Tau Geminorum, Latinized from τ Geminorum, is a star in the northern zodiac constellation of Gemini. It has the apparent visual magnitude of +4.42, making it visible to the naked eye under suitably good seeing conditions. This star is close enough to the Earth that its distance can be measured using the parallax technique, which yields a value of roughly 392abbr=offNaNabbr=off.
It is an evolved giant star of the spectral type K2 III. It has double the mass of the Sun and has expanded to 30 times the Sun's radius. Tau Geminorum is radiating 364 times as much radiation as the Sun from its expanded outer atmosphere at an effective temperature of 4,583 K, giving it the characteristic orange-hued glow of a K-type star. It appears to be rotating slowly with a projected rotational velocity of .
This star has a brown dwarf or Super-Jupiter companion designated Tau Geminorum b, whose mass is at least 20.6 Jupiter masses. It was discovered in 2004 by Mitchell and colleagues, who also discovered Nu Ophiuchi b at the same time. This brown dwarf takes 305days to revolve around Tau Gem. It may also have a stellar companion; a magnitude 11, K0 dwarf at a projected separation of about .