HD 25912 is a Sun-like G-type star (about 1.08 solar masses, 5,921 K), 49.2 light-years from Earth. HD 25912 b is a 0.12-Jupiter-mass companion, with an orbital period of 41.8 days, at 0.242 AU from its star, discovered in 2022 via radial velocity. HD 25912 c is a 16.5-Jupiter-mass companion, with an orbital period of 72.0 years, at 17.8 AU from its star, on an eccentric orbit (e ≈ 0.05), discovered in 2022 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.