ハヤブサ2からの小惑星162173リウグの表面組成 近赤外線スペクトロスコーピー
K Kitazato1, R E Milliken2, T Iwata3,4
1The University of Aizu, Fukushima, Japan. kitazato@u-aizu.ac.jp.
まとめ
地球近傍小惑星リウグ
科学分野:
- 惑星科学
- スペクトロスコーピー
- 天文地質学
背景:
- 小惑星162173リウグは,ハヤブサ2ミッションのターゲットです.
- リュウグは原始的な炭鉱物と考えられています
研究 の 目的:
- リュウグの表面構成を 反射スペクトルで分析する
- ハヤブサ2が返したサンプルの地質学的な背景を提供するためです.
主な方法:
- ハヤブサ2の近赤外線スペクトロメーター (NIRS3) を使用して反射スペクトルを取得.
- スペクトル特性の分析,特に吸収帯.
主要な成果:
- 水素 (OH) 含有鉱物を示す,至る所に存在する2.72マイクロメートルの吸収特性は,Ryuguの表面で検出されました.
- OHの特徴の強さと低いアルベドは,変形した炭酸コンドライト隕石に似ています.
- OH帯の位置の最小の変動は,組成の均一性を示唆する.
結論:
- の表面はヒドロキシル含有鉱物で満ちている.
- 小惑星は,水分的に変化した親体の断片から形成された瓦の堆積物です.
- Ryuguの構成は熱またはショックで変形した炭酸性コンドライトと一致します.
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