COSPAR 2019

GEO-X : GEOSPACE X-RAY IMAGER

Yuichiro Ezoe 1 Ryu Funase 2 Harunori Nagata 3 Yoshizumi Miyoshi 4 Satoshi Kasahara 5 Hiroshi Nakajima 6 Ikuyuki Mitsuishi 7 Kumi Ishikawa 8 Junko Hiraga 9 Kazuhisa Mitsuda 10 Masaki Fujimoto 11 Munetaka Ueno 12 Masaki Numazawa 1 Daiki Ishi 1 Ryota Otsubo 1 Aoto Fukushima 1 Hikaru Suzuki 1 Tatsuya Yuasa 1 Sae Sakuda 1 Tomoki Uchino 1
1Physics, Tokyo Metropolitan University, Japan
2Interdisciplinary Space Science, ISAS/JAXA, Japan
3Engineering Mechanical and Space Engineering, Hokkaido University, Japan
4ISEE, Nagoya University, Japan
5Earth and Planetary Science, University of Tokyo, Japan
6Physics, Kanto Gakuin University, Japan
7Physics, Nagoya University, Japan
8Spacecraft Engineering, ISAS/JAXA, Japan
9Physics, Kwansei Gakuin University, Japan
10Space Astronomy and Astrophysics, ISAS/JAXA, Japan
11Solar System Sciences, ISAS/JAXA, Japan
12Space Exploration Innovation Hub Center, JAXA, Japan

GEO-X (GEOspace X-ray imager) is a Japanese CubeSat project to be injected in the vicinity of the Moon. GEO-X aims X-ray imaging of the Earth’s dayside magnetospheric structures including cusps and magneto-sheaths. From past X-ray astronomy observations, charge exchange X-ray emission is observed between solar wind heavy ions (O7+, N5+, …) and neutrals in the Earth’s exosphere. Observational and simulation results strongly suggest that X-rays can be used for imaging of the Earth’s magnetosphere. For this purpose, a 12U CubeSat GEO-X is planned. It will carry a wide field of view X-ray imaging spectrometer composed of an ultra light-weight X-ray telescope and a high-speed Si sensor (Ezoe et al. 2018 J. Astron. Telescope Instrum., 4, 0406001). To observe the X-ray emission from the Earth’s magnetosphere, the satellite will be injected into a high Earth orbit. A launch time will be around the next solar maximum 2022-25.

Yuichiro Ezoe
Yuichiro Ezoe
Tokyo Metropolitan University








Powered by Eventact EMS