HD 7199 is a Sun-like G-type star (about 0.77 solar masses, 5,371 K, 0.97 solar radii), 36.2 light-years from Earth. HD 7199 b is a 0.27-Jupiter-mass companion, with an orbital period of 1.68 years, at 1.360 AU from its star, on an eccentric orbit (e ≈ 0.19), discovered in 2011 via radial velocity. The planet betrayed itself through the star's reflex motion — a technique that first revealed worlds around Sun-like stars in the 1990s and remains a workhorse of exoplanet discovery. The planet's marked eccentricity suggests past scattering events or perturbations from unseen companions.