JpGU-AGU Joint Meeting 2017

講演情報

[EE] ポスター発表

セッション記号 P (宇宙惑星科学) » P-CG 宇宙惑星科学複合領域・一般

[P-CG23] [EE] 宇宙・惑星探査の将来計画と関連する機器開発の展望

2017年5月24日(水) 10:45 〜 12:15 ポスター会場 (国際展示場 7ホール)

コンビーナ:笠原 慧(東京大学)、亀田 真吾(立教大学理学部)、尾崎 光紀(金沢大学理工研究域電子情報学系)、笠原 禎也(金沢大学総合メディア基盤センター)

[PCG23-P01] 超小型深宇宙探査機「エクレウス」搭載,月面衝突閃光観測カメラ「デルフィヌス」の開発

*阿部 新助1柳澤 正久2矢野 創4船瀬 龍3 (1.日本大学、2.電気通信大学、3.東京大学、4.JAXA)

キーワード:超小型衛星、月面衝突閃光、メテオロイド、流星、小惑星

EQUULEUS (EQUilibriUm Lunar-Earth point 6U Spacecraft) will be the world’s smallest spacecraft to explore the Earth-Moon Lagrange2 point (EML2). The spacecraft will be jointly developed by the University of Tokyo and JAXA which will be launched by NASA’s SLS (Space Launch System) EM-1 (Exploration Mission-1) in 2018. The spacecraft will fly to a libration orbit around the EML2 point and demonstrate trajectory control techniques within the Sun-Earth-Moon region.
DELPHINUS (DEtection camera for Lunar impact PHenomena IN 6U Spacecraft) is one of the onboard scientific instruments onboard EQUULEUS to observe meteoroids by using imaging of lunar impact flashes and near-Earth asteroids. Meteoroid are a small rocky bodies traveling through interplanetary space. When a meteoroid impacts the moon at several 10s of km/s, a brilliant flash at the point of impact can be observed as a lunar impact flash. The influx rate of interplanetary dusts onto the Earth-Moon surface are essential for understanding solar system evolution and are useful information for the future human space activities in the Cis-Lunar space that is the volume within the Moon's orbit. Thus, it is very important to investigate size distributions, influx rate and daily variation of meteoroids. Ground-based meteor observations by using all-sky cameras are limited to the roughly 10,000 km2 of upper-atmosphere visible from their location. On the other, Lunar impact monitoring enables to monitor the more than 106 km2 collecting area. Lunar impact monitoring has a great advantage to detect large meteoroids in the mass range between 10s of grams and few kilograms corresponding to centimeters and tens of centimeters, which is as a bridge between small asteroids, larger than few meters size, and meteors, smaller than millimeter size, observed mainly from the ground.
This paper describes newly developed DELPHINUS camera system.