Satellite Type Estination from Ground-based Photometric Observation

Takao Endo, Mitsubishi Electric Corporation, Hitomi Ono, Mitsubishi Electric Corporation, Jiro Suzuki, Mitsubishi Electric Corporation, Toshiyuki Ando, Mitsubishi Electric Corporation, Takashi Takanezawa, Mitsubishi Electric Corporation

Keywords: Space Situational Awareness, Color index, Photometry, Spectroscopy, Ground-base observation

Abstract:

The optical photometric observation is potentially a powerful tool for understanding of the Geostationary Earth Orbit (GEO) objects. At first, we measured in laboratory the surface reflectance of common satellite materials, for example, Multi-layer Insulation (MLI), mono-crystalline silicon cells, and Carbon Fiber Reinforced Plastic (CFRP). Next, we calculated visual magnitude of a satellite by simplified shape and albedo. In this calculation model, solar panels have dimensions of 2 by 8 meters, and the bus area is 2 meters squared with measured optical properties described above. Under these conditions, it clarified the brightness can change the range between 3 and 4 magnitudes in one night, but color index changes only from 1 to 2 magnitudes. Finally, we observed the color photometric data of several GEO satellites visible from Japan multiple times in August and September 2014. We obtained that light curves of GEO satellites recorded in the B and V bands (using Johnson filters) by a ground-base optical telescope. As a result, color index changed approximately from 0.5 to 1 magnitude in one night, and the order of magnitude was not changed in all cases. In this paper, we briefly discuss about satellite type estimation using the relation between brightness and color index obtained from the photometric observation.

Date of Conference: September 20-23, 2016

Track: Poster

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