Abstract
26Al ages of 17 chondrules from the least equilibrated CO3.0 Yamato-81020 were analyzed. The chondrule formation ages show 1.3 to 2.4 Myr for ferromagnesian chondrules and 2.9 Myr for Al-rich chondrules after CAIs formations, assuming 26Al was homogeneously distributed in the early solar nebula. The forming period of ferromagnesian chondrules in carbonaceous chondrites (CC) clearly consists with those in ordinary chondrites (OC), 1.0-2.5 Myr after CAIs. Thus, ferromagnesian chondrules in CC formed contemporaneously with ferromagnesian chondrules in OC.