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雾使冥王星的大气层变热, 却解释了它的寒冷温度
Xi Zhang1, Darrell F Strobel2, Hiroshi Imanaka3,4
1Department of Earth and Planetary Sciences, University of California Santa Cruz, Santa Cruz, California 95064, USA.
Nature
|November 17, 2017
概括
而不是气体, 解释了它的寒冷温度. 雾粒子主导着辐射平衡,使得冥王星在中红外波长上更明亮,以供未来的望远镜探测.
科学领域:
- 星球科学
- 大气物理
- 天体物理学
背景情况:
- 冥王星的大气层出乎意料地冷, 违背理论预测.
- 一个未知的冷却机制被怀疑解释低温.
- 水蒸气以前被提议作为冷却剂,但所需的超和水平在热力学上是不可能的.
研究的目的:
- 调查大气雾在冥王星温度调节中的作用.
- 要确定雾粒子是否可以解释观察到的热谱.
- 为了重新评估冥王星的辐射能量平衡.
主要方法:
- 对冥王星大气温度的观测数据进行分析.
- 模拟粒子与气体分子的太阳能加热和热冷却速度.
- 使用和不使用雾影响的辐射导电平衡模型的比较.
主要成果:
- 雾颗粒的太阳加热和热冷却速度明显高于气体分子.
- 雾粒子占据了冥王星大气中的辐射平衡, 高达700公里.
- 在700公里以上,热传导形成同热气氛.
结论:
- 冥王星的大气温度主要由雾粒子调节, 而不是气体分子.
- 在太阳系行星大气层中, 这种以雾气为主导的能量平衡是独一无二的.
- 预计冥王星在中红外波长上会更亮,
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