| The Lunascan Project presents KEPLER Directory - Section 30 Updated 20 Oct 2011 BRIEF DESCRIPTION The dark background of Mare Insularum contrasts with bright ray systems from two main centers: the crater Copernicus (in the east) and, especially, the crater Kepler which dominates this area. Perhaps the best-known group of lunar domes is that situated north of the crater Hortensius. Other domes that can be seen through even a quite small telescope lie to the west of the crater Milichius and to the south of the crater T. Mayer.Refer to your Anton Rukl atlas of the Moon, page 87. EARTH BASED TELESCOPIC IMAGES: Since many EBTI's are not kept long on the internet is best to use Google for these images. Image - Kepler and Procellarum (Naoyuk Kurita) LUNAR ORBITER IMAGES: Lunar
Orbiter Database
APOLLO IMAGES: Davy Chain ESA's SMART 1 LUNAR RECONNAISANCE ORBITER IMAGES http://lro.gsfc.nasa.gov/ http://wms.lroc.asu.edu/lroc_browse/ Kepler's Central Peak (LRO) RESEARCH NOTES Kepler Image by Apollo 12 crew, AS12-52-7745 (LPOD) Rayless Crater - (LPOD Lunar Photo of the day) The Moon: Lunar Orbiter 3 (NASA)Kepler (Lunascan) AS14-78-10378(H) - Oceanus Procellarum near Kunowsky (AOTM, SP-362) Around Procellarum (Naoyuki Kurita) ANOMALIES
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