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三浦弥生研究室（同位体地球惑星科学）
Showing the original Japanese · View translation
同位体の分析から、惑星や隕石の歩みをたどる研究室。
AboutAbout the lab
同位体から読む、惑星と隕石の歴史。
三浦研究室は、
同位体の
希ガスや
Key terms
- 同位体
- 同じ
元素で 重さだけが 違う 原子。 割合を 調べると、 物質の 起源や 年代が 分かる - 希ガス
- ヘリウムや
ネオン、 アルゴンなど、 ほかの 物質と ほとんど 反応しない 気体の 元素 - 母天体
- 隕石が
もともと 属していた、 小惑星などの 大きな 天体
ResearchResearch themes
同位体の
MembersFaculty
- Associate Professor三浦 弥生Publications ↗
VoicesStudent voices
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Student ratings (0 students)
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Write a lab reviewAnonymous · Your draft is saved if you stopThe 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: “Bishopville meteorite, aubrite ( )” James St. John / CC BY 2.0 (cropped)
- 同位体で
探る 天体の 進化: “Pena Blanca Spring meteorite, part slice” Jon Taylor / CC BY-SA 2.0 (cropped)
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