We examine two scenarios for formation of the planetary nebula K648: a
prompt scenario in which the planetary nebula is ejected and formed i
mmediately after a helium shell flash and a delayed scenario in which
a third dredge-up occurs and the envelope is ejected during the follow
ing interpulse phase. We present models of both scenarios and find tha
t each can produce K648-like systems. We suggest that the prompt scena
rio is more favorable but cannot rule out the delayed scenario.