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ReportsLack of Exposed Ice Inside Lunar South Pole Shackleton Crater
The inside of Shackleton Crater at the lunar south pole is permanently shadowed; it has been inferred to hold water-ice deposits. The Terrain Camera (TC), a 10-meter-resolution stereo camera onboard the Selenological and Engineering Explorer (SELENE) spacecraft, succeeded in imaging the inside of the crater, which was faintly lit by sunlight scattered from the upper inner wall near the rim. The estimated temperature of the crater floor, based on the crater shape model derived from the TC data, is less than
1 Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency, Sagamihara, Kanagawa 229-85105, Japan. 90 kelvin, cold enough to hold water-ice. However, at the TC's spatial resolution, the derived albedo indicates that exposed relatively pure water-ice deposits are not on the crater floor. Water-ice may be disseminated and mixed with soil over a small percentage of the area or may not exist at all.
2 Center for Global Environmental Research, National Institute for Environmental Studies, Tsukuba, Ibaraki 305-8506, Japan. 3 Department of Geological Sciences, Brown University, Providence, RI 02912, USA. 4 NTT DATA CCS Corporation, Koto-ku, Tokyo 136-0071, Japan. 5 Department of Earth and Space Science, Graduate School of Science, Osaka University, Toyonaka, Osaka 560-0043, Japan. 6 University Museum, The University of Tokyo, Bunkyo-ku, Tokyo 113-0033, Japan. 7 Department of Aerospace and Astronautics, The University of Tokyo, Bunkyo-ku, Tokyo 113-8656, Japan. 8 Forum Research, Chiba Institute of Technology, Narashino, Chiba 275-0016, Japan. 9 Taito-ku, Tokyo 111-0035, Japan. 10 Division of Earth and Planetary Sciences, Kyoto University, Sakyo-ku, Kyoto 606-8502, Japan. 11 Space Exploration Institute, CP 774, CH-2002 Neuchatel, Switzerland.
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Science. ISSN 0036-8075 (print), 1095-9203 (online)