Değil Hakkında Detaylar bilinen Vega 100 mg
The unusually low metallicity of Vega makes it a weak Lambda Boötis yıldız.[78][79] However, the reason for the existence of such chemically peculiar, spectral class A0–F0 stars remains unclear. One possibility is that the chemical peculiarity may be the result of diffusion or mass loss, although stellar models show that this would normally on