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タイトル: NinjaSat: Astronomical X-ray CubeSat observatory
著者: Tamagawa, Toru
Enoto, Teruaki
Kitaguchi, Takao
Iwakiri, Wataru
Kato, Yo
Numazawa, Masaki
Mihara, Tatehiro
Takeda, Tomoshi
Ota, Naoyuki
Watanabe, Sota
Aoyama, Amira
Iwata, Satoko
Takahashi, Takuya
Yamasaki, Kaede
Hu, Chin-Ping
Takahashi, Hiromitsu
Yoshida, Yuto
Sato, Hiroki
Hayashi, Shoki
Zhou, Yuanhui
Uchiyama, Keisuke
Jujo, Arata
Odaka, Hirokazu
Tamba, Tsubasa
Taniguchi, Kentaro
キーワード: X-rays: general
instrumentation: detectors
space vehicles
space vehicles: instruments
発行日: 2025
出版者: Oxford University Press (OUP)
The Astronomical Society of Japan
誌名: Publications of the Astronomical Society of Japan
巻: 77
号: 3
開始ページ: 466
終了ページ: 479
抄録: NinjaSat is an X-ray CubeSat designed for agile, long-term continuous observations of bright X-ray sources, with the size of 6U (112.7 × 237.1 × 340.5 mm³) and a mass of 8 kg. NinjaSat is capable of pointing at X-ray sources with an accuracy of less than 0゚゚.1 (2σ confidence level) with three-axis attitude control. The satellite bus is a commercially available NanoAvionics M6P, equipped with two non-imaging gas X-ray detectors covering an energy range of 2–50 keV. A total effective area of 32 cm² at 6 keV is capable of observing X-ray sources with a flux of approximately10⁻¹⁰ erg cm⁻² s⁻¹. The arrival time of each photon can be tagged with a time resolution of 61μs. The two radiation belt monitors continuously measure the fluxes of protons above 5 MeV and electrons above 200 keV trapped in the geomagnetic field, alerting the X-ray detectors when the flux exceeds a threshold. The NinjaSat project started in 2020. Fabrication of the scientific payloads was completed in 2022 August, and satellite integration and tests were completed in 2023 July. NinjaSat was launched into a Sun-synchronous polar orbit at an altitude of about 530 km on 2023 November 11 by the SpaceX Transporter-9 mission. After about three months of satellite commissioning and payload verification, we observed the Crab Nebula on 2024 February 9 and successfully detected the 33.8262 ms pulsation from the neutron star. With this observation, NinjaSat met the minimum success criterion and stepped forward to scientific observations as initially planned. By the end of 2024 November, we successfully observed 21 X-ray sources using NinjaSat. This achievement demonstrates that, with careful target selection, we can conduct scientific observations effectively using CubeSats, contributing to time-domain astronomy.
記述: キューブサットX線衛星NinjaSatによる宇宙観測の革新 --決まった時間間隔で爆発を起こす奇妙な中性子星の長期観測-- . 京都大学プレスリリース. 2025-05-29.
著作権等: © The Author(s) 2025. Published by Oxford University Press on behalf of the Astronomical Society of Japan.
This is an Open Access article distributed under the terms of the Creative Commons Attribution License, which permits unrestricted reuse, distribution, and reproduction in any medium, provided the original work is properly cited.
URI: http://hdl.handle.net/2433/294651
DOI(出版社版): 10.1093/pasj/psaf014
関連リンク: https://www.kyoto-u.ac.jp/ja/research-news/2025-05-29-1
出現コレクション:学術雑誌掲載論文等

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