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富田 賢吾 研究室
Showing the original Japanese · View translation
星と惑星系のでき方を大規模計算で探る研究室。
AboutAbout the lab
計算機の中で星と円盤の誕生を再現する。
計算宇宙物理学研究室は、
磁場や
計算結果から
こうした
Key terms
- 原始星
- 星に
なる 途中の、 できたばかりの 天体。 周りの ガスが 集まって 作られる - 星周円盤
- 星の
まわりに 広がる 円盤状の ガス。 惑星が できる ときの 初期条件に なる - 輻射磁気流体シミュレーション
- ガスの
流れに、 磁場と 光（輻射）の 影響を 合わせて 計算する 数値シミュレーション - ALMA
- アタカマ大型ミリ波サブミリ波望遠鏡。
若い 原始星や 原始惑星系円盤の 観測を 進めている - AMR
- 計算結果に
合わせ、 必要な 場所にだけ細かい 格子を 動的に 作る 技術
ResearchResearch themes
星や
*Illustrative image原始星と円盤ができる過程
重力で
*Illustrative imageシミュレーションと観測の直接比較
シミュレーションの
*Illustrative image共通で使える計算コードの開発
Princeton高等研究所の
MembersFaculty
- Associate Professor富田 賢吾
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: “HD 163296 protoplanetary disk by ALMA (16CB25B)” ALMA (ESO/NAOJ/NRAO); A. Isella; B. Saxton (NRAO/AUI/NSF) / CC BY 4.0 (cropped)
- 原始星と
円盤が できる 過程: “Feeding a Baby Star with a Dusty Hamburger” ALMA (ESO/NAOJ/NRAO)/ Lee et al. / CC BY 4.0 (cropped) - シミュレーションと
観測の 直接比較: “European Antennas at ALMA's Operations Support Facility” ALMA (ESO/NAOJ/NRAO) / CC BY 4.0 (cropped) - 共通で
使える 計算コードの 開発: “Virginia Tech - data center” Christopher Bowns / CC BY-SA 2.0 (cropped) - Related lab (大向 一行 研究室
（TAP 理論天文学グループ） ): “Hubble2005-01-barred-spiral-galaxy-NGC1300” NASA, ESA, and The Hubble Heritage Team STScI/AURA) / Public domain (cropped) - Related lab (惑星大気物理学分野): “Mars atmosphere” NASA / Public domain (cropped)
- Related lab (宇宙地球電磁気学分野): “Aurora Seen From Space by NASA” NASA -- US government agency / Public domain (cropped)
- Related lab (森下 貴弘 研究室): “NASA-HS201427a-HubbleUltraDeepField” NASA, ESA, H. Teplitz and M. Rafelski (IPAC/Caltech), A. Koekemoer (STScI), R. Windhorst (Arizona State University), and Z. Levay (STScI) / Public domain (cropped)
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