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橘研究室
Showing the original Japanese · View translation
実験と分析と探査で、太陽系のはじまりの化学を解き明かす研究室。

AboutAbout the lab
太陽系のはじまりを、実験と分析から。
橘研究室は、
実験室での
ケイ酸塩や
小惑星の
Key terms
- コンドライト
- 小さな
球の 粒(コンドルール)を ふくむ、 もっとも ありふれた 種類の 隕石 - 原始惑星系円盤
- 生まれた
ばかりの 星の まわりを 取り巻く、 ガスと 塵で できた 円盤 - プレソーラー粒子
- 太陽系が
できる 前に、 別の 星の まわりで つくられた 微粒子
ResearchResearch themes
地球を
*Illustrative image太陽系初期の化学進化
蒸発や
*Illustrative image銀河・分子雲と太陽系
元素合成や
*Illustrative image星のまわりでのダスト形成
進化した
*Illustrative imageコンドライトの構成物の形成
Ca・
MembersFaculty
- Professor橘 省吾Publications ↗
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RelatedLabs similar to 橘研究室
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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: “HL Tau protoplanetary disk” ALMA (ESO/NAOJ/NRAO) / CC BY 4.0 (cropped)
- 太陽系初期の
化学進化: “Artist’s impression of grains in the disc around a brown dwarf (eso1248b)” ALMA (ESO/NAOJ/NRAO)/L. Calçada (ESO) / CC BY 4.0 (cropped) - 銀河・分子雲と
太陽系: “Infrared Rho Ophiuchi Complex” Judy Schmidt / CC BY 2.0 (cropped) - 星の
まわりでの ダスト形成: “Structure of the pulsating red giant S Ori (artist's impression)” ESO / CC BY 4.0 (cropped) - コンドライトの
構成物の 形成: “Hart CK3 Chondrule-5mmFOV-01” North Creaton / CC BY-SA 4.0 (cropped) - Related lab (黒川研究室(Kurokawa-lab)): “HL Tau protoplanetary disk” ALMA (ESO/NAOJ/NRAO) / CC BY 4.0 (cropped)
- Related lab (竝木研究室
(RISE 月惑星探査検討室) ): “PIA16587 - GRAIL's Gravity Field of the Moon” NASA/ARC/MIT / Public domain (cropped) - Related lab (天野研究室): “Supernova Remnant SN 1006” X-ray: NASA/CXC/Rutgers/G.Cassam-Chenaï, J.Hughes et al.; Radio: NRAO/AUI/NSF/GBT/VLA/Dyer, Maddalena & Cornwell; Optical: Middlebury College/F.Winkler, NOAO/AURA/NSF/CTIO Schmidt & DSS / CC BY 4.0 (cropped)
- Related lab (生駒研究室
(系外惑星理論グループ) ): “Artist's Impression of Kepler 138 Planetary System (2022-048)” NASA, ESA, Leah Hustak (STScI) / CC BY 4.0 (cropped)
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