Proxima Centauri, like many M class red dwarfs, is a [[flare star]] that may brighten suddenly to many times its normal luminosity. Visual evidence of such flare activity occurred from May to August 1995 when several fares were recorded<ref>http://www.csc.villanova.edu/~astronom/obs96/node26.html</ref><ref>http://www.sciencemag.org/cgi/content/abstract/268/5215/1327</ref>. | Proxima Centauri, like many M class red dwarfs, is a [[flare star]] that may brighten suddenly to many times its normal luminosity. Visual evidence of such flare activity occurred from May to August 1995 when several fares were recorded<ref>http://www.csc.villanova.edu/~astronom/obs96/node26.html</ref><ref>http://www.sciencemag.org/cgi/content/abstract/268/5215/1327</ref>. |