火星パスファインダー着陸機の磁気特性の実験: 予備的な結果
S F Hviid1, M B Madsen, H P Gunnlaugsson
1Oersted Laboratory, Niels Bohr Institute for Astronomy, Physics, and Geophysics, University of Copenhagen, Copenhagen, Denmark.
まとめ
火星の磁気粒子は,火星に存在しています.
科学分野:
- 惑星科学は惑星科学である.
- 地質化学 地質化学
- 大気科学 大気科学
背景:
- 火星の大気粒子には磁気特性がある.
- これらの粒子は主に酸化鉄 (Fe2O3),潜在的にマゲミット (ガンマ-Fe2O3) で構成されています.
研究 の 目的:
- 火星の大気粒子の磁気特性と組成を特徴づけるために.
- これらの磁気粒子の起源と形成経路を推論する.
主な方法:
- 飽和磁化を含む磁性特性の分析.
- 鉄酸化物相 (Fe2O3,ガンマ-Fe2O3) を特定するための鉱物学的検査.
主要な成果:
- 火星の大気粒子には,平均的な飽和磁化が4Aである. m2/kg.
- 粒子は,おそらく鉄酸化物によって凝固された粘土のような積層であり,おそらくマゲミットが構成要素である.
結論:
- マゲミットの存在は,Fe2+イオンが岩底から液体の水に浸出することを示唆しています.
- 粒子は凍結乾燥した地下水の沈殿物から発生したり,チタノ磁石のような玄武岩前駆体から継承される可能性があります.
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