まとめ
コンドリート隕石の新たな微細探査分析により,平衡温度が約850°Cの低いことが明らかになった. オリビン-オルトピロキセンの分割は理想的な行動から逸脱し,以前の推定に異議を唱える.
科学分野:
- 地質化学 地質化学
- ミネラロジーは,鉱物学です.
- 惑星科学は惑星科学である.
背景:
- コンドリート隕石は,太陽系の初期状態の洞察力を提供します.
- ミネラル分割の理解は,温度計測定において極めて重要です.
研究 の 目的:
- 併存するピロキセンとオリヴィンにおけるFe(++) とMg(++) の分布係数を計算する.
- 均衡温度を決定し,鉱物分割における理想的な振る舞いを評価するために.
主な方法:
- オリヴィン,オルトピロキセン,およびカルシックピロキセンの共存に関する新しいデータのための電子マイクロプローブ分析を使用しました.
- Fe-Mg交換のための計算された配分係数 (KD).
主要な成果:
- 均衡温度は約850°Cと推定されている.
- オリヴィン-オルトピロキセンのFe-Mg分割で理想的な行動からの偏差が観察されました.
- 以前の研究と比較して,著しく低い均衡温度が決定されました.
結論:
- 850°Cの均衡温度は,これらのコンドリート隕石の改訂された熱史を提供します.
- オリヴィン・オルトピロキセン系における非理想的な混合は,温度計の計算において慎重に考慮する必要がある.
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