隕石の硫黄酸における硫黄と水素同位体異常
G W Cooper1, M H Thiemens, T L Jackson
1SETI Institute and NASA Ames Research Center, MS 239-4, Moffett Field, CA 94035, USA.
まとめ
マーチソン隕石で見つかった有機硫酸は,ユニークな同位体シグネチャーを示しています. これらは,冷たい恒星間環境で形成され,おそらく一硫化炭素前駆体から形成されたことを示唆しています.
科学分野:
- アストロケミストリー アストロケミストリー
- イソトープ地球化学 イソトープ地球化学
背景:
- 隕石には有機化合物が含まれており,初期の太陽系化学に関する手がかりを提供します.
- 有機分子の硫黄と水素の同位体は,その形成条件を示すことができる.
研究 の 目的:
- マーチソン隕石からの有機硫酸の同位体組成を調べるために.
- これらの地球外有機化合物の起源と形成環境を決定する.
主な方法:
- 分子内炭素,水素,硫黄の同位体比の分析.
- デウテリウム/水素 (D/H) と硫黄-33 (33S) の同位体比を測定する.
主要な成果:
- 観測された質量独立の硫黄同位体分離と高いD/H比.
- デュテリウム濃縮は,低温の恒星間環境で炭化水素の形成を示唆しています.
- メタネスルフォニック酸の硫黄-33濃縮は,二酸化炭素前駆体に対する潜在的紫外線照射を示している.
結論:
- オーガニック・スルフォン酸は,おそらく冷たい星間雲で形成された.
- 前駆体には,一硫化炭素のような星間分子が含まれている可能性があります.
- 紫外線照射は形成経路に役割を果たした.
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