Abstract
The periodic table provides an intuitive framework for understanding chemical properties. However, its traditional patterns may break down for the heaviest elements occupying the bottom of the chart. The large nuclei of actinides (Z > 88) and superheavy elements (Z ≥ 104) give rise to relativistic effects that are expected to substantially alter their chemical behaviours, potentially indicating that we have reached the end of a predictive periodic table1. Relativistic effects have already been cited for the unusual chemistry of the actinides compared with those of their lanthanide counterparts2. Unfortunately, it is difficult to understand the full impact of relativistic effects, as research on the later actinides and superheavy elements is scarce. Beyond fermium (Z = 100), elements need to be produced and studied one atom at a time, using accelerated ion beams and state-of-the-art experimental approaches. So far, no experiments have been capable of directly identifying produced molecular species. Here ions of actinium (Ac, Z = 89) and nobelium (No, Z = 102) were synthesized through nuclear reactions at the 88-Inch Cyclotron facility at Lawrence Berkeley National Laboratory and then exposed to trace amounts of H2O and N2. The produced molecular species were directly identified by measuring their mass-to-charge ratios using FIONA (For the Identification Of Nuclide A)3. These results mark the first, to our knowledge, direct identification of heavy-element molecular species using an atom-at-a-time technique and highlight the importance of such identifications in future superheavy-element chemistry experiments to deepen understanding of their chemical properties.
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Data availability
The data to support the findings of this study are available on Zenodo (https://zenodo.org/records/14277708)53.
Code availability
The code used to analyse the findings of this study is available on Zenodo (https://zenodo.org/records/14277708)53.
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Acknowledgements
We gratefully acknowledge the operations staff of the 88-Inch Cyclotron. The work of J.L.P., J.M.G., J.A.G. and R.O. was supported in part by the US Department of Energy, Office of Science, Office of Nuclear Physics under contract no. DE-AC02-05CH11231 (LBNL). The work of J.L.P., J.M.G., J.K.G., M.M., Z.S. and D.K.S. was supported by the US Department of Energy, Office of Science, Office of Basic Energy Sciences, Heavy Element Chemistry Program under contract number DE-AC02-05CH11231 (LBNL). The University of Alabama work of D.A.D. and S.S. was supported by the US Department of Energy, Office of Science, Office of Basic Energy Sciences, Heavy Element Chemistry Program through grant no. DE-SC0018921. D.A.D. thanks the Robert Ramsay Fund at the University of Alabama. F.H.G. was supported through a LBNL Laboratory Directed Research and Development programme.
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J.L.P., J.M.G., M.M., J.K.G. and D.A.D. conceived the study. J.L.P., J.M.G., F.H.G., M.M. and R.O. prepared the experiment. J.L.P., J.M.G., F.H.G., J.K.G., J.A.G., M.M., R.O., Z.S. and D.K.S. participated in the experimental measurements. J.L.P. analysed the experimental data. D.A.D. and S.S. performed the electronic structure calculations. J.L.P., J.M.G., D.A.D., J.K.G. and D.K.S. were responsible for the interpretation of the experimental results. J.L.P. wrote the paper. J.L.P., D.A.D. and S.S. prepared materials for the Supplementary Information. All authors reviewed and edited the paper.
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This Supplementary Information file contains the following three sections: S1: Secondary production formation for Ac2+ and No2+ reactions with H2O; S2: Electronic structure calculations; S3: Residual Gas Analyzer Readings. It includes 16 Supplementary Figures, 12 Supplementary Tables, and additional references.
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Pore, J.L., Gates, J.M., Dixon, D.A. et al. Direct identification of Ac and No molecules with an atom-at-a-time technique. Nature 644, 376–380 (2025). https://doi.org/10.1038/s41586-025-09342-y
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DOI: https://doi.org/10.1038/s41586-025-09342-y