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The discovery of live  60 Fe in a deep-sea crust with proposed interstellar origin followed by evidence for elevated interplanetary  3 He in the same crust raised the question on how to unambiguously identify the true production site of the identified  60 Fe. Here, we show the implementation of the dyadic radionuclide system  60 Fe /  53 Mn to serve as a tool for the identification of surplus interstellar  60 Fe over interplanetary production. The recent updates in experimental  60 Fe and  53 Mn data from iron meteorites as well as in production rate models confirm the validity and robustness of this dyadic system for future applications.

The Dyadic Radionuclide System 60Fe / 53Mn to Distinguish Interstellar from Interplanetary 60Fe

The Dyadic Radionuclide System ⁶⁰Fe / ⁵³Mn to Distinguish Interstellar from Interplanetary ⁶⁰Fe