HR 830

HR 830, also known as VZ Arietis, is an Alpha² Canum Venaticorum variable star in the constellation Aries. Varying between magnitudes 5.82 and 5.89, the star can be easily seen with the naked eye in dark, unpolluted areas. Located approximately 122 parsecs (400 ly) distant and with a spectral type of A0V, the star is a blue-white star currently fusing hydrogen into helium in its core. The star was formerly known as 16 Trianguli, but as the star is no longer in the constellation Triangulum, this designation has fallen out of use.