惑星科学. 惑星科学. MESSENGERによる低高度磁場測定は,水星の古代地殻の磁場を明らかにしています
Catherine L Johnson1, Roger J Phillips2, Michael E Purucker3
1Department of Earth, Ocean and Atmospheric Sciences, University of British Columbia, Vancouver, BC, V6T 1Z4, Canada. Planetary Science Institute, Tucson, AZ 85719, USA. cjohnson@eos.ubc.ca.
まとめ
メルキュール メルキュール メルキュール メルキュール
科学分野:
- 惑星科学は惑星科学である.
- 地質物理学 地質物理学とは地質物理学です.
- 宇宙探査 宇宙探査
背景:
- 惑星の磁場は,惑星の内部構造と進化に関する重要な洞察を提供します.
- 水星の磁場の歴史を理解することは,その熱的および地質的過去を解読する鍵です.
研究 の 目的:
- 水星の地殻における残存磁化の存在と年齢を調査する.
- 水星の初期の地球磁場の歴史と強さを制限するために.
主な方法:
- MMercury Surface,Space ENvironment,GEochemistry,およびRanging (MESSENGER) の宇宙船からの軌道ベクトル磁場測定の分析について.
- 低高度での磁場データに基づく地殻磁化年齢の推論.
主要な成果:
- 水星の地殻における残存磁化の検出.
- 磁気化の平均年齢の推定下限は37億年から39億年です.
- 古代の磁場強さは,水星の現在の磁場や地球の磁場に匹敵する.
結論:
- 水星は,コアダイナモプロセスによって生成された初期の地球磁場を持っていた.
- 磁場は,少なくとも39億年前から活動していた可能性が高い.
- フィールド強度の推定値は,MESSENGERのデータと水銀の低地殻鉄含有量と一致しています.
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