月面材料の固有温度はケルヴィン90度から350度までである
まとめ
アポロ11号の月のサンプルの特定の熱測定は,温度とともに順調に上昇することを示しています. この発見は,昼と夜の間で大きく変化する月の表面の熱パラメータの理解に影響を与えます.
科学分野:
- 地質物理学 地質物理学とは地質物理学です.
- 惑星科学は惑星科学である.
- マテリアルサイエンス 材料科学
背景:
- 月面のレゴリティの熱的性質を理解することは,表面探査と熱モデリングに不可欠です.
- アポロ11号は,現地分析のためのユニークなサンプルを提供した.
研究 の 目的:
- アポロ11号の月面サンプル (10057と10084) の特異的な熱を測定するために.
- 90Kから350Kまでの比熱の温度依存度を測定する.
- 月面の熱パラメータへの影響を評価する.
主な方法:
- 特定熱を測定するために,アディアバティック熱計が用いられました.
- サンプルには,ベジキュラ状の玄武岩のような岩と月面の土壌が含まれていました.
主要な成果:
- 固有熱は90Kでの約0.06cal/g/Kから350Kでの0.2cal/g/Kまでスムーズに増加した.
- 測定された特異熱値は,分析された月の材料の特徴です.
結論:
- 固有熱データは,月の熱モデルのための重要なパラメータを提供します.
- 月面の計算された熱パラメータ (ガンマ) は,約2の因数で昼間変動を示しています.
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