Three olivine tracks with etching rates above uranium are claimed to be superheavy nuclei near Z=119, and abundance differences between two meteorites are read as evidence for neutron-star merger origin.
Goeppert Mayer,The shell model, Science 145 (1964) 999
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Natural superheavy nuclei in astrophysical data
Three olivine tracks with etching rates above uranium are claimed to be superheavy nuclei near Z=119, and abundance differences between two meteorites are read as evidence for neutron-star merger origin.