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山崎研究室
Showing the original Japanese · View translation
X線で銀河団やダークマターを観測し、新しい検出器もつくる研究室。

AboutAbout the lab
X線の目で、宇宙の高温ガスを見る。
山崎研究室は、
宇宙航
銀河団や
X線分光撮像衛星XRISMなどの
Key terms
- 銀河団
- たくさんの
銀河が 重力で 集まった、 宇宙で 最大級の 天体の 集まり。 高温の ガスに 満たされている - ダークマター
- 光では
見えないが、 重力を 通して 存在が 分かる 正体 不明の 物質。 暗黒物質とも 呼ぶ - マイクロカロリメータ
- X線が
当たった ときの ごく わずかな 温度上昇から、 その エネルギーを 精密に 測る 検出器
ResearchResearch themes
ビッグバンから
*Illustrative imageX線で見る宇宙の高温ガス
銀河間の
*Illustrative imageX線分光撮像衛星XRISM
2023年9月に
*Illustrative imageTES型X線マイクロカロリメータの開発
超
MembersFaculty
山崎研究室の
- Professor山崎 典子
VoicesStudent voices
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Report an errorAbout the images
The top and research theme images are illustrative and were not taken at the lab. They are cropped from Wikimedia Commons images. Cropped CC BY-SA images are provided under the same CC BY-SA license as the original (version shown on each line).
- Top image: “XRISM Model” テレストレラッソ / CC BY-SA 4.0 (cropped)
- X線で
見る宇宙の 高温ガス: “XRISM Reveals Its First Look at X-ray Cosmos (SVS14492 - Xtend Abell 2319 with DSS and frame)” NASA's Scientific Visualization Studio - Francis Reddy, Jeanette Kazmierczak, Scott Wiessinger, Sophia Roberts / Public domain (cropped) - X線分光撮像衛星XRISM: “XRISM 001” NASA's Goddard Space Flight Center Conceptual Image Lab / Public domain (cropped)
- TES型X線マイクロカロリメータの
開発: “XRISM Resolve Animation (SVS14244)” NASA's Scientific Visualization Studio - Scott Wiessinger, Francis Reddy, Brian J. Williams / Public domain (cropped)
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