Special Issue: Lunar Science with the SELENE “Kaguya” Mission-Prelaunch Studies-
- Open Access
Global lunar-surface mapping experiment using the Lunar Imager/Spectrometer on SELENE
Earth, Planets and Space volume 60, pages 243–255 (2008)
The Moon is the nearest celestial body to the Earth. Understanding the Moon is the most important issue confronting geosciences and planetary sciences. Japan will launch the lunar polar orbiter SELENE (Kaguya) (Kato et al., 2007) in 2007 as the first mission of the Japanese long-term lunar exploration program and acquire data for scientific knowledge and possible utilization of the Moon. An optical sensing instrument called the Lunar Imager/Spectrometer (LISM) is loaded on SELENE. The LISM requirements for the SELENE project are intended to provide high-resolution digital imagery and spectroscopic data for the entire lunar surface, acquiring these data for scientific knowledge and possible utilization of the Moon. Actually, LISM was designed to include three specialized sub-instruments: a terrain camera (TC), a multi-band imager (MI), and a spectral profiler (SP). The TC is a high-resolution stereo camera with 10-m spatial resolution from a SELENE nominal altitude of 100 km and a stereo angle of 30° to provide stereo pairs from which digital terrain models (DTMs) with a height resolution of 20 m or better will be produced. The MI is a multi-spectral imager with four and five color bands with 20 m and 60 m spatial resolution in visible and near-infrared ranges, which will provide data to be used to distinguish the geological units in detail. The SP is a line spectral profiler with a 400-m-wide footprint and 300 spectral bands with 6–8 nm spectral resolution in the visible to near-infrared ranges. The SP data will be sufficiently powerful to identify the lunar surface’s mineral composition. Moreover, LISM will provide data with a spatial resolution, signal-to-noise ratio, and covered spectral range superior to that of past Earth-based and spacecraft-based observations. In addition to the hardware instrumentation, we have studied operation plans for global data acquisition within the limited total data volume allotment per day. Results show that the TC and MI can achieve global observations within the restrictions by sharing the TC and MI observation periods, adopting appropriate data compression, and executing necessary SELENE orbital plane change operations to ensure global coverage by MI. Pre-launch operation planning has resulted in possible global TC high-contrast imagery, TC stereoscopic imagery, and MI 9-band imagery in one nominal mission period. The SP will also acquire spectral line profiling data for nearly the entire lunar surface. The east-west interval of the SP strip data will be 3–4 km at the equator by the end of the mission and shorter at higher latitudes. We have proposed execution of SELENE roll cant operations three times during the nominal mission period to execute calibration site observations, and have reached agreement on this matter with the SELENE project. We present LISM global surface mapping experiments for instrumentation and operation plans. The ground processing systems and the data release plan for LISM data are discussed briefly.
Basilevsky, A. T., H. U. Keller, A. Nathues, U. Mall, H. Hiesinger, and M. Rosiek, Scientific Objectives and Selection of Targets for the SMART-1 Infrared Spectrometer (SIR), Planet. Space Sci., 52, 14, 1261–1285, 2004.
Butler, B. J., The Migration of Volatiles on the Surfaces of Mercury and the Moon, J. Geophys. Res., 102(E8), 19283–12291, 1997.
Demura, H., N. Hirata, H. Otake, M. Ohtake, A. Sugihara, M. Higa, T. Matsunaga, and J. Haruyama, Data Processing Flow and Products of LISM: Lunar Imager and SpectroMeter, 32nd Lunar Planet. Sci. Conf., abst. #11648, 2001.
Feldman, W. C., A. B. Binder, B. L. Barraclough, and R. D. Belian, First results from the Lunar Prospector Spectrometers, 29th Lunar Planet. Sci. Conf., abst. #1936, 1998.
Feldman, W. C., D. J. Lawrence, S. Maurice, R. C. Elphic, B. L. Barraclough, A. B. Binder, and P. G. Lucey, Classification of Lunar Terranes using Neutron and Thorium Gamma-ray Data, 30th Lunar Planet. Sci. Conf., abst. #2056, 1999.
Feldman, W. C., S. Maurice, D. J. Lawrence, R. C. Little, S. L. Lawson, O. Gasnault, R. C. Wiens, B. L. Barraclough, R. C. Elphic, T. H. Prettyman, J. T. Steinberg, and A. B. Binder, Evidence forWater Ice Near the Lunar Poles, J. Geophys. Res., 106(E10), 23,231–23,251, 2001.
Giguere, T. A., B. R. Hawke, L. R. Gaddis, D. T. Blewett, J. J. Gillis-Davis, P. G. Lucey, G. A. Smith, P. D. Spudis, and G. J. Taylor, Remote Sensing Studies of the Dionysius Region of the Moon, J. Geophys. Res., 111(E6), doi:10.1029/2005JE002639, 2006.
Hapke, B., Theory of Reflectance and Emittance Spectroscopy, 262, Cambridge Univ. Press, 1993.
Haruyama, J., H. Otake, M. Ohtake, A. Shiraishi, N. Hirata, and T. Matsunaga, LISM (Lunar Imager/SpectroMeter) Mission for SELENE Project, 31st Lunar Planet. Sci. Conf., abst. #1317, 2000.
Haruyama, J., H. Otake, and M. Ohtake, LISM Mission for SELENE Project, Proc. 22nd Int. Sym. Tec. Space Sci., 1686–1691, 2001.
Haruyama, J., M. Ohtake, N. Hirata, R. Nakamura, and T. Matsunaga, Expected Performance of Lunar Imager/SpectroMeter on SELENE, 34th Lunar Planet. Sci. Conf., abst. #1565, 2003a.
Haruyama, J., M. Ohtake, T. Matsunaga, N. Hirata, and LISM Working Group, Flight Model Performance of SELENE Terrain Camera, Proc. 23rd. Int. Sym. Tec. Space Sci., 1992–1996, 2003b.
Haruyama, J., M. Ohtake, T. Matsunaga, and LISM Working Group, The Detectability of Degradation of Lunar Impact Crater by SELENE Terrain Camera, 35th Lunar Planet. Sci. Conf., abst. #1496, 2004.
Haruyama, J., M. Ohtake, N. Hirata, R. Nakamura, and T. Matsunaga, Flight model performance of SELENE Terrain Camera (II), Proc. 25th Int. Sym. Tec. Space Sci., 857–862, 2005.
Haruyama, J., M. Ohtake, T. Matsunaga, T. Morota, A. Yoshizawa, and LISM Working Group, Planned Digital Terrain Model Products from SELENE Terrain Camera Data, 37th Lunar Planet. Sci. Conf., abst. #1132, 2006a.
Haruyama, J., M. Ohtake, T. Matsunaga, and LISM Working Group, Global High-resolution stereo mapping of the Moon with the SELENE Terrain Camera, in Adv. Geosci., 3: Planetary Science, World Scientific Publishing, edited by W.-H. Ip and A. Bhardwaj, pp. 101–108, 2006b.
Haruyama, J., T. Matsunaga, T. Morota, C. Honda, M. Torii, Y. Yokota, H. Kawasaki, M. Ohtake, and LISM Working Group, Pre-Launch Operation Planning of Lunar Imager/Spectrometer (LISM) on SELENE, 38th Lunar Planet. Sci. Conf., abst. #1136, 2007.
Head, J. W., Lunar volcanism in space and time, Rev. Geophys. Space Phys., 14, 265–300, 1976.
Hörz, F., R. A. Grieve, G. D. Heiken, P. D. Spudis, and A. B. Binder, Lunar Surface, Processes, in The Lunar Sourcebook: A User’s Guide to the Moon, edited by G. D. Heiken, D. Vaniman, and B. M. French, Lunar and Planet. Inst. and Cambridge Univ. Press, pp. 61–120, 1991.
Hiesinger, H. and J. M. Head, New Views of Lunar Geosiceces: An Introduction and Overview, in New Views of the Moon, Rev. Min. Gechem., 60, 1–81, 2006.
Hiesinger, H., R. Jaumann, G. Neukum, J. W. Head, and U. Wolf, Ages and Stratigraphy of Mare Basalts on the Lunar Nearside, J. Geophys. Res., 105(E12), 29239–29275, 2000.
Hiesinger, H., J.W. Head, U. Wolf, R. Jaumann, and G. Neukum, Ages and Stratigraphy of Mare B Basalts in Oceanus Procellarum, Mare Nubium, Mare Cognitum, and Mare Insularum, J. Geophys. Res., 108(E7), 5065, doi:10.1029/2002JE001985, 2003.
Iwata, T., N. Namiki, H. Hanada, H. Minamino, T. Takano, N. Kawano, K. Matsumoto, and S. Sasaki, SELENE Small Sub-Satellites for Lunar Gravity Observation, 38th Lunar Planet. Sci. Conf., abst. #1557, 2007.
Jolliff, B. L., J. J. Gillis, L. A. Haskin, R. L. Korotev, and M. A. Wieczorek, Major Lunar Crustal Terrains: Surface Expression and Crust-mantle Origins, J. Geophys. Res., 105(E2), 4197–4216, 2001.
Kato, M., Y. Takizawa, and S. Sasaki, Selene Project Team, The SELENE Mission: Present Status and Science Goals, 38th Lunar Planet. Sci. Conf., abst. #1211, 2007.
Lawrence, D. J., W. C. Feldman, R. C. Elphic, J. J. Hagerty, S. Maurice, G. W. McKinney, and T. H. Prettyman, Improved Modeling of Lunar Prospector Neutron Spectrometer Data: Implications for Hydrogen Deposits at the Lunar Poles, J. Geophys. Res., 111, E08001, doi:10.1029/2005JE002637, 2006.
Matsunaga, T., M. Ohtake, Y. Makiko, and J. Haruyama, Development of a Visible and Near-infrared Spectrometer for Selenological and Engineering Explorer (SELENE), in Hyperspectral Remote Sensing of the Land and Atmosphere, edited by W. L. Smith and Y. Yasuoka, Proc. SPIE, 4151, 32–39, 2001.
Matsunaga, T., M. Ohtake, J. Haruyama, T. Sugihara, and LISM Working Group, Environmental Test Resutls and Their Implications to the Perfommance of SELENE Spectral Profiler, Proc. 23rd Int. Sym. Tec. Space Sci., 1922–1927, 2003.
Melosh, H. J., Impact Cratering: A Geological Process, Oxford University Press, 1989.
Namiki, N., H. Hanada, T. Tsubokawa, N. Kawano, M. Ooe, K. Heki, T. Iwata, M. Ogawa, and T. Takano, Selenodetic Experiments of SELENE: Relay Subsatellite, Differential VLBI, and Laser Altimeter, Adv. Space Res., 23, 11, 1817–1820, 1999.
Neukum, G., B. A. Ivanov, and W. K. Hartmann, Cratering records in the inner solar system in relation to the lunar reference system, Space Sci. Rev., 96, 55–86, 2001.
Nozette, S. and the Clementine team, The Clementine Mission to the Moon: Scientific Overview, Science, 266, 1835–1839, 1994.
Nyquist, L. E. and C.-Y. Shih, The isotopic record of lunar volcanism, Geochim. Cosmochim. Acta, 56, 2213–2234, 1992.
Ohtake, M., J. Haruyama, and T. Matsunaga, Scientific Goals and Performance of Multiband Imager for the SELENE mission, Proc. 23rd Int. Sym. Tec. Space Sci., 1997–2000, 2003.
Ohtake, M., J. Haruyama, T. Matsunaga, T. Morota, Y. Yokota, C. Honda, A. Yamamoto, T. Arai, and H. Takeda, Objectives of the SELENE Multiband Imager and Spectral Study of Dho489, 38th Lunar Planet. Sci. Conf., abst. #1829, 2007.
Pieters, C. M., Compositional diversity and stratigraphy of the lunar crust derived from reflectance spectroscopy, in Remote Geochemical Analysis Elemental and Mineralogical Composition, edited by C. M. Pieters and P. A. J. Englert, Cambridge University Press, Cambridge, pp. 309–339, 1993.
Pieters, C. M., L. Gaddis, B. Jolliff, and M. Duke, Rock Types of South Pole-Aitken Basin and Extent of Basaltic Volcanism, J. Geophys. Res., 106(E11), 28001–28022, 2001.
Sasaki, S., Y. Iijima, K. Tanaka, M. Kato, M. Hashimoto, H. Mizutani, and Y. Takizawa, The SELENE mission: Goals and status, Adv. Space Res., 31(11), 2335–2340, 2003.
Starukhina, L. V., Polar Regions of the Moon as a Potential Repository of Solar-Wind-Implanted Gases, Adv. Space Res., 37(1), 50–58, 2006.
Starukhina, L. V. and Y. G. Shkuratov, The lunar poles: water ice or chemically trapped hydrogen, Icarus, 147, 585–587, 2000.
Tompkins, S. and C. M. Pieters, Mineralogy of the Lunar Crust: Results from Clementine, Meteorit. Planet. Sci., 34(1), 25–41, 1999.
Wilhelms, D. E., The Geologic History of the Moon, U.S. Geol. Surv. Prof. Pap., 1348, 302 pp, 1987.
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Haruyama, J., Matsunaga, T., Ohtake, M. et al. Global lunar-surface mapping experiment using the Lunar Imager/Spectrometer on SELENE. Earth Planet Sp 60, 243–255 (2008). https://doi.org/10.1186/BF03352788