R136a1
出典: フリー百科事典『ウィキペディア（Wikipedia）』 (2023/04/02 02:20 UTC 版)
RMC 136a1（通称 R136a1）は、タランチュラ星雲にある散開星団のNGC 2070の中心にある超星団「R136」に属するウォルフ・ライエ星に分類される恒星である。銀河系の近隣にある銀河として知られている大マゼラン雲の中に位置しており、地球からは約49,970パーセク（約163,000光年）の距離にある。既知の恒星の中で最も大きな質量[8][9]と光度を持ち、質量は315太陽質量、光度は約8,700,000太陽光度と推定されており、最も表面温度が高い恒星の1つでもある。
注釈
出典
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[続きの解説]
「R136a1」の続きの解説一覧
- 1 R136a1とは
- 2 R136a1の概要
- 3 発見
- 4 可視性
- 5 進化
- 6 脚注
固有名詞の分類
- R136a1のページへのリンク
