HD 108236

HD 108236 is a G-type main-sequence star. Its surface temperature is 5660$$ K. HD 108236 is severely depleted in heavy elements compared to the Sun, with a metallicity Fe/H index of −0.28$$ (52% of the Solar System), and is probably older than the Sun at an age of 6.7$$ billion years.

According to WISE mission data, the star was suspected to be surrounded by a debris disk, but a reanalysis of the data rejected the debris disk hypothesis by 2014. The reason for the false positive was contamination from a nearby infrared source.

Planetary system
In 2020, four planets orbiting HD 108236 were discovered by the transit method, followed by another one in 2021.