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Updated: Jun 15, 2026

09:33
An Anaerobic Biosensor Assay for the Detection of Mercury and Cadmium
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水星の大気圏でカルシウムを発見した
T A Bida1, R M Killen, T H Morgan
1W.M. Keck Observatory, CARA, Kamuela, Hawaii 96743, USA. tbida@keck.hawaii.edu
Nature
|March 21, 2000
まとめ
科学者は水銀のカルシウムを発見しました.
科学分野:
- 惑星科学は惑星科学である.
- 大気化学 大気化学
背景:
- 水銀の地殻の構成と進化は依然として不確実である.
- 予測された耐火性,無水化合物の構成は,観測された大気中の揮発性物質と対照的です.
- 大気組成は,様々なプロセスを通して表面材料から発生すると考えられています.
研究 の 目的:
- 水星の大気中のカルシウムの存在と起源を調査する.
- 水星の大気組成に寄与するプロセスを理解する.
主な方法:
- 水星の大気中のカルシウムの観測,極の近く.
- 大気柱の密度と気温の分析.
主要な成果:
- 水星の極の近くの大気中のカルシウムを発見.
- 大気中のカルシウムの低い柱密度と高温 (12,000 K) を観測した.
- 局所的な分布は,オーロラゾーンとの潜在的なリンクを示唆しています.
結論:
- 大気中のカルシウムは,オーロラゾーンにおけるイオン誘発のスプッタリングから発生する可能性がある.
- 低量の水星は,水星にカルシウムが欠乏したレゴリットがあることを示唆しています.
- この発見は,水星の表面構成に関する以前の仮定に異議を唱えている.
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