In astronomy, the main sequence is a classification of stars which appear on plots of stellar color versus brightness as a continuous and distinctive... 60 KB (6,813 words) - 07:50, 7 April 2024 |
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 (luminosity class... 12 KB (1,133 words) - 10:07, 8 April 2024 |
Red dwarf (redirect from M-type main sequence) A red dwarf is the smallest kind of star on the main sequence. Red dwarfs are by far the most common type of fusing star in the Milky Way, at least in... 36 KB (4,242 words) - 21:49, 3 May 2024 |
A pre-main-sequence star (also known as a PMS star and PMS object) is a star in the stage when it has not yet reached the main sequence. Earlier in its... 4 KB (481 words) - 21:34, 25 September 2023 |
Star (section Main sequence) cores. Such stars are said to be on the main sequence and are called dwarf stars. Starting at zero-age main sequence, the proportion of helium in a star's... 146 KB (16,321 words) - 04:24, 9 May 2024 |