LAB LOGA page on LabLog, a review site (not the lab's official page)
理論宇宙進化学研究室
Showing the original Japanese · View translation
星と惑星の誕生と進化を理論と観測で探る研究室。
AboutAbout the lab
星と惑星の誕生を、理論とシミュレーションで探る。
理論宇宙進化学研究室は、
星や
その
誕生したばかりの
ALMAなどでの
Key terms
- 分子雲コア
- 星の
母体と なる 分子雲の 中で、 特に 密度が 高い 部分。 重力で 収縮すると、 中心に 星と 円盤が できる - 原始惑星系円盤
- 誕生したばかりの
星の まわりに 広がる、 ガスと 塵の 円盤。 塵が 集まって 惑星の 材料に なると 考えられている - ALMA
- 南米チリの
高地に 設置された 電波望遠鏡。 星や 円盤の 姿を 高い 解像度で 描き出せる - 磁気回転不安定性
- 磁場の
働きで 生じる 不安定性で、 原始惑星系円盤の 中で 乱流を 引き起こすと 考えられている。 略称は MRI
ResearchResearch themes
この
*Illustrative imageALMA望遠鏡で探る星と惑星の誕生
ALMA望遠鏡の
*Illustrative image星形成の環境とダストの運動・成長
3次元の
*Illustrative image星のゆりかごに広がる放射状のガス構造
複数の
*Illustrative image磁場がダストの成長に与える影響
磁気回転不安定性に
MembersFaculty
- Professor町田 正博
- Associate ProfessorDoris Arzoumanian
VoicesStudent voices
Ratings and reviews reflect the experiences of individual current or former students, not the lab's official views. Whether a lab has reviews, or how many, says nothing about the lab itself.
Students who take part in an interview may receive a thank-you gift worth ¥1,000, regardless of what they say.
Student ratings (0 students)
--
--
--
--
--
--
Student voices answer questions like these
- What's great about this lab?
- What did you learn after joining?
- What's the vibe, and what is the professor like?
- Who is this lab for?
- Where do graduates go?
Your experience can help younger students choose their lab. Your name won't be shown.
Write a lab reviewAnonymous · Your draft is saved if you stopRelatedLabs similar to 理論宇宙進化学研究室
The information on this page is compiled by the LabLog team from the lab's public information and interviews. For corrections or removal requests, please contact LabLog, not the lab.
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: “Protoplanetary disk HH-30” NASA / Public domain (cropped)
- ALMA望遠鏡で
探る 星と 惑星の 誕生: “Disco anular con forma de media luna en torno al sistema protoplanetario IRS 48” Manferna78 / CC BY-SA 4.0 (cropped) - 星形成の
環境と ダストの 運動・成長: “Stages of Star Formation (webb potm2605a)” ESA/Webb, NASA & CSA, T. Megeath, M. Zamani (ESA/Webb) Acknowledgement: M. H. Özsaraç / Public domain (cropped) - 星の
ゆりか ごに 広がる 放射状の ガス構造: “Herschel’s view of a molecular cloud ESA384010” European Space Agency / CC BY-SA 3.0 igo (cropped) - 磁場が
ダストの 成長に 与える 影響: “Birefringence” Vektorfeld / CC BY-SA 4.0 (cropped) - Related lab (物質宇宙進化学研究室): “Namibie Hoba Meteorite 05” No machine-readable author provided. Calips assumed (based on copyright claims). / CC BY 2.5 (cropped)
- Related lab (太陽地球系物理学研究室): “Mercury’s magnetosphere during BepiColombo’s third flyby (annotated) ESA501746” European Space Agency / CC BY-SA 3.0 igo (cropped)
- Related lab (大気流体力学研究室): “PSM V53 D324 General circulation of atmosphere” 作者不詳 / Public domain (cropped)
- Related lab (地球惑星博物学研究室): “Uncoiled Lower Creataceous Ammonites from Northern Bulgaria (Coll. N. Dimitrova) at the Sofia University 'St. Kliment Ohridski' Museum of Paleontology and Historical Geology” Motekov / CC BY-SA 4.0 (cropped)
About LabLog
LabLog is a lab review app for students only. Student members at each university interview students in labs and publish what they say. Student voices can only be read by students who sign up with a university email address. Operated by bestiee Inc.
Learn more about LabLog ↗Search engines and AI may reference the basic lab info and rating summaries on this page and the description of LabLog. Student voices are for student members only. Automated collection by programs (scraping, or input to or training of AI) is prohibited under Article 8 of the Terms of Service. If you need data for research or analysis, please contact us.