関連する実験動画
Updated: May 28, 2026

11:34
Scattering And Absorption of Light in Planetary Regoliths
Published on: July 1, 2019
小惑星21 Lutetiaの画像:太陽系の初期から残った小惑星
1Max-Planck-Institut für Sonnensystemforschung, Max-Planck-Strasse 2, 37191 Katlenburg-Lindau, Germany. sierks@mps.mpg.de
まとめ
小惑星21 Lutetiaは,複雑な地質学と高密度を示しており,原始小惑星であることを示唆しています. この発見は,小惑星の断片や瓦の山である可能性が高い小さな小惑星と対照的です.
科学分野:
- 惑星科学 惑星科学
- 小惑星研究研究.
- 地質学 地質学 地質学
背景:
- 以前のミッションでは,より小さな小惑星は,しばしば断片化されているか,瓦の山であることを明らかにしました.
- 小惑星21 Lutetiaの性質は,より小さな天体と比較して,理解されていなかった.
研究 の 目的:
- 小惑星21 Lutetia.の地質学的特徴と密度を調査するために.
- 21 Lutetiaが小惑星のクラスと比較して小惑星のクラスが異なるかどうかを判断する.
主な方法:
- ローゼッタ宇宙船の光学,光譜,赤外線遠隔画像システム (OSIRIS) カメラからの画像の分析.
主要な成果:
- 21 ルテシアは,北極圏の厚いレゴリット層と滑り込みを含む複雑な地質を呈しています.
- 測定された密度は3.4 ± 0.3g/cm3で,小惑星で記録された最も高い密度です.
- 表面の特徴は,古代の年齢を示唆しています.
結論:
- 複雑な地質学,古代の表面,そして高い密度は,21 ルテシアが原始小惑星であることを強く示唆しています.
- ルテシアの特徴は,以前に研究された小さな,断片化された小惑星と異なる.
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