ハヤブサ2号は,炭酸性小惑星162173Ryugu-Aの渦巻く頂上形の瓦堆に到着した
S Watanabe1,2, M Hirabayashi3, N Hirata4
1Nagoya University, Nagoya 464-8601, Japan. seicoro@eps.nagoya-u.ac.jp.
まとめ
ハヤブサ2ミッションは,小惑星リウグが"回転する頂部"の形と高孔性を有していることを明らかにし,それは急速な回転によって再構成されたことを示唆しています. 適したサンプル採取場所が赤道上の山脊に特定されました.
科学分野:
- 惑星科学
- 小惑星科学
- 宇宙ミッション分析
背景:
- ハヤブサ2号は2018年に地球近傍の炭化小惑星162173リウグに到達した.
- 小惑星の性質を理解することは 惑星形成の研究に不可欠です
研究 の 目的:
- ハヤブサ2の観測を用いてリウグの形状,質量,地形を分析する.
- 独特の形状と構造の起源を 調べるために
- 検体採取場所を特定する
主な方法:
- ハヤブサ2号からの遠隔観測
- リュウグの形状,質量,表面の特徴を分析した.
- 過去の回転ダイナミクスを推測する.
主要な成果:
- リュウグウは,はっきりとした赤道縁の頂上を回転させる形状を呈している.
- 1.19 ± 0.02 g/cm3の散布密度は,高い内部の多孔性 (> 50%) を示す.
- 表面の岩石と物質の均質性は 急速な回転によって形成されたかもしれない 瓦の積み重ね構造を示唆しています
結論:
- リュウグの現在の形状は 過去の急速な回転と遠心分離によるものです
- 小惑星の内部は 非常に多孔性で 瓦の積み重ねモデルと一致します
- 標本採取に適した場所は赤道上の山脊で特定された.
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