19 Canum Venaticorum

19 Canum Venaticorum is a binary star in the constellation Canes Venatici. It is approximately 245 light years from Earth.

The primary component, 19 Canum Venaticorum A, is a white A-type main sequence dwarf with an apparent magnitude of +5.77. Its companion, 19 Canum Venaticorum B, is a tenth magnitude star located only 0.37 arcseconds from the primary.