结合142Nd-143Nd的证据表明,火星上存在着长期存在的岩海洋
V Debaille1, A D Brandon, Q Z Yin
1Lunar and Planetary Institute, 3600 Bay Area Boulevard, Houston, Texas 77058, USA. debaille@lpi.usra.edu
Nature
|November 23, 2007
概括
火星 火星 火星 火星 火星
科学领域:
- 行星科学 行星科学
- 地质化学 地质化学
- 宇宙化学 宇宙化学
背景情况:
- 早期的酸盐分化是理解陆地行星演变的关键.
- 行星岩海洋的寿命很少受到限制.
- 由于有限的对流,火星的内部保留了早期分化的记录.
研究的目的:
- 为了解决火星上早期酸盐分化的时间尺度.
- 为了研究火星岩海洋结晶的历史.
主要方法:
- 使用了短寿命的146Sm-142Nd和长寿命的147Sm-143Nd计时器.
- 分析了一套火星Shergottite,Nakhla和Chassigny (SNC) 的石.
主要成果:
- 火星的酸盐分化发生在核心形成后大约1亿年的时间里.
- 数据表明,岩海洋的逐渐结晶.
- 长时间的固化表明火星有一个原始的,厚厚的大气层.
结论:
- 火星早期的酸盐分化历史受到石分析的限制.
- 长期存在的岩海洋表明,由于厚厚的早期大气层,冷却速度有所降低.
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