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Recently, 60Fe was found in the Earth crust formed in a nearby recentsupernova (SN). If the distance to the SN and mass of the progenitor of that SNwas known, then one could constrain SN models. Knowing the positions, propermotions, and distances of dozens of young nearby neutron stars, we candetermine their past flight paths and possible kinematic origin. Once the birthplace of a neutron star in a SN is found, we would have determined the distanceof the SN and the mass of the SN progenitor star.

On identifying the neutron star that was born in the supernova that placed 60Fe onto the Earth