関連する実験動画
Updated: Jul 12, 2026

06:14
Simulating Imaging of Large Scale Radio Arrays on the Lunar Surface
Published on: July 30, 2020
まとめ
赤外線画像は,月の熱異常は一時的なものではなく,安定した特徴であることを明らかにしています. 内部地質学的プロセスに潜在的に関連している,新たに発見された線形異常は,月の地殻の骨折の近くで特定されました.
科学分野:
- 惑星科学は惑星科学である.
- 天文学 (astronomy) 天文学 (astronomy) とは,天文学 (astronomy) とは,天文学 (astronomy) とは,天文学 (astronomy) とは
- 地質物理学 地質物理学とは地質物理学です.
背景:
- 月食は,月の熱的性質を研究するためのユニークな機会を提供します.
- 以前の赤外線観測では,月面の熱異常が確認されていた.
研究 の 目的:
- 2つの月食の赤外線画像を比較して,熱異常の安定性を評価する.
- 新しい熱的特徴を特定し,特徴づけること.
主な方法:
- 1968年4月13日と1964年12月19日の月食による赤外線画像の取得と比較分析.
- 月面マリアで熱異常分布と強度の調査.
主要な成果:
- 月面マリアの観測された熱異常のほとんどは,2つの日食の間に一貫した強さと分布を示し,長期的な安定性を示唆しています.
- 新しい線形熱異常が検出され,月曜日の午後に熱信号が強化されました.
- この新しい異常は,月の地殻の断層線と空間的に相関しているように見える.
結論:
- ほとんどのマリア熱異常の安定性は,それらはおそらく持続的な地質学的または地物理学的特徴であることを示しています.
- 新しく発見された線形異常の特徴は,月の内部プロセスや地下構造に関連する潜在的な起源を示唆しています.
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