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Updated: Feb 28, 2026

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Scattering And Absorption of Light in Planetary Regoliths
Published on: July 1, 2019
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67P/Churyumov-Gerasimenkoのキセノン同位体は,彗星が地球の大気に寄与したことを示しています
B Marty1, K Altwegg2,3, H Balsiger2
1Centre de Recherches Pétrographiques et Géochimiques, CNRS, Université de Lorraine, 15 rue Notre Dame des Pauvres, BP 20, 54501 Vandoeuvre lès Nancy, France. bmarty@crpg.cnrs-nancy.fr.
まとめ
彗星67P/チュリュモフ・ゲラシメンコ
科学分野:
- 惑星科学
- 宇宙化学
- 天体生物学
背景:
- 彗星の物質の起源と 惑星の内部の大気の形成における役割は 重要な科学的な問題です
- 彗星の組成を理解することで 初期の太陽系についての洞察が得られます
研究 の 目的:
- 彗星67P/チュリュモフ・ゲラシメンコのクセノンの同位体成分を分析する.
- 彗星からのクセノンの地球大気への貢献を 決定するためです
主な方法:
- ローゼッタ宇宙船に搭載されたイオンと中性分析のためのローゼッタ軌道スペクトロメーター (ROSINA) が使用された.
- 低高度の軌道で彗星のガスの詳細な分析が可能になった.
主要な成果:
- 彗星67P/チュリュモフ・ゲラシメンコのキセノン同位体は重量同位体の欠乏を示した.
- 同位体記号は 大気の原始成分と一致する
結論:
- 彗星は地球の大気の形成に大きく貢献した可能性がある.
- 地球の大気中のクセノンの約22%は,コンドリートクセノンのほかに彗星からのものです.
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