In a deep ocean ferromanganese crust an excess of Fe-60 radioactivity was m
easured by means of high sensitivity accelerator mass spectrometry. The enh
anced concentrations measured in the first two of three layers (correspondi
ng to a time span of 0-2.8 Myr and 3.7-5.9 Myr, respectively) suggest the d
eposition of supernova produced Fe-60 on earth. There is even a weak indica
tion that the flux into the crust was higher about 5 Myr ago.