Qatar-2 is a K-type main-sequence star about 595 light-years away in the constellation of Virgo. The star is much older than Sun, and has a concentration of heavy elements similar to solar abundance. The star features a numerous and long-lived starspots, and belongs to a peculiar variety of inflated K-dwarfs with strong magnetic activity inhibiting internal convection.

In 2011 a transiting superjovian planet Qatar-2b was detected by the Qatar Exoplanet Survey. The planet has a large measured temperature difference between dayside 1,368±32 K and nightside 724±135 K. The planetary orbit is well aligned with the equatorial plane of the star, misalignment angle equal to 4.3°±4.5°. No orbital decay was detected. The color of planetary atmosphere is blue due to Rayleigh scattering of light, and albedo is very low, being below 0.06.

An additional massive companion on wide orbit was suspected in 2011, but search utilizing transit-timing variation method has yielded zero results in 2017.