太阳系外部的:证据表明有两个不同的储存库
1Department of Earth and Space Sciences, State University of New York at Stony Brook 11794, USA.
Nature
|March 20, 1986
概括
科学家测量了土星,泰坦和天王星中的与甲的比率. 研究结果表明,在太阳系形成之前,有两个原始的储库:一个在气体中,另一个被困在冷固体中.
科学领域:
- 行星科学 行星科学
- 天体化学是天体化学.
- 太阳系的形成太阳系的形成
背景情况:
- 在行星大气层中大量的 (的重同位素) 提供了关于早期太阳系的线索.
- 之前的研究已经表明储库的变化,但缺乏全面的理解.
研究的目的:
- 为了确定土星,泰坦和天王星大气中的CH3D/CH4比率.
- 调查这些比率对太阳系原始储存器的影响.
主要方法:
- 来自土星,泰坦和天王星的大气样本的光谱分析.
- 新获得的CH3D/CH4比率与其他天体的现有数据进行比较.
主要成果:
- 对土星,泰坦和天王星的CH3D/CH4比率的测量成功完成.
- 结合以前的研究结果,结果表明至少存在两个不同的原始储库.
- 这些储库被确定为冷,固体材料中被困的气态和挥发物.
结论:
- 在形成之前,太阳系的已经建立在至少两个单独的储中.
- 一个储由气态中的组成.
- 第二个储包括在低温下保存的挥发物中含有的或从中分离出来的挥发物中含有的,如在冰中.
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