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Scattering And Absorption of Light in Planetary Regoliths
Published on: July 1, 2019
在小行星表面检测冰和有机物质
Andrew S Rivkin1, Joshua P Emery
1Johns Hopkins University Applied Physics Laboratory, Laurel, Maryland 20723, USA. andy.rivkin@jhuapl.edu
Nature
|April 30, 2010
概括
光谱分析检测到小行星24Themis上的水冰和有机物质,这表明这些化合物在小行星和主带彗星上很常见.
科学领域:
- 天文学和行星科学 天文学和行星科学
- 天体生物学 天体生物学
- 地质化学 地质化学
背景情况:
- 最近对主带彗星 (MBC) 的发现已经模糊了彗星和小行星之间的区别.
- 以前的研究没有在小行星表面检测到冰或有机物质.
研究的目的:
- 为了调查小行星24 Themis的组成,以确定存在水冰和有机物质.
- 评估这些发现对了解MBCs的性质和小行星带中挥发性物质的分布的影响.
主要方法:
- 使用光谱分析检测特定分子特征的存在.
- 获得了对光谱检测结果的独立确认.
主要成果:
- 水冰和有机物质在小行星24Themis上被光谱检测到.
- 这些发现得到了独立的证实,加强了它们的有效性.
- 小行星24Themis与已知的MBCs有动态联系.
结论:
- 在小行星24Themis上存在水冰和有机物质,为它们在MBC上存在提供了强有力的证据.
- 水冰在小行星上可能比以前假设的更为普遍.
- 小行星内部可能会在比预期的更小的日中心距离上藏大量的水冰.
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