Discovered in 1918 by German astronomer Max Wolf, whom the star is named after, Wolf 359 is a dim [[red dwarf]] with a [[spectral class]] of M6.5. The star's mass is between 9 and 13 percent of Sol's, and has a diameter of approximately 16 to 19 of Sol's. The luminosity is a mere .002% of our own star, so dim if Wolf 359 replaced our sun, it would appear only 10 times brighter then the moon from our world. Like many [[red dwarf|red dwarfs]], Wolf 359 is a [[flare star]] and can violently flare and brighten on occasion<ref>http://www.solstation.com/stars/wolf359.htm</ref>. | Discovered in 1918 by German astronomer Max Wolf, whom the star is named after, Wolf 359 is a dim [[red dwarf]] with a [[spectral class]] of M6.5. The star's mass is between 9 and 13 percent of Sol's, and has a diameter of approximately 16 to 19 of Sol's. The luminosity is a mere .002% of our own star, so dim if Wolf 359 replaced our sun, it would appear only 10 times brighter then the moon from our world. Like many [[red dwarf|red dwarfs]], Wolf 359 is a [[flare star]] and can violently flare and brighten on occasion<ref>http://www.solstation.com/stars/wolf359.htm</ref>. |