分类:Main Sequence G-type:修订历史

来自星际公民中文百科

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2023年3月8日 (星期三)

  • 当前之前 17:422023年3月8日 (三) 17:42imported>CxJuice 1,192字节 +1,192 创建页面,内容为“{{等待翻译|翻译者=}} A '''G-type main-sequence star''' (Spectral type: G-V), also often, and imprecisely called a '''yellow dwarf''', or '''G star,''' is a main sequence star of spectral type G and luminosity class V. Such a star has about 0.9 to 1.1 solar masses and an effective temperature between about 5,300 and 6,000 K. Like other main-sequence stars, a G-type main-sequence star is converting the element hydrogen to…”

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