関連する実験動画
Updated: Dec 25, 2025

11:34
Scattering And Absorption of Light in Planetary Regoliths
Published on: July 1, 2019
10.8K
小惑星 (162173) に人工的に衝突し,重力が支配する状態でクレーターを形成した
1Department of Planetology, Kobe University, Kobe 657-8501, Japan. masahiko.arakawa@penguin.kobe-u.ac.jp.
まとめ
ハヤブサ2ミッションは,小惑星リウグにインパクターを使って人工クレーターを作りました. この実験により,小惑星の重力によるクレーター形成と表面の年齢が明らかになった.
科学分野:
- 小惑星科学
- 惑星地質学
- 宇宙探査
背景:
- 小惑星リウグは,瓦の積み重ね構造のC型小惑星である.
- 小惑星の表面過程を理解することは 惑星科学にとって極めて重要です
研究 の 目的:
- 小惑星の表面での衝突実験の 影響を調査するためです
- 低重力環境でのクレーター形成と 噴出物ダイナミクスを分析する
主な方法:
- ハヤブサ2の小型キャリーオンインパクター (SCI) を使用した人工衝突実験を実施.
- デプロイブルカメラ3 (DCAM3) を使用して衝突事故とエジェクタを記録する.
- 発生したクレーターの形状と 噴出物の振る舞いを分析した
主要な成果:
- 直径10メートル以上の人工クレーターが成功しました.
- 半円形のクレーターに 高い縁と 中央の穴がありました
- エジェクタカーテンの動態は,重力によるクレーター形成を示し,非対称性と不完全な分離を示した.
結論:
- 衝突実験は,リウグーの重力によるクレーター形成の直接的な証拠を提供しました.
- この発見は,リウグの地表年齢と地質史の推定に意味を持つ.
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