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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
月面の反対側から発生する地震的切断波は,アポロ衛星のいくつかのステーションでは検出されない. これは,月の内部が1000~1100kmの深さで,地球のアステノスフィアと似たように,部分的に溶けた状態にある可能性があることを示唆している.
科学分野:
- * 地震学について
- * 惑星科学 (惑星科学)
- * 月面内部の構造
背景:
- * アポロ地震ネットワークは,月の内部構造に関する重要なデータを提供した.
- *地震波の伝播を理解することで,地表下の物質の性質が明らかになる.
研究 の 目的:
- *月面内部の地震特性を調査する.
- *月のマントルが部分的に溶けたかどうかを判断する.
主な方法:
- *地震による直接的なシェア波の到着の分析.
- * アポロ月の地震ネットワークからの地震データの比較.
主要な成果:
- * 月の反対側での出来事のために,特定の地震ステーションでは,直接的なシェア波の到着は観察されなかった.
- *月面内部の深さ1000~1100kmでは,その上に横たわる石層よりも高い地震シーア波の消散を示している.
結論:
- *深さ1000~1100kmの月の内部は,地震性剪定波に対する消耗性が高い可能性が高い.
- * この領域は,地球のアステノスフィアと類似した部分的に溶けた状態に存在している可能性があります.
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