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中本研究室
Showing the original Japanese · View translation
星や惑星がどう生まれるのかを、理論とシミュレーションで探る研究室。
AboutAbout the lab
円盤、ダスト、輻射で星と惑星の誕生に迫る。
中本研究室は、
星や
「円盤」
惑星が
Key terms
- 原始惑星系円盤
- 生まれた
ばかりの 星を 取り囲む、 ガスと ちりの 円盤。 ここから 惑星が 生まれると 考えられている - ダスト粒子
- 原始惑星系円盤の
ガスに 含まれる、 氷や 岩石、 金属などの 小さな 固体の 粒 - 輻射
- 天体が
放つ光や 熱の エネルギー。 その 伝わり方を 計算するのが 輻射輸送計算
ResearchResearch themes
星・惑星系が
*Illustrative image原始惑星系円盤の形成と進化
惑星を
*Illustrative image円盤の中のダスト粒子の進化
円盤の
*Illustrative image重い星のでき方
太陽より
*Illustrative image系外惑星の大気
中
MembersFaculty
中本研究室の
- Professor中本 泰史Publications ↗
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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.
- Top image: “Artist’s impression of protoplanetary disc (weic2329a)” ESO/L. Calçada / CC BY 4.0 (cropped)
- 原始惑星系円盤の
形成と 進化: “TW Hydrae protoplanetary disc” S. Andrews (Harvard-Smithsonian CfA); B. Saxton (NRAO/AUI/NSF); ALMA (ESO/NAOJ/NRAO) / CC BY 4.0 (cropped) - 円盤の
中の ダスト粒子の 進化: “NWA 5930 Meteorite Thin Section Chondrule - Image 7” Solar Anamnesis / CC0 (cropped) - 重い星のでき方: “NASA’s Webb Reveals Cosmic Cliffs, Glittering Landscape of Star Birth” NASA, ESA, CSA, STScI / Public domain (cropped)
- 系外惑星の
大気: “Illustration (Artist’s Impression) of WASP-39 b and Its Star (weic2221a)” NASA, ESA, CSA, J. Olmsted (STScI) / CC BY 4.0 (cropped) - Related lab (奥住研究室): “HL Tau protoplanetary disk” ALMA (ESO/NAOJ/NRAO) / CC BY 4.0 (cropped)
- Related lab (玄田研究室): “The Earth seen from Apollo 17” NASA/Apollo 17 crew / Public domain (cropped)
- Related lab (佐藤研究室): “Subaru Telescope on Mauna Kea (geminiann12013b)” International Gemini Observatory/NOIRLab/NSF/AURA/Subaru Observatory / CC BY 4.0 (cropped)
- Related lab (癸生川研究室): “Carbonaceous chondrite (Murchison Meteorite) ( )” James St. John / CC BY 2.0 (cropped)
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