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. 2024 Nov 13;635(8038):321–326. doi: 10.1038/s41586-024-08130-4

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© The Author(s) 2024

Open Access This article is licensed under a Creative Commons Attribution 4.0 International License, which permits use, sharing, adaptation, distribution and reproduction in any medium or format, as long as you give appropriate credit to the original author(s) and the source, provide a link to the Creative Commons licence, and indicate if changes were made. The images or other third party material in this article are included in the article’s Creative Commons licence, unless indicated otherwise in a credit line to the material. If material is not included in the article’s Creative Commons licence and your intended use is not permitted by statutory regulation or exceeds the permitted use, you will need to obtain permission directly from the copyright holder. To view a copy of this licence, visit http://creativecommons.org/licenses/by/4.0/.

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Extended Data Fig. 4 — The same probability density functions plotted in Fig. 4 are replicated for the min/best/max values of the galactic evolution parameter K following equation (2) and including the lower limit derived from ¹³⁵Cs/¹³³Cs, which is represented by dashed lines as a reminder that its calculation assumes a different δ (approximately 1 Myr) than that for the other three isotopes (approximately 3 Myr). ESS and CC represent the standard early Solar System (ESS) value from ref. ⁹ and the carbonaceous chondrites (CC) ESS value from ref. ¹⁰, respectively.