概括
在哈雷彗星中检测到气态水 (H2O).
科学领域:
- 彗星科学是一门彗星科学.
- 天体化学是天体化学.
- 星球科学 星球科学
背景情况:
- 彗星是冰冷的天体,可以提供关于太阳系早期的见解.
- 水是彗星的关键组成部分,对于理解它们的组成和演变至关重要.
研究的目的:
- 在哈雷彗星的昏迷中检测和量化气态水 (H2O).
- 分析彗星水的光谱特性,推断出它的起源和物理条件.
主要方法:
- 使用了NASA-Kuiper空中天文台上的福里埃变换光谱仪.
- 在2.65微米的v(3) 波段中观察到9个H2O的光谱线.
- 分析了光谱线强度,以确定旋转群体和激发条件.
主要成果:
- 在1985年12月22日和24日,在哈雷彗星昏迷中检测到气态中性H2O.
- 测量的水生产速度大约为6 x 10^28分子/秒和1.7 x 10^29分子/秒.
- 确定了2.66±0.13的正正比比,对应于32 K (+5 K, -2 K) 的核旋转温度.
结论:
- 观察到的光谱数据与非热平衡彗星模型一致.
- 由此产生的低核旋转温度表明,水蒸气起源于低温冰.
- 提供了了解彗星组成和早期太阳系条件的关键数据.
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