Curriculum Vitaes
Profile Information
- Affiliation
- Senior Researcher, Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency
- Degree
- 博士(理学)(東京大学)
- ORCID ID
https://orcid.org/0000-0001-6366-2608- J-GLOBAL ID
- 200901078920834652
- researchmap Member ID
- 5000019324
Research Areas
2Research History
7-
Apr, 2016 - Sep, 2024
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Oct, 2015 - Mar, 2016
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Apr, 2005 - Sep, 2015
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Apr, 2004 - Mar, 2005
Education
3-
Apr, 1996 - Mar, 1999
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Apr, 1993 - Mar, 1995
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Apr, 1989 - Mar, 1993
Committee Memberships
2-
Apr, 2015 - Present
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Apr, 2009 - Mar, 2015
Awards
2Papers
288-
The Planetary Science Journal, Dec 1, 2025Impact ejecta with velocities exceeding the escape velocity of planetary bodies become meteorites and dust particles in interplanetary space. We present a new method that allows simultaneous measurement of the size and velocity of the largest high-velocity ejecta. High-speed camera images revealed the time required for the ejecta to reach the secondary target, and ejecta size was determined after the experiment by analyzing the craters formed upon their impact on the secondary target. We defined the size─velocity relationships of submillimeter ejecta with velocities exceeding 1 km s−1, focusing on the largest detectable ejecta in our experiments. The results show that millimeter-sized meteoroids impacting the rocky surfaces of planetary bodies at 7 km s−1 eject particles up to a few tens of micrometers in size toward interplanetary space at velocities exceeding the escape velocity of the body, even when it is greater than 1 km s−1....
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Discover Life, 55(1), Sep, 2025In space, asteroids have collided with planets and satellites throughout their long history, and many types of organic molecules have been synthesized. In particular, on satellites with gas atmospheres such as titan, a satellite of saturn, asteroid impacts cause hot reactions in a hot gas plume. To investigate the effects of asteroid impacts, simulation experiment has been carried out using a two-stage light-gas gun in nitrogen gas. we used a small polycarbonate bullet to impact on an iron-based target in nitrogen gas at a pressure of 100 kpa and a speed of approximately 7 km/s. As a result, many carbonaceous nanoparticles were produced. By analyzing the produced soot, using a water extraction method, a dabsylation method and a liquid chromatography method, we detected markedly large amounts of amino acids (glycine and alanine). The reaction process in the hot gas plume was considered. Many types of radicals collide with each other in nitrogen gas and the impact provides a suitable environment for the synthesis of amino acids and precursors of amino acids....
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International Journal of Impact Engineering, Aug, 2025High velocity impact experiments were conducted on a conical shaped sand target, simulating a large-scale cratering formed in gravity-dominated regime, which could be affected by a surface topography such as curvature of bodies. The target material consists of dry quartz sand, prepared in conical shape with its vertex angle 120° A spherical Al projectile with its diameter of 2 mm was impacted vertically on the top part of a cone at the velocity from 1 to 4 km/s. After the impact, a top part of the conical target was excavated to form a shallow bowl-shaped crater on the top. The target resembled a trapezoid when observed from the side. The crater rim radius was able to be scaled by a conventional π-scaling relationship although it's radius was about 10 % smaller than that of the crater formed on semi-infinite flat surface. This might be caused by the geometrical effect of the target. The ejecta opening angle was measured at the time of crater formation and it was about 130°, where this is larger than that of the ejecta curtain, <90°, formed over the target of semi-infinite flat surface. This wider ejecta opening angle on conical target was able to be well reproduced by utilizing the Maxwell Z-model to a conical target....
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Journal of Spacecraft and Rockets, (in press), Jul, 2025 Peer-reviewedElectrodynamic tethers are promising for removing debris but may be severed when they collide with orbital debris. Hollow cylindrical tethers (HCTs) had more severance-resistant designs than conventional solid cylindrical tethers (SCTs) because of their larger diameters for the same weight. However, high survivability could not be achieved if the cross-sectional shape of the HCT deviated from a cylindrical one. In this paper, we propose a novel device called a shape keeper (SK) that maintains the shape of the HCT. We propose three SKs made of different materials: aluminum, nonconductive polyurethane foam, and conductive polyurethane foam. The proposed SKs are evaluated in three aspects. First, the collision damage to a HCT with SKs is evaluated through hypervelocity collision experiments. The introduced SK functions as a bumper and suppresses tether damage depending on the collision point. Second, the debris removal time is investigated by considering the influence of the installed SKs on the debris removal mission. Third, the survivability of the HCT with SKs is assessed according to the two aforementioned evaluations. The results indicate that HCTs with SKs are superior to conventional SCTs in terms of survivability with the same weight....
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Journal of Space Safety Engineering, Jun, 2025
Misc.
635-
スペース・プラズマ研究会・講演集(Web), 2010 43 (WEB ONLY), 2011
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Abstracts of Annual Meeting of the Geochemical Society of Japan, 58 175-175, 2011始原小天体有機物は、太陽系および生命原材料物質の起源と進化を理解するための重要な情報を記録している。「たんぽぽ計画」では、大気圏突入時の熱変成や地上での汚染を受けていない宇宙塵を、国際宇宙ステーション上に超低密度シリカエアロゲルを設置して回収を試みる予定である。しかし、この方法では、宇宙塵のエアロゲルへの衝突により変成する可能性を考慮する必要がある。そこで本研究では、宇宙科学研究所・スペースプラズマ実験施設の二段式高速ガス銃を用いて、隕石微粒子の高速衝突模擬実験を行い、マーチソン隕石微粒子をシリカエアロゲルに撃ち込んだものを取り出し、2枚のアルミ板にはさみハンドプレスして圧着された隕石微粒子を、片方のアルミ板に載せた状態で、赤外顕微分光装置と顕微ラマン分光装置で測定を行った。また、SPring-8, BL43IRの高輝度赤外顕微分光装置IFS120HRでイメージング測定を行い、衝突前後の隕石有機物の分子構造の変化を見出すことを目的とした。
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Abstracts Fall Meeting of the Japanese Society for Planetary Sciences, 2010 90-90, Oct 6, 2010
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日本惑星科学会秋期講演会予稿集, 2010 91-91, Oct 6, 2010
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Abstract of Dusty Visions 2010: A Workshop on Dust Spectroscopy and Dust Astronomy, Jul, 2010
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応用物理学関係連合講演会講演予稿集(CD-ROM), 57th ROMBUNNO.19P-G-18, Mar 3, 2010
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法政大学情報メディア教育研究センター研究報告(Web), 23, 2010
Major Presentations
132Professional Memberships
3Research Projects
17-
科学研究費助成事業, 日本学術振興会, Apr, 2024 - Mar, 2028
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Grants-in-Aid for Scientific Research Grant-in-Aid for Scientific Research (A), Japan Society for the Promotion of Science, Apr, 2022 - Mar, 2026
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科学研究費助成事業 基盤研究(B), 日本学術振興会, Apr, 2021 - Mar, 2024
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科学研究費助成事業 基盤研究(B), 日本学術振興会, Apr, 2021 - Mar, 2024
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Grants-in-Aid for Scientific Research Grant-in-Aid for Scientific Research (C), Japan Society for the Promotion of Science, Apr, 2020 - Mar, 2023