HD 103774 is a star with a close orbiting planetary companion in the southern constellation of Corvus.
Parallax measurements provide a distance estimate of 184 light years from the Sun.
[2] The stellar classification of HD 103774 is F6 V,[3] indicating this is an F-type main-sequence star that is generating energy through core hydrogen fusion.
The object is orbiting close to the host star at a distance of 0.07 AU (10 Gm) with a period of just 5.9 days and an eccentricity (ovalness) of 0.09.
There is marginal evidence for an infrared excess at a wavelength of 12 μm, indicating the likely grain size.