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Updated: Jun 29, 2026

06:04
Simulation of the Planetary Interior Differentiation Processes in the Laboratory
Published on: November 16, 2013
クレメンタイン・ミッションからの月の形状と内部構造
まとめ
ニュークレメンタインのデータは,月が月であることを明らかにしています.
科学分野:
- 惑星科学 惑星科学
- 地質物理学 地質物理学とは地質物理学です.
- 月面地質学 月面地質学
背景:
- 月の形状と内部構造に関する以前の理解.
- 以前の地形データと重力データの限界.
研究 の 目的:
- 月面の地形と重力の新たな世界観を提示する.
- 月の内部構造と熱の歴史を調査する.
主な方法:
- グローバルな地形学および重力場モデルの分析.
- クレメンタイン宇宙船のミッションから得られたデータ.
主要な成果:
- 16キロメートルの高さを示し,その反対側には極端な地形が描かれています.
- 月の高地では,ほぼ同静的補償を示し,衝突盆地では様々な状態を示します.
- 月面盆地の下で見られた地球上の地殻の薄れ方.
結論:
- 月面の構造と熱の歴史は,これまで考えられていたよりも複雑です.
- アイソスタティック補償は,高地と衝撃盆地間で大きく変化します.
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