相关实验视频
Updated: Jul 25, 2026

11:34
Scattering And Absorption of Light in Planetary Regoliths
Published on: July 1, 2019
证据表明,彗星C/1996 B2 (Hyakutake) 的昏迷中相互作用的气体流和扩展的挥发性源分布
W M Harris1, M R Combi, R K Honeycutt
1Space Astronomy Laboratory, University of Wisconsin, 1150 University Avenue, Madison, WI 53706, USA. wharris@sal.wisc.edu
概括
彗星Hyakutake是一颗彗星.
科学领域:
- 彗星科学是一门彗星科学.
- 天文学 天文学
- 天体物理学 天体物理学
背景情况:
- 彗星C/1996 B2 (Hyakutake) 的图像显示了明显的气体和尘埃分布.
- 在内部昏迷中观察到两个弧形分子共振发射特征.
研究的目的:
- 为了研究彗星Hyakutake的内部昏迷中的特征的形态学.
- 了解冰粒对生产不稳定性的贡献.
主要方法:
- 从彗星Hyakutake接近地球的图像的分析.
- 模型模拟用于解释观测数据.
主要成果:
- 在内部昏迷中观察到气体与尘埃的脱.
- 证据表明,核周围有一个延伸的冰粒区域.
- 带有冰颗粒的尾随凝结解释了更明亮的弧度,贡献了23%的挥发性产量.
结论:
- 一个延伸的冰粒区域显著促进了彗星Hyakutake的挥发性生产.
- 模型模拟支持这种冰冷粒区的存在和活动.
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