在火星尘埃中的碳酸盐矿物质的光谱识别
Joshua L Bandfield1, Timothy D Glotch, Philip R Christensen
1Department of Geological Sciences, Arizona State University, Tempe, AZ 85287-6305, USA. joshband@asu.edu
概括
火星表面的尘埃中含有少量的石碳酸盐矿物质. 这些碳酸盐可能会隔离出大量的二氧化碳,这表明火星上过去的大气层更厚.
科学领域:
- 行星科学 行星科学
- 地质化学 地质化学
背景情况:
- 火星拥有一个薄薄的大气层,主要是二氧化碳.
- 了解过去的火星大气组成对于评估可居住性至关重要.
- 表面矿物学为行星进化提供了线索.
研究的目的:
- 为了识别和量化火星表面的碳酸盐矿物.
- 评估这些碳酸盐在大气二氧化碳捕获中的作用.
- 为了推断火星上过去的大气状况.
主要方法:
- 来自火星表面的热红外光谱的分析.
- 识别矿物学特征,表明碳酸盐.
- 在火星尘埃中碳酸盐度的量化.
主要成果:
- 检测碳酸盐的重量度为2-5%,主要是石 (MgCO3).
- 这些碳酸盐在火星尘埃中的广泛分布.
- 没有发现缩碳酸盐沉积物的证据.
结论:
- 火星表面的尘埃中含有大量的石,作为二氧化碳沉降器.
- 这些广泛分布的碳酸盐表明,过去火星大气中含有几条CO2的二氧化碳.
- 碳酸盐封存在调节火星古代大气层方面发挥了关键作用.
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