相关实验视频
Updated: Nov 2, 2025

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Scattering And Absorption of Light in Planetary Regoliths
Published on: July 1, 2019
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一个尘埃覆盖着贝特尔盖斯的面
M Montargès1,2, E Cannon3, E Lagadec4
1LESIA, Observatoire de Paris, Université PSL, CNRS, Sorbonne Université, Université de Paris, Meudon, France. miguel.montarges@observatoiredeparis.psl.eu.
Nature
|June 17, 2021
概括
红色超巨星通过未知的机制失去质量. 贝特尔盖斯
科学领域:
- 天文学与天体物理学
- 恒星进化
背景情况:
- 红色超巨星代表大质量恒星 (835太阳质量) 的最后一个进化阶段.
- 这些恒星经历了大量的质量损失, 对于它们的进化和超新星命运至关重要, 但机制仍然不清楚.
- 附近的红色超巨星贝特尔盖斯从2019年到2020年经历了前所未有的暗化事件.
研究的目的:
- 为了调查贝特尔盖兹大暗变的原因.
- 了解红超巨星的质量丧失机制.
主要方法:
- 在大暗变期间对贝特尔盖斯的高角分辨率观测.
- 用光球建模来解释观察到的亮度变化.
主要成果:
- 据观察,贝特尔盖兹的南半球比平时黑暗十倍.
- 一个由光球上局部温度下降形成的尘埃团被认为是原因.
- 亮度变化在几周内演变, 表明光球的快速变化.
结论:
- 由于光球变化而形成的尘埃团造成了大阴暗.
- 红色超巨星的质量损失可能是不均的,由动态光球过程驱动.
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