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酒井 剛 研究室
Showing the original Japanese · View translation
電波望遠鏡で恒星の誕生を探り、受信機も自ら開発する研究室。

AboutAbout the lab
恒星の誕生の仕組みを、電波で解き明かす。
酒井研究室は、
特に、
既存の
星が
Key terms
- 大質量星
- 太陽の
8倍以上の 質量を 持つ恒星。 一生の 最後に 超新星爆発を 起こす - 分子雲
- 恒星が
生まれる 元に なる 希薄な ガス雲。 重力で 収縮して 恒星に なる - スペクトル線
- 分子などが
出す電波の 線。 強さから、 どんな 分子が どれくらい あるか 分かる - SIS素子
- 超伝導トンネル接合を
用いた 素子。 ミリ波サブミリ波帯の 電波観測に 使われる
NewsLab news
学部の
学生が、 電子情報通信学会 ジュニア&学生ポスターセッションで 特別賞を 受賞 修士課程の
学生が、 電子工学 プログラムの 修論発表会で 優秀発表賞を 受賞 学部の
学生が、 III類電子工学 プログラムの 卒業論文発表会で 優秀発表賞を 受賞 学部の
学生が、 III類電子工学 プログラムの 輪講発表会で 優秀発表賞を 受賞 修士課程の
学生が、 電子工学 プログラムの 修論発表会で 優秀発表賞を 受賞
ResearchResearch themes
この
*Illustrative image電波観測による星形成過程の解明
恒星は、
*Illustrative image大質量星の形成過程
太陽の
*Illustrative imageスペクトル線で星形成の進化を探る
分子が
*Illustrative image電波望遠鏡用の受信機の開発
アルマ望遠鏡と
MembersFaculty
酒井研究室の
- Professor酒井 剛
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: “Mount Pleasant Radio Telescope” Noodle snacks / CC BY-SA 3.0 (cropped)
- 電波観測に
よる 星形成過程の 解明: “The Very Large Telescope Snaps a Stellar Nursery and Celebrates Fifteen Years of Operations” ESO / CC BY 4.0 (cropped) - 大質量星の
形成過程: “Star-forming Region G” Credit: NASA, ESA, and J. Tan (Chalmers University of Technology); Processing; Gladys Kober (NASA/Catholic University of America) / Public domain (cropped) - スペクトル線で
星形成の 進化を 探る : “Cone Nebula (NGC 2264) Star-Forming Pillar of Gas and Dust” NASA, H. Ford (JHU), G. Illingworth (UCSC/LO), M.Clampin (STScI), G. Hartig (STScI), the ACS Science Team, and ESA The ACS Science Team: H. Ford, G. Illingworth, M. Clampin, G. Hartig, T. Allen, K. Anderson, F. Bartko, N. Benitez, J. Blakeslee, R. Bouwens, T. Broadhurst, R. Brown, C. Burrows, D. Campbell, E. Cheng, N. Cross, P. Feldman, M. Franx, D. Golimowski, C. Gronwall, R. Kimble, J. Krist, M. Lesser, D. Magee, A. Martel, W. J. McCann, G. Meurer, G. Miley, M. Postman, P. Rosati, M. Sirianni, W. Sparks, P. Sullivan, H. Tran, Z. Tsvetanov, R. White, and R. Woodruff. / CC BY 4.0 (cropped) - 電波望遠鏡用の
受信機の 開発: “Sample radio telescope receiver, )” Science Museum London / Science and Society Picture Library / CC BY-SA 2.0 (cropped) - Related lab (坂野 昌人 研究室): “CSIRO ScienceImage 2578 Preparing a Protein Crystal sample for Xray” North Sullivan Photography, CSIRO / CC BY 3.0 (cropped)
- Related lab (上野 芳康 研究室): “Propagation of light through the core of an optical fiber. Macro visualization.” AZToshkov / CC BY-SA 3.0 (cropped)
- Related lab (加藤 峰士 研究室): “Frequency Comb ( )” National Institute of Standards and Technology / Public domain (cropped)
- Related lab (大饗 千彰 研究室): “Nonlinear Processes” Benjamin Cromey / Public domain (cropped)
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