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Updated: Oct 4, 2025

11:34
Scattering And Absorption of Light in Planetary Regoliths
Published on: July 1, 2019
10.5K
小惑星 (162173) の小石と砂: 現場観測と地球に戻された粒子
S Tachibana1,2, H Sawada2, R Okazaki3
1UTokyo Organization for Planetary and Space Science-Department of Earth and Planetary Science, The University of Tokyo, Tokyo 113-0033, Japan.
まとめ
ハヤブサ2号は小惑星のサンプルを回収し 砂と小石の形状を明らかにしました この炭素質の小惑星の物質は リオグーと一致する
科学分野:
- 惑星科学
- 天文地質学
- 宇宙ミッション分析
背景:
- ハヤブサ2ミッションは,C型 (炭酸性) 小惑星 (162173) リュウグを標的にした.
- 小惑星の組成と表面の特徴を理解することは,惑星形成の研究に不可欠です.
研究 の 目的:
- 小惑星の表面と地下から採取したサンプルを分析する
- 戻った小惑星の物質の形状を特徴づけるため
- 採取したサンプルの代表性を評価する.
主な方法:
- 2回の陸上作戦の現場撮影
- 人工衝突による噴出物を含む地表と地下の材料の分析.
- 5グラム以上の小石と砂の形状の説明
主要な成果:
- 第2着陸地点で人工衝突クレーターからの噴出物が見られた.
- 表面の小石は形状的な変化 (粗いから滑らか) と多様な形状を示した.
- 返還されたサンプルには 色や形や構造が様々で 留古の観測した素材と一致していました
結論:
- 採取したサンプルは形態学的に多様で,リウグの表面特性を反映しています.
- 返還された材料は,炭酸性小惑星の代表的なサンプルと考えられています.
- ハヤブサ2は小惑星の組成と進化に関する貴重な洞察を提供することに成功した.
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