在小行星24 Themis表面的水冰和有机物质
Humberto Campins1, Kelsey Hargrove, Noemi Pinilla-Alonso
1University of Central Florida, PO Box 162385, Orlando, Florida 32816-2385, USA. campins@physics.ucf.edu
Nature
|April 30, 2010
概括
小行星24Themis显示了普遍存在的表面冰和有机化合物,支持小行星将水送到地球的理论. 这一发现为行星水的起源提供了新的见解.
科学领域:
- 行星科学 行星科学
- 天文学 天文学
- 天体生物学 天体生物学
背景情况:
- 地球的水可能是由月球形成后的小行星提供的.
- 一些小行星中类似彗星的活动表明存在水冰.
- 以前的研究推断,但没有直接测量小行星上的水冰.
研究的目的:
- 为了研究小行星24Themis的组成.
- 确认小行星上存在水冰和有机化合物.
- 了解水的起源和运送到地球.
主要方法:
- 红外光谱学被用来分析小行星24Themis的表面.
- 频谱数据与各种化合物的已知的光谱特征进行了比较.
- 使用独立结果验证了光谱特征的识别.
主要成果:
- 红外光谱显示,小行星24Themis上存在水冰和有机化合物.
- 小行星24 Themis与其他小行星相比,具有独特的光谱特征.
- 广泛的表面冰是意想不到的,因为它的升温率在3.2 AU.
结论:
- 小行星24 Themis 很富有表面冰和有机物质.
- 这些发现支持小行星将水送到地球的假设.
- 地下水库和冲击园艺是观察到的表面冰的合理解释.
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