HD 8357

HD 8357 is a G1V-type star located approximately 136 light-years away in the constellation Hydrus. It is a main-sequence star, meaning it is currently fusing hydrogen into helium in its core. HD 8357 is similar to our Sun in terms of mass and temperature, although it is slightly more massive and luminous.

The star is also notable for its relatively high metallicity, indicating a greater abundance of elements heavier than hydrogen and helium compared to the Sun. This higher metallicity may be linked to the presence of planets orbiting the star.

As of the current date, no planets have been confirmed to orbit HD 8357. However, radial velocity measurements and other observational techniques are constantly being employed to search for potential exoplanets around this and other nearby stars. The star is a target of interest for exoplanet surveys due to its solar-like properties.