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Planetary geodynamics and age constraints on circumstellar habitable zones around main sequence stars – CORRIGENDUM

Published online by Cambridge University Press:  12 March 2024

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Abstract

Type
Corrigendum
Creative Commons
Creative Common License - CCCreative Common License - BY
This is an Open Access article, distributed under the terms of the Creative Commons Attribution licence (https://creativecommons.org/licenses/by/4.0/), which permits unrestricted re-use, distribution, and reproduction in any medium, provided the original work is properly cited.
Copyright
Copyright © The Author(s), 2024. Published by Cambridge University Press

Upon publication of Mello F de S, Friaça ACS (Reference Mello and Friaça2023) the image presented for 6d has its values mistakenly normalized to the initial value for a 1.0 Earth-mass planet, where it shouldn't have been normalized.

The incorrect image is presented as below

This should have been as per the correct image below:

Due to this where the original, incorrect, image was cited on page 24 as “The behaviour in ocean depth is a reflex of the above, with low-mass planets being able to create deep ocean basins and deep oceans (Fig. 6(d)).” This should instead have read “The behaviour in ocean depth is a reflex of the above combined with our choice of scaling planetary water content with planetary mass (Fig. 6(d)).”

References

Mello, F de S, Friaça, ACS. Planetary geodynamics and age constraints on circumstellar habitable zones around main sequence stars. International Journal of Astrobiology. 2023;22(4):272316. doi:10.1017/S1473550423000083CrossRefGoogle Scholar