V2376 Ori is a cool M-dwarf (about 0.45 solar masses, 5,778 K). V2376 Ori b is a 20.0-Jupiter-mass companion, at 71.0 AU from its star, and an equilibrium temperature near 2,100 K, discovered in 2025 via direct imaging. Direct imaging revealed these planets because they are young, massive, and widely separated from their star, appearing bright in infrared light against the glare. V2376 Ori b orbits far from its host star. The planet's large radius (87.2 Earth radii) indicates a bloated atmosphere heated by intense stellar radiation.