Analysis of lunar samples returned by the US Apollo missions revealed that the lunar highlands consist of anorthosite, plagioclase, pyroxene, and olivine; also, the lunar maria are composed of materials such as basalt and ilmenite. More recently, the remote sensing approach has enabled reduction of the time required to investigate the entire lunar surface, compared to the approach of returning samples. Moreover, remote sensing has also made it possible to determine the existence of specific minerals and to examine wide areas. In this paper, an investigation was performed on the reflectance distribution and its trend. The results were applied to the example of the double ray stretched in parallel lines from the Tycho crater to the third-quadrant of Mare Nubium. Basic research and background information for the investigation of lunar surface characteristics is also presented. For this research, resources aboard the SELenological and ENgineering Explorer (SELENE), a Japanese lunar probe, were used. These included the Multiband Imager (MI) in the Lunar Imager / Spectrometer (LISM). The data of these instruments were edited through the toolkit, an image editing and analysis tool, Exelis Visual Information Solution (ENVI).

1. INTRODUCTION
 2. METHODS
 3. RESULTS
 4. CONCLUSIONS
 ACKNOWLEDGEMENTS
 REFERENCES

• Eung Seok Yi(Chungnam National University,Korea Institute of Geoscience and Mineral Resources)
• Kyeong Ja Kim(Korea Institute of Geoscience and Mineral Resources) Corresponding Author
• Yi Re Choi(Korea Institute of Geoscience and Mineral Resources,University of Science and Technology)
• Yong Ha Kim(Chungnam National University)
• Sung Soon Lee(Korea Institute of Geoscience and Mineral Resources)
• Seung Ryeol Lee(Korea Institute of Geoscience and Mineral Resources)