サイキーのガンマ線とニュートロンスペクトロメーター
David J Lawrence1, John O Goldsten1, Patrick N Peplowski1
1Johns Hopkins University Applied Physics Laboratory, Laurel, MD USA.
まとめ
ガンマ線と中性子スペクトロメーター (GRNS) は小惑星サイキーを分析する
科学分野:
- 惑星科学
- 天文地質学
- 核天体物理学
背景:
- 小惑星 (16) サイケはユニークなM級小惑星で,潜在的に金属に富んだ惑星の中心である.
- 惑星の形成と分化を理解するには その構成を理解することが重要です
研究 の 目的:
- ガンマ線とニュートロンスペクトロメーター (GRNS) の詳細を NASAのサイキーのミッションに
- サイキーの元素と金属からシリケートの組成を 判断する能力の概要
- サイキーの起源と性質に関する重要なミッションを GRNS データでどのように解決するか説明します.
主な方法:
- 高純度ゲルミウム (HPGe) センサーを搭載したガンマ線スペクトロメーター (GRS) を用いてガンマ線を検出する (60〜9000 keV).
- バックグラウンドの拒絶,高速ニュートロン測定,宇宙線流量モニタリングのための反偶然シールドを使用します.
- 中性子スペクトロメーター (NS) を用いて3Heの比例センサを使用して,熱エネルギーと熱エネルギー範囲の間の中性子を測定する.
主要な成果:
- GRNSは,主要な元素 (Ni,Fe,Si,K,S,Al,Ca) の表面付近の豊富さを測定するために設計されています.
- 装置はサイキーの金属分子を マップする 内部構造を理解するために不可欠だ
- 打ち上げ前のデータと 宇宙での初期性能は 機体の準備が整っていることを確認します
結論:
- GRNSは小惑星"サイケ"の起源を調査する 重要な装置です
- その測定は サイキーの惑星核と その形成条件を直接調べるでしょう
- この文書は,GRNS,そのデータ製品,および運用計画の包括的な概要を提供します.
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