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. 2021 Jun 24;11:13212. doi: 10.1038/s41598-021-92130-1

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© The Author(s) 2021

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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Surface temperature ranges of several Solar System bodies. The light cyan window encloses the values of volume expansion discussed in this work; orange bars show surface temperature range of several Solar System bodies that match the range discussed in this work; black circles indicate the evolution of volume as a function of temperature for olivine Mg_1.84Fe_0.16SiO₄ here investigated.