We present photometric and spectroscopic observations of the classical T Tauri stars in the Chamaeleon II dark cloud. The distance to Cha II is 200 +/- 20 pc, based on a plot of extinction versus distance for field stars seen against the cloud. The ages of the pre-main-sequence stars in Cha II range between 10(5) and 10(7) yr. The stellar population of the Cha II cloud consists mostly of low mass stars-at least 17 of the 19 known T Tauri stars in Cha II have masses less than 1M . . The only intermediate mass star in the cloud is IRAS 12496-7650, a highly embedded Herbig Ae star. The mass function of Cha II resembles that of the Lupus complex, and there are a larger fraction of low mass stars in Cha II than there are in the Taurus-Auriga region.