宇宙航空研究開発機構 宇宙科学研究本部
みさと天文台
東京都庁
東京大学 理学部附属天文学教育研究センター
University of Hawaii Institute for Astronomy
宇宙航空研究開発機構 宇宙科学研究本部
著者所属（英）
Japan Aerospace Exploration Agency Institute of Space and Astronautical Science
Misato Observatory
Tokyo Metropolitan Government
University of Tokyo Institute of Astronomy, School of Science
University of Hawaii Institute for Astronomy
Japan Aerospace Exploration Agency Institute of Space and Astronautical Science
出版者
宇宙航空研究開発機構宇宙科学研究本部
出版者（英）
Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (JAXA/ISAS)
雑誌名
第38回月・惑星シンポジウム
雑誌名(英)
Proceedings of the 38th ISAS Lunar and Planetary Symposium
ページ
151 - 154
発行年
2006-03
抄録（英）
Lightcurves of three V-type asteroids 4383 Suruga, 4796 Lewis and 6331 1992 FZ1 were obtained by five telescope: the 0.30-m telescope at the Kiso Observatory (K.3T), the 0.36-m telescope at the Miyasaka Observatory, the 3-color MITSUME 0.5-m telescope at the Okayama Astrophysical Observatory, the 1.05-m telescope at the Misato Observatory, and the 2.24-m telescope at Mauna Kea (UH88). 4383 Suruga has a period of 3.811 hour and an amplitude of 0.10 mag, 4796 Lewis has a period of 3.508 hour and an amplitude of 0.4 mag, and 6331 1992 FZ1 has a period of 9.333 hour and an amplitude of 0.7 mag.
Lightcurve observations of three V-type asteroids 4383 Suruga, 4796 Lewis, and 6331 1992 FZ1
