日本地球惑星科学連合2022年大会

講演情報

[E] 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-CG18] 宇宙・惑星探査の将来計画および関連する機器開発の展望

2022年5月31日(火) 11:00 〜 13:00 オンラインポスターZoom会場 (4) (Ch.04)

コンビーナ:坂谷 尚哉(立教大学 理学部 物理学科)、コンビーナ:小川 和律(宇宙航空研究開発機構)、吉岡 和夫(東京大学大学院新領域創成科学研究科)、コンビーナ:横田 勝一郎(大阪大学・理学研究科)、座長:坂谷 尚哉(立教大学 理学部 物理学科)、小川 和律(宇宙航空研究開発機構)、吉岡 和夫(東京大学大学院新領域創成科学研究科)、横田 勝一郎(大阪大学・理学研究科)

11:00 〜 13:00

[PCG18-P01] Test results of the breadboard-model ion mass spectrometer for the Comet Interceptor mission

*笠原 慧1渡辺 瑞穂1川島 桜也1横田 勝一郎2斎藤 義文3浅村 和史3平原 聖文4 (1.東京大学、2.大阪大学、3.宇宙科学研究所、4.名古屋大学)

Comets are pristine small bodies and thus provide key information about the solar system evolution. Remote observations by ground observatories have characterized various comets, while in-situ observations by spacecraft have brought much more detailed information on several comets. However, the direct observations by spacecraft fly-by or rendezvous have been limited to the short-period comets, which neared the sun many times in the past and thus lost some of primitive characteristics. The Comet Interceptor mission, led by ESA, aims at a long period comet or an interstellar object. JAXA will provide an ultra-small (24 U) daughter spacecraft (probe B1), whose closest approach will be less than 1,000 km, allowing the first-ever multi-spacecraft fly-by observations of a comet. Probe B1 will be equipped with three scientific instruments: (1) the Plasma Suite, which is comprised of an ion mass spectrometer and a three-axis magnetometer, (2) the Hydrogen Imager, and (3) the Narrow/wide Angle Cameras. Here we report our test results of the breadboard-model ion mass spectrometer. The mass resolution obtained in the laboratory experiment is M/dM > 30, which agrees with the numerical simulation. It enables the discrimination among carbon, nitrogen, and oxygen ions, which are major elements in cometary comae.