Secular spin-axis dynamics of exoplanets (Corrigendum)
IMCCE, Observatoire de Paris, PSL Research University, CNRS, Sorbonne Université, LAL, Université de Lille, 75014 Paris, France
e-mail: melaine.saillenfest@obspm.fr
Key words: planets and satellites: dynamical evolution and stability / celestial mechanics / planets and satellites: general / errata, addenda
Some errors have occurred during the production of the original article.
In Sect. 3.3, last but one paragraph, a unit was incorrect in the second sentence. It should read: “Using the average density of the Earth, we obtain a minimum rotation period of about 2.4 h, leading to a maximum precession constant of about 230′′ yr−1. The true value for the Earth is 20′′ yr−1, or 50′′ yr−1 if we include the additional effects of the Moon (Laskar & Robutel 1993).”
In Appendix F, the titles of Tables F.2, F.3 and F.4 have been mistakenly replaced by “Table F.1. continued”. Here, we publish these tables with their correct names. In the text, the citations of “Table F.1” should read “Tables F.1–F.4”.
References
- Laskar, J. 1990, Icarus, 88, 266 [Google Scholar]
- Laskar, J., & Robutel, P. 1993, Nature, 361, 608 [Google Scholar]
© M. Saillenfest et al. 2019
Open Access article, published by EDP Sciences, under the terms of the Creative Commons Attribution License (http://creativecommons.org/licenses/by/4.0), which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.