プロキシマ・ケンタウリ vs シリウス

Between magnitude −1.44 and +11.01 lies a factor of 95,499 in the light that reaches the eye. Spectroscopically プロキシマ・ケンタウリ resolves as an M-type star in Centaurus and シリウス as an A-type star in Canis Major. シリウス is the remoter of the pair at 8.60 light-years, roughly 2.0 times the 4.23 that separates us from プロキシマ・ケンタウリ.

Property comparison

Property プロキシマ・ケンタウリ シリウス
名称 N/A 9Alp CMa
星座 Centaurus Canis Major
スペクトル型 Class M — M-type (Red) Class A — A-type (White)
見かけの等級 +11.01 -1.44
絶対等級 15.45 1.45
距離 4.2 ly 8.6 ly
質量 N/A N/A
半径 N/A N/A
温度 N/A N/A
光度 N/A N/A

Full data for each star: プロキシマ・ケンタウリ · シリウス

Key differences

Key Differences

  • ◆ Sirius is a brilliant A-type star 8.6 ly away; Proxima Centauri is a faint M-type red dwarf at 4.24 ly.
  • ◆ Proxima Centauri is the closest star to the Sun; Sirius is the closest naked-eye star in its direction.
  • ◆ Sirius is 25.4 times more luminous than the Sun; Proxima Centauri produces only 0.17% of the Sun's light.
  • ◆ Proxima Centauri hosts confirmed exoplanets in the habitable zone; Sirius has no known planets.
  • ◆ Sirius shines at magnitude −1.46; Proxima Centauri at magnitude 11.1 is invisible to the naked eye.
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