HD 93351 is a Sun-like G-type star (about 0.94 solar masses, 5,408 K), 56.2 light-years from Earth. HD 93351 b is a 3.5-Earth-mass planet, with an orbital period of 2.5 days, at 0.035 AU from its star, on an eccentric orbit (e ≈ 0.55), discovered in 2022 via radial velocity. HD 93351 c is a 13.1-Jupiter-mass companion, with an orbital period of 38.4 years, at 11.2 AU from its star, on an eccentric orbit (e ≈ 0.11), discovered in 2022 via radial velocity. Mutual gravitational tugs between the planets can slowly reshape their orbits, preserving clues to the system's assembly.