在一个黑暗的云层中以分子形式的低微量
S Maret1, E A Bergin, C J Lada
1Department of Astronomy, University of Michigan, 500 Church Street, Ann Arbor, Michigan 48109-1042, USA. smaret@umich.edu
Nature
|July 28, 2006
概括
大多数星际是原子的,而不是分子 (N2). 这解释了彗星中的低N2和石和尘埃中的异常,挑战了关于宇宙的先前假设.
科学领域:
- 太空化学 太空化学
- 天体化学是天体化学.
- 行星科学 行星科学
背景情况:
- 在宇宙中是丰富的,但它的分子形式 (N2) 很难在星际介质中检测到.
- 与太阳值相比,彗星显示了较低的N2丰度和元素缺乏.
- 石和星际尘埃表现出显著的同位素异常.
研究的目的:
- 为了确定冷暗分子云中的分子 (N2) 的丰度.
- 在星际介质中研究 (原子与分子) 的相位.
- 解释彗星,石和尘埃中观察到的耗和同位素异常.
主要方法:
- 使用N2H+作为分子 (N2) 丰度的标记物.
- 分析了来自冷暗分子云的数据.
主要成果:
- 发现冷暗云中的气相中的大部分是原子的,而不是分子 (N2).
- 观察到N2的丰度明显低于之前的假设.
- 推断出原子主导这些云中的气相.
结论:
- 彗星中较低的N2丰度很可能是由于它们的母暗云中分子含量较低.
- 彗星中的元素缺乏可能与低于预期的原子氧气丰度有关.
- 云层中分子的稀缺性解释了石和星际尘埃中的同位素异常,通过增强原子分离.
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