在火星的Jezero火山口富含的岩石的变化历史,火星
A P Broz1,2, B H N Horgan1, C Bedford1
1Department of Earth, Atmospheric and Planetary Sciences, Purdue University, West Lafayette, IN USA.
概括
富含粘土的古代火星岩石暗示了长时间的水变化. 分析表明形成是通过强烈的气候变化,类似于地球最潮湿的时期,而不是热水活动.
科学领域:
- 地质地质地质地质地质地
- 行星科学 行星科学
- 矿物学是什么?矿物学是什么?
背景情况:
- 火星上富含的粘土矿物质表明过去的液态水变化.
- 这些火星粘土的形成机制仍然不确定.
- 耐力探测器发现富含的浮动岩石,含有高酸盐的痕迹.
研究的目的:
- 研究火星上古老的高利尼特带地形的形成.
- 将火星浮岩与地球上的类似物进行比较,以了解它们的起源.
- 确定火星粘土是否通过热水变化或化学气候变化形成.
主要方法:
- 使用了来自Perseverance火星车的SuperCam和Mastcam-Z仪器数据.
- 分析了火星浮岩的化学和反射光谱.
- 将火星数据与以地球为基础的古和水热高沉积物进行了比较.
主要成果:
- 火星的浮岩岩石显示和的缩与铁和耗尽.
- 这些化学特征与陆地水热沉积物不同.
- 组成非常类似于地球古岩层在大量降雨下形成的漂白的地平线.
结论:
- 分析的火星岩石很可能是通过强烈的化学气候变化而形成的,而不是水热变化.
- 这些发现表明,火星在其过去经历了显著的潮湿间隔.
- 这些岩石提供了火星过去温室气候的证据.
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