The advances made during the last decade in estimating the time that has elapsed since the original material of the earth became differen tiated into crust, mantle and core are briefly reviewed. The earlier estimates (3,300-3,500 m.y.) based on the isotopic compositions of lead from galenas of known age are now replaced by one of about 4,500 m.y., as a result of the steadily increasing wealth of available data. Patterson and his co-workers have found that the proportions of lead isotopes (to lead-204) in lead from iron meteorites are lower than those in lead from any other known source. Adopting such lead as primeval, Patterson finds that both meteorites and the earth have essentially the same age, 4,550 ± 70 m.y. Using a series of leads ranging in age from the present to over 2,900 m.y. ago, I find 4,500 ±100 m.y. for the time since primary differentiation. Using only Palaeozoic and younger leads, Russell and Allan reach an estimate of 4,300 ±400 m.y. Possible differences between meteorites and the earth in age and primeval-lead composition are discussed, and reasons are given for thinking that the sialic crust seems to be a more likely source of lead ores than the ultrabasic material of the underlying mantle.