Barnard's Star

Barnard’s Star is a very low-mass red dwarf star about six light-years away from Earth in the constellation of Ophiuchus, the Snake-holder. Barnard’s Star is the fourth-closest known individual star to the Sun, after the three components of the Alpha Centauri system, and the closest star in the Northern Hemisphere. Despite its proximity, Barnard’s Star, at a dim apparent magnitude of about nine, is not visible with the unaided eye; however, it is much brighter in the infrared than it is in visible light.

Barnard’s Star has been the subject of much study, and it has probably received more attention from astronomers than any other class M dwarf star due to its proximity and favorable location for observation near the celestial equator. Historically, research on Barnard’s Star has focused on measuring its stellar characteristics, its astrometry, and also refining the limits of possible extrasolar planets. Although Barnard’s Star is an ancient star, some observations suggest that it still experiences star flare events.

Once we reached Barnard’s Star during the Interstellar Space Era, we found it particularly uninteresting as it has one Iron Planet and a series of iron and icy asteroids of little value.

Barnard's Star

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