We have identified three faint new members of the \eta Chamaeleontis cluster .
Spectral types of the new members are estimated to be \sim M5 based on their TiO band strengths and broadband colors .
With an age of 5 - 8 Myr for the cluster , masses of these new members are estimated to be \sim 0.08 M _ { \odot } .
All three display strong Li 6708 Å absorption and H \alpha 
emission features including one with H \alpha emission equivalent width \sim 60 Å along with HeI 6678 & 7605 Å emission features that are characteristics of classical T Tauri stars .