HD 5319

HD 5319 is an approximately 400 light-years distant star, the 5319 b is orbiting with a period of 626 days from the exoplanet HD. The star has a spectral type of G5 IV and a mass of 1.6 solar masses.

Exoplanet

The semi-major axis of the exoplanet HD 5319 b measures just 2 astronomical units. The object has a mass of at least 1.9 Jupiter masses (about 600 Earth masses ). It was developed by Robinson et al. discovered using the radial velocity method and published in 2007.