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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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大 暗闇 の 間,ベテルゲウス を 覆っ て いる 塵 の 幕
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
まとめ
赤の超巨大惑星は 解明されていないメカニズムで 質量を失っています ベテルゲウス
科学分野:
- 天文学と天体物理学
- スター進化
背景:
- 赤の超巨大星は,巨大な星 (835太陽の質量) の最終的な進化段階を表しています.
- これらの恒星は進化と超新星運命を決定する 重要な質量損失を経験しますが そのメカニズムは不明です
- 近くの赤い超巨大惑星であるベテルゲウスは,2019~2020年に前例のない暗くなった.
研究 の 目的:
- ベテルギュゼの大暗闇の原因を調査する
- 赤い超巨大惑星の 質量減少メカニズムを理解するために
主な方法:
- グレートディミング中のベテルゲウスの高角解像度観測.
- 観測された明るさの変動を解釈するための光球モデル化.
主要な成果:
- ベテルゲーゼ の 南半球 は 通常 の 10 倍 に 暗く 観測 さ れ まし た.
- 光球の局所的な温度低下から形成された 塵の塊が原因とされています
- 明るさの変動は数週間で進化し,光球の急速な変化を示しています.
結論:
- フォトスフィアの変化によって形成された 塵の塊によって引き起こされました
- 赤の超巨大星の質量損失は不均一であり,ダイナミックな光球プロセスによって引き起こされる可能性が高い.
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