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- Proxima Centauri is a red dwarf star with a mass about 12.5% of the Sun's mass. It is too faint to be seen with the unaided eye and has an apparent magnitude of 11.05. The star is classified as a flare star, which means it randomly undergoes sudden increases in brightness due to magnetic activity12. Proxima Centauri has the stellar classification M5.5Ve and a mass of only 0.1221 solar masses3.Learn more:✕This summary was generated using AI based on multiple online sources. To view the original source information, use the "Learn more" links.Proxima Centauri is a red dwarf star with a mass about 12.5% of the Sun's mass (M☉), and average density about 33 times that of the Sun. Because of Proxima Centauri's proximity to Earth, its angular diameter can be measured directly. Its actual diameter is about one-seventh (14%) the diameter of the Sun.en.wikipedia.org/wiki/Proxima_CentauriProxima Centauri is a red dwarf, too faint to be seen with the unaided eye. It has an apparent magnitude of 11.05. It was discovered by the Scottish astronomer Robert Innes in 1915. The star is classified as a flare star, which means that it is a variable star that randomly undergoes sudden increases in brightness as a result of magnetic activity.www.constellation-guide.com/proxima-centauri/Proxima Centauri has the stellar classification M5.5Ve, indicating a main sequence star appearing reddish in colour. The star has a mass of only 0.1221 solar masses (an eighth of the Sun’s mass or 129 times the mass of Jupiter) and a radius of 0.1542 solar radii (about a seventh of the Sun’s radius).www.star-facts.com/proxima-centauri/
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