still from a HDTV video we are over the northern third of the Orientale impact basin. Maunder is seen to be a very fresh crater with steeply-dipping terraces, relatively small central peaks and possible impact melt splayed on the surface to the right and left (dark coating). The narrow ribbon of mare lava - Lacus Veris - near the middle of the image is just along the inner edge of the Outer Rook Mountains, and the peaks this side of the lacus help define the Inner Rook Mountains. The puffy, rounded looking, fractured material is the US Geologic Survey-named Maunder Formation. It is interpreted to be Orientale Basin impact melt, a larger scale version of the material on the floor of Tycho. The Cordillera Mountains are on the limb and the area between there and the Outer Rook is thought to be ejecta from the impact that formed the Orientale Basin. If this so-called Rook Formation is ejecta then the Outer Rook is the rim of Orientale, not the Cordillera Mountains. This interpretation is generally accepted but seems counter-intuitive because of the massive scarp of the Cordillera. Two massive peaks of the Outer Rook occur at the 1 o'clock and 11 o'clock positions from the Maunder crater. These wonderful massifs deserve names. Finally, notice the dark halo impact craters that penetrate light dusting and bring up dark debris on to the surface of Lacus Veris.
Clementine Atlas plate 90
Yesterday's LPOD: Monumental Lunar Reference
Tomorrow's LPOD: Another Corner