The Link Between the Local Bubble and Radioisotopic Signatures on Earth
Jenny Feige, Dieter Breitschwerdt, Anton Wallner, Michael M., Schulreich, Norikazu Kinoshita, Michael Paul, Christian Dettbarn, L. Keith, Fifield, Robin Golser, Maki Honda, Ulf Linnemann, Hiroyuki Matsuzaki, Silke, Merchel, Georg Rugel, Peter Steier, Stephen G. Tims

TL;DR
This paper links recent terrestrial radioisotope signatures to nearby supernova activity and the evolution of the Local Bubble, using models to explain the timing and distribution of 60Fe signals on Earth and lunar samples.
Contribution
It introduces analytical and numerical models connecting supernova activity, the Local Bubble's evolution, and terrestrial radioisotope signatures, providing a comprehensive explanation for observed 60Fe signals.
Findings
Extended 60Fe signal in deep-sea archives
Detection of older 60Fe signature in manganese crust
Models explain timing and distribution of radioisotope signatures
Abstract
Traces of 2-3 Myr old 60Fe were recently discovered in a manganese crust and in lunar samples. We have found that this signal is extended in time and is present in globally distributed deep-sea archives. A second 6.5-8.7 Myr old signature was revealed in a manganese crust. The existence of the Local Bubble hints to a recent nearby supernova-activity starting 13 Myr ago. With analytical and numerical models generating the Local Bubble, we explain the younger 60Fe-signature and thus link the evolution of the solar neighborhood to terrestrial anomalies.
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