ADS 7251
ADS 7251 is a binary star system 6.16 ±0.02 parsecs from the Sun. Both are of nearly equal brightness, but ADS 7251 A, which is 0.06 magnitudes brighter than ADS 7251 B, is a red dwarf of spectral type M0.0. The latter is spectral type K7.0 and slightly further away.ADS 7251 B also known as Gliese 338B has one known super-Earth planet detected by radial velocity.
