HD 193373

HD 193373 is a star located in the constellation Capricornus. It is a G-type main-sequence star, similar to our Sun, though slightly larger and more luminous.

HD 193373 is known to host at least one exoplanet, designated HD 193373 b. This exoplanet is a gas giant with a mass greater than Jupiter. Its orbit is relatively close to the star, making it a hot Jupiter.

The star HD 193373 is of interest to astronomers studying exoplanets because it provides insights into the formation and evolution of planetary systems around Sun-like stars. Its characteristics, combined with the properties of its known exoplanet, contribute to a broader understanding of the diversity of planetary systems beyond our own. Further study of this system may reveal additional planets or provide more detailed information about the existing exoplanet's atmosphere and composition. The star's relatively brightness makes it a suitable target for spectroscopic observations.