Japan Geoscience Union Meeting 2022

Presentation information

[E] Oral

P (Space and Planetary Sciences ) » P-CG Complex & General

[P-CG18] Future missions and instrumentation for space and planetary science

Mon. May 23, 2022 1:45 PM - 3:15 PM 303 (International Conference Hall, Makuhari Messe)

convener:Naoya Sakatani(Department of Physics, Rikkyo University), convener:Kazunori Ogawa(Japan Aerospace Exploration Agency), Kazuo Yoshioka(Graduate School of frontier Science, The University of Tokyo), convener:Shoichiro Yokota(Graduate School of Science, Osaka University), Chairperson:Shoichiro Yokota(Graduate School of Science, Osaka University), Kazuo Yoshioka(Graduate School of frontier Science, The University of Tokyo), Naoya Sakatani(Department of Physics, Rikkyo University), Kazunori Ogawa(Japan Aerospace Exploration Agency)

3:00 PM - 3:15 PM

[PCG18-12] Development of an ultra-lightweight X-ray telescope using MEMS technology

*Hiromi Morishita1, Yuichiro Ezoe 1, Kumi Ishikawa 1, Masaki Numazawa1, Daiki Ishi1, Aoto Fukushima1, Tomoki Uchino1, Sae Sakuda1, Ayata Inagaki1, Yoko Ueda1, Luna Sekiguchi1, Yukine Tsuji1, Takatoshi Murakawa1, Kazuhisa Mitsuda2, Kohei Morishita3, Kazuo Nakajima4, Yoshiaki Kanamori4 (1.Tokyo Metropolitan University, 2.National Astronomical Observatory of Japan, 3.Kyushu University, 4.Tohoku University)


Keywords:MEMS, GEO-X, X-ray telescope

We have been developing an ultra-lightweight Wolter type-I X-ray telescope fabricated with micro electro mechanical systems (MEMS) technologies for GEO-X (GEOspace X-ray Imager) mission. GEO-X will aim for global imaging of the Earth's magnetosphere using X-rays. The MEMS X-ray telescope utilizes sidewalls of micropores formed by deep reactive ion etching on a 4-inch Si wafers for X-ray mirrors. The sidewalls are smoothed by high-temperature hydrogen annealing and chemical mechanical polishing processes. The Si wafers are plastically deformed into a spherical shape to focus X-rays. Sidewalls are coated with Pt using the atomic layer deposition method. Finally, two wafers are assembled to form a Wolter I-type telescope. In this talk we show our recent development to smooth the sidewalls in order to achieve an angular resolution of 10 arcmin required in the GEO-X mission and describe environmental test results.