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梅田研究室
Showing the original Japanese · View translation
星の一生と最期の大爆発、元素の起源を数値計算で探る研究室。
AboutAbout the lab
星の最期から、元素の起源へ。
梅田研究室は、
重い星が
爆発の
学部の
Key terms
- 超新星
- 重い
星などが 一生の 最後に 起こす大爆発。 急に 明るく 輝き、 星の 中で できた 元素を 宇宙に まき散らす - ガンマ線バースト
- 宇宙の
どこかで 突然、 強い ガンマ線が 短い 時間だけ放たれる 現象。 宇宙で 最も 激しい 爆発の 一つ - 元素合成
- 星の
中の 核融合や 爆発の ときに、 軽い 元素から 重い 元素が つくられる こと
NewsLab news
View More ↗ResearchResearch themes
超
*Illustrative image重い星の進化・爆発と元素の起源
超
*Illustrative image超新星残骸に残る爆発直前の記憶
国際共同研究グループの
MembersFaculty
梅田研究室の
- Associate Professor梅田 秀之
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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: “EtaCarinae” Nathan Smith (University of California, Berkeley), and NASA / Public domain (cropped)
- 重い星の
進化・爆発と 元素の 起源: “SN 1987A HST” ESA/Hubble & NASA / CC BY 4.0 (cropped) - 超新星残骸に
残る 爆発直前の 記憶: “Crab Nebula” NASA, ESA, J. Hester and A. Loll (Arizona State University) / Public domain (cropped) - Related lab (藤井研究室): “Full Hubble ACS Image of NGC )” NASA, ESA, and the Hubble Heritage (STScI/AURA)-ESA/Hubble Collaboration / Public domain (cropped)
- Related lab (柏川研究室): “Subaru Telescope. Mauna Kea Summit ( )” Robert Linsdell / CC BY 2.0 (cropped)
- Related lab (戸谷研究室): “Cosmic web” Volker Springel / Max Planck Institute For Astrophysics / CC BY-SA 4.0 (cropped)
- Related lab (嶋作研究室): “Webb's First Deep Field” NASA, ESA, CSA, and STScI / Public domain (cropped)
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