HD 167042

HD 167042 is an approximately 164 light years from Earth distant giant star of spectral type K1 in the constellation Draco. It has an apparent magnitude of 6.0 mag. The star is surrounded by an exoplanet HD 167042 b with the name.

Exoplanet

HD 167042 b is an exoplanet, orbiting the central star with a period of slightly more than 400 days. The exoplanet with a minimum mass of about 1.6 Jupiter masses, an eccentricity of around 0.03 and a semimajor axis of about 1.3 astronomical units. He was discovered using the radial velocity method.