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メインベルトのS-コンプレックス小惑星の年齢と色の関係
Robert Jedicke1, David Nesvorný, Robert Whiteley
1Institute for Astronomy, University of Hawaii, Honolulu, Hawaii 96822, USA. jedicke@ifa.hawaii.edu
Nature
|May 21, 2004
まとめ
宇宙の気象は小惑星の表面を変化させ,隕石のスペクトルが母体とは異なる理由を説明します. この研究は,S複合の小惑星の宇宙気象化の速度を定量化し,それらを普通のコンドライトと結びつけています.
科学分野:
- 惑星科学は惑星科学である.
- 天文学 (astronomy) 天文学 (astronomy) とは,天文学 (astronomy) とは,天文学 (astronomy) とは,天文学 (astronomy) とは
- 地質学 地質学 地質学
背景:
- 小惑星の衝突は,隕石になる断片を放出します.
- 普通のコンドライト (OC) 隕石のスペクトルは,S複合小惑星と一致しません.
- 宇宙の気象は,スペクトル差異の説明として提案されている.
研究 の 目的:
- S-コンプレックス小惑星の宇宙気象の速度を定量化します.
- S-コンプレックス小惑星とOC隕石の遺伝的関係を調査する.
主な方法:
- 小惑星ファミリーの年齢と色との関係を分析した.
- 年齢・色別データを若年層に推計した.
主要な成果:
- S-コンプレックス小惑星の宇宙気象の速度を測定しました.
- 推定された年齢と色の関係は,新鮮なOC隕石サンプルの色と一致しました.
結論:
- 強力な証拠は,S複合の小惑星とOC隕石の間の遺伝的リンクを支持しています.
- 宇宙の気象は,小惑星の表面を変更し,隕石の起源を説明する重要なプロセスです.
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