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The Measurement of Unsteady Surface Pressure Using a Remote Microphone Probe
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Surveyor v:月の表面の機械的性質について
まとめ
Surveyor Vの月の土壌の機械的性質は,Surveyor IとIIIの場所と類似しています. しかし,静的ベアリング能力は低い場合があり,細い粒と凝結性の証拠があります.
科学分野:
- 地質学 地質学 地質学
- 惑星科学は惑星科学である.
- 土壌力学 土壌力学
背景:
- 月面の土壌特性を理解することは,宇宙船の安全な着陸に不可欠です.
- 以前のミッション (Surveyor IとIII) は,月のレゴリットメカニズムに関する初期データを提供した.
研究 の 目的:
- サーベイヤーVの着陸地における月面土壌の機械的性質を特徴づけるため.
- これらの特性を,以前のSurveyorミッションのデータと比較する.
主な方法:
- 宇宙船の着陸効果を含むSurveyor Vミッションからのデータの分析.
- 侵食実験およびその他の観測データの評価.
主要な成果:
- Surveyor Vの月の土壌の機械的性質は,Surveyor IとIIIのサイトと一致しています.
- サーベイヤーVの静的ベアリング能力は低い場合もあります (2-6 x 10^5ダイネ/cm2).
- 証拠は,月面の土壌における有意な微粒度物質と測定可能な凝結性を示唆しています.
結論:
- Surveyor Vの場所の月面土壌は,他のマリアの着陸場所と一般的な機械的特性を共有しています.
- 細粒子の存在と結束は,土壌の行動と耐力性に影響を与えます.
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