土星 の 大気 と 環 の 間 の 化学 的 相互作用
J H Waite1, R S Perryman2, M E Perry3
1Space Science and Engineering Division, Southwest Research Institute, San Antonio, TX 78238, USA. hwaite@swri.edu.
まとめ
土星
科学分野:
- 惑星科学
- 大気化学
- 宇宙物理学
背景:
- 初期のミッションでは 土星の環と大気の間の化学相互作用が示唆されました
- この相互作用を理解すると 環の組成と大気の影響が分かります
研究 の 目的:
- 土星の大気構造を記述する.
- 環から大気への物質の流入を量化します.
主な方法:
- カッシーニ・イオン・ニュートラル・マス・スペクトロメーターを用いた現地測定.
- カッシーニ宇宙船のグランドフィナーレのデータ分析
主要な成果:
- 土星の大気中のヘリウム/水素 (He/H2) の比率は10~16%と決定された.
- 揮発性化合物 (メタン,CO,N2) と有機粒子は,リングから4800〜45,000kg/sで内側に流れます.
結論:
- 土星の環と大気間の物質交換が 確認されました
- 環の組成と大気動態に関する新しいデータを提供します.
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