1 Correction to: Surveys in Geophysics https://doi.org/10.1007/s10712-021-09677-x
In this paper, in Sect. 3.6 concerning Enceladus, Fig. 9 was erroneously used. Instead of the original Fig. 9 shown below, a similar figure by Nimmo et al. (2018) was submitted instead.
Sketch of the likely internal structure of Enceladus derived from gravity, topography and libration observations (see text). The South Polar Terrain (SPT) has a reduced ice shell thickness
In addition, when referencing the results of Beuthe et al (2016), the North and South pole regions were confused. According to their results, the ice shell thickness is approximately 15 km beneath the North pole and 7 km beneath the South pole.
We deeply apologize for using the figure from Nimmo et al. (2018) erroneously and inappropriately, and also for misquoting Beuthe et al. (2016).
References
Beuthe M, Rivoldini A, Trinh A (2016) Enceladus’s and Dione’s floating ice shells supported by minimum stress isostasy. Geophys Res Lett 43(19):10088–10096. https://doi.org/10.1002/2016GL070650
Nimmo F, Barr AC, Behounkova M, McKinnon WB (2018) The thermal and orbital evolution of Enceladus: observational constraints and models. In: Schenk PM, Clark RN, Howett CJA, Verbiscer AJ, Waite JH (eds) Enceladus and the icy moons of Saturn. University of Arizona Press, Tucson, pp 79–94. https://doi.org/10.2458/azu_uapress_9780816537075-ch005
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Breuer, D., Spohn, T., Van Hoolst, T. et al. Correction to: Interiors of Earth-like planets and satellites of the Solar System. Surv Geophys 43, 227–228 (2022). https://doi.org/10.1007/s10712-021-09687-9
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DOI: https://doi.org/10.1007/s10712-021-09687-9