Here's the image in the form of an info panel from this morning's observing session: South Pole misc topo study 2009-9-10 12:19UT http://members.csolutions.net/fisherka/astronote/observed/LCROSS/20090910_12... http://tinyurl.com/lzoggo This morning, the east flank of Leibnitz beta was much brighter. Only the "back" or pole side rim of Shoemaker was illuminated as a silver. At this high negative libration in latitude, Caebus finally makes sense to me as being hidden from view behind M1. The main lesson learned from observing and imaging the south pole the last three mornings is that efficient orienting to features involves clearly identifying the main Earth-side massifs at the south pole. Once you locate the massifs, identifying craters is easy regardless of the current libration. The relevant south polar lunar massifs from lunar east to lunar west are: Leibnitz Beta Malapert alpha a.k.a. M8 M1 M3 and in the far background at higher negative librations - M5. This outstanding 2007-12-19 LPOD image by Tom Bash highlights these massifs. http://www.lpod.org/?m=20071219 This massifs are all fragments of a rim arc left by the South Polar Atkin basin impact. See LPODs 10-21-2006 and 12-19-2007. http://www.lpod.org/?m=20061021 and http://www.lpod.org/?m=20060920 Clear Skies - Kurt