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- XRISM acronyme de X-Ray Imaging and Spectroscopy Mission (auparavant XARM pour X-ray Astronomy Recovery Mission) est un télescope spatial à rayons X mous développé par l'agence spatiale japonaise JAXA. Il reprend une partie de l'instrumentation du télescope Hitomi qui s'était désintégré en mars 2016 peu après son lancement durant son déploiement sans avoir pu fournir une seule donnée scientifique. Le lancement de XRISM est prévu en 2022. (fr)
- The X-Ray Imaging and Spectroscopy Mission (XRISM, pronounced "crism"), formerly the X-ray Astronomy Recovery Mission (XARM), is an X-ray astronomy satellite of the Japan Aerospace Exploration Agency (JAXA) to provide breakthroughs in the study of structure formation of the universe, outflows from galaxy nuclei, and dark matter. As the only international X-ray observatory project of its period, XRISM will function as a next generation space telescope in the X-ray astronomy field, similar to how the James Webb Space Telescope, Fermi Space Telescope, and the Atacama Large Millimeter Array (ALMA) Observatory are placed in their respective fields. The mission is a stopgap for avoiding a potential observation period gap between X-ray telescopes of the present (Chandra, XMM-Newton) and those of the future (Advanced Telescope for High Energy Astrophysics (ATHENA), Lynx X-ray Observatory). Without XRISM, a blank period in X-ray astronomy may arise in the early 2020s due to the loss of Hitomi. During its formulation, XRISM/XARM was also known as the "ASTRO-H Successor" or "ASTRO-H2". (en)
- X線分光撮像衛星（えっくすせんぶんこうさつぞうえいせい）、XRISM（クリズム、X-Ray Imaging and Spectroscopy Mission）は、2016年に姿勢制御系の不具合のため短期間で運用終了したX線天文衛星「ひとみ」の代替機として、宇宙航空研究開発機構 (JAXA) 宇宙科学研究所 (ISAS) が開発中のX線天文衛星。「ひとみ」と同じく、アメリカ航空宇宙局 (NASA)、欧州宇宙機関 (ESA) との国際協力ミッションである。特にNASAではJAXA主導の下に行うジョイント・プロジェクトとして位置付けしている。 (ja)
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- XARM (en)
- XRISM (en)
- ASTRO-H Successor (en)
- ASTRO-H2 (en)
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- XARM (en)
- XRISM (en)
- ASTRO-H Successor (en)
- ASTRO-H2 (en)
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- X-ray astronomy satellite in Japan (en)
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- Soft X-ray Telescope (en)
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- XRISM acronyme de X-Ray Imaging and Spectroscopy Mission (auparavant XARM pour X-ray Astronomy Recovery Mission) est un télescope spatial à rayons X mous développé par l'agence spatiale japonaise JAXA. Il reprend une partie de l'instrumentation du télescope Hitomi qui s'était désintégré en mars 2016 peu après son lancement durant son déploiement sans avoir pu fournir une seule donnée scientifique. Le lancement de XRISM est prévu en 2022. (fr)
- X線分光撮像衛星（えっくすせんぶんこうさつぞうえいせい）、XRISM（クリズム、X-Ray Imaging and Spectroscopy Mission）は、2016年に姿勢制御系の不具合のため短期間で運用終了したX線天文衛星「ひとみ」の代替機として、宇宙航空研究開発機構 (JAXA) 宇宙科学研究所 (ISAS) が開発中のX線天文衛星。「ひとみ」と同じく、アメリカ航空宇宙局 (NASA)、欧州宇宙機関 (ESA) との国際協力ミッションである。特にNASAではJAXA主導の下に行うジョイント・プロジェクトとして位置付けしている。 (ja)
- The X-Ray Imaging and Spectroscopy Mission (XRISM, pronounced "crism"), formerly the X-ray Astronomy Recovery Mission (XARM), is an X-ray astronomy satellite of the Japan Aerospace Exploration Agency (JAXA) to provide breakthroughs in the study of structure formation of the universe, outflows from galaxy nuclei, and dark matter. As the only international X-ray observatory project of its period, XRISM will function as a next generation space telescope in the X-ray astronomy field, similar to how the James Webb Space Telescope, Fermi Space Telescope, and the Atacama Large Millimeter Array (ALMA) Observatory are placed in their respective fields. The mission is a stopgap for avoiding a potential observation period gap between X-ray telescopes of the present (Chandra, XMM-Newton) and those of (en)
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- X-Ray Imaging and Spectroscopy Mission (fr)
- X線分光撮像衛星 (ja)
- X-Ray Imaging and Spectroscopy Mission (en)
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