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ハッブル宇宙望遠鏡から撮影した2パラスの形状と表面の変異
B E Schmidt1, P C Thomas, J M Bauer
1Institute of Geophysics and Planetary Physics, University of California, Los Angeles, CA 90095, USA. britneys@ucla.edu
まとめ
ハッブル望遠鏡の画像は,2 パラスの表面の違いと衝突の特徴を明らかにしています. その密度は,水に富んだ物質から形成されたことを示唆し,それは無傷の原惑星であることを示しています.
科学分野:
- 惑星科学 惑星科学
- 小惑星研究研究.
- 観測天文学 観測天文学
背景:
- 2 Pallasは大きな小惑星で,小惑星帯の2番目に大きな天体です.
- 以前の研究では,Pallasが微分化されていて,水分が有意に含まれている可能性が示唆されていました.
研究 の 目的:
- 小惑星2 Pallasの表面特性と物理的性質を分析する.
- 2 パラスの起源と進化を調査する.
主な方法:
- ハッブル宇宙望遠鏡の高解像度画像の取得と分析.
- 表面特性のフォトメトリックおよびスペクトロフォトメトリック分析.
- 形状モデリングと密度計算は,観測された次元に基づいています.
主要な成果:
- 2 Pallasの表面全体で顕著な色とアルベドの変動が観察されました.
- 291,278,250 kmの半径で決定された円形の形状.
- 計算された密度は2400kg/m3で,水分が豊富な材料と一致しています.
- 紫外線に照らされた暗黒の地形の中で,大きな衝撃の特徴 (直径240km) の特定.
結論:
- 2 Pallasは,完全に分類されていない,無傷の原惑星です.
- 小惑星は,重大な衝突発掘と内部変化を経験しています.
- その構成は,水氷が豊富な地域で形成されたことを示唆しています.
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