火星表面の古気温は,隕石の熱クロノロジーから得られたものです
David L Shuster1, Benjamin P Weiss
1Division of Geological and Planetary Sciences, California Institute of Technology, 100-23, Pasadena, CA 91125, USA.
まとめ
火星表面の気温は,数十億年もの間冷たいままです. 火星の隕石の新たな分析によると,気温はめったに0°Cを超えなかったことが判明し,古代の火星は一貫して寒かったことを示唆している.
科学分野:
- 惑星科学は惑星科学である.
- 地質学 地質学 地質学
- サーモロジック・サーモロジック
背景:
- 過去の火星の表面温度の理解は,惑星の居住可能性の評価に不可欠です.
- 以前の研究では,火星の長期的な熱進化に関する限られたデータしか得られなかった.
研究 の 目的:
- 火星の隕石,特にナクリットとALH84001.1の熱史を再構築する.
- 地質的な時間尺度で火星の表面近くの過去の温度条件を推論する.
主な方法:
- 熱クロノロジー技術を活用して隕石のサンプルを分析した.
- 総合的な分析のために,公開された貴重ガスと石油学的データを組み込みました.
主要な成果:
- ナクリット隕石は,形成以来,350°C以上の加熱の証拠はない.
- 計算によると,火星の近地温度は,過去40億年間,ほぼ0°C以下にとどまっている.
結論:
- 火星の気候は,その歴史の大部分を通して,主に寒かった.
- これらの発見は,火星上の過去の生命の探求に重大な意味を持つ.
関連する概念動画
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