Pi Chamaeleontis is a binary star system located in the southern circumpolar constellation of Chamaeleon. Its name is a Bayer designation that is Latinized from π Chamaeleontis, and abbreviated Pi Cha or π Cha. This system is dimly visible to the naked eye as a point of light with an apparent visual magnitude of 5.64. Parallax measurements put the system approximately 144 light-years (44.2 pc) away. It is drifting closer with a radial velocity of −10 km/s. The Hipparcos satellite mission derived a 223 d orbit on the basis of its motion caused by an unseen companion. The visible component is an A-type subgiant or F-type giant star with an effective temperature of about 6,900 K. It has an absolute magnitude of 2.56, a mass of 1.52 M☉, and a radius of 2.2 R☉. It is roughly 1.8 billion years old.
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