Front. Astron. Space Sci. Frontiers in Astronomy and Space Sciences Front. Astron. Space Sci. 2296-987X Frontiers Media S.A. 1385545 10.3389/fspas.2024.1385545 Astronomy and Space Sciences Correction Corrigendum: The characteristic and size–frequency distribution of rocks at the Zhurong landing site, Mars Sun et al. 10.3389/fspas.2024.1385545 Sun Xiukuo 1 Li Shouding 1 2 * Li Juan 2 3 * Wu Yanfang 1 4 Zhang Shuo 5 Zheng Bo 1 2 Zhang Zhaobin 1 2 Xu Tao 1 2 Chen Xinshuo 1 2 Diao Yiming 1 2 1 Key Laboratory of Shale Gas and Geoengineering, Institute of Geology and Geophysics, Chinese Academy of Sciences, Beijing, China 2 College of Earth and Planetary Sciences, University of Chinese Academy of Sciences, Beijing, China 3 Key Laboratory of Earth and Planetary Physics, Institute of Geology and Geophysics, Chinese Academy of Sciences, Beijing, China 4 School of Mathematics, North University of China, Taiyuan, China 5 Aerospace Information Research Institute, Chinese Academy of Sciences, Beijing, China

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 *Correspondence: Shouding Li, lsdlyh@mail.iggcas.ac.cn; Juan Li, juanli@mail.iggcas.ac.cn 29 02 2024 2024 11 1385545 13 02 2024 14 02 2024 Copyright © 2024 Sun, Li, Li, Wu, Zhang, Zheng, Zhang, Xu, Chen and Diao. 2024 Sun, Li, Li, Wu, Zhang, Zheng, Zhang, Xu, Chen and Diao

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 A Corrigendum on The characteristic and size–frequency distribution of rocks at the Zhurong landing site, Mars by Sun X, Li S, Li J, Wu Y, Zhang S, Zheng B, Zhang Z, Xu T, Chen X and Diao Y (2024). Front. Astron. Space Sci. 11:1270079. doi: 10.3389/fspas.2024.1270079 rock size–frequency distribution Zhurong rover excavated depression Mars section-at-acceptance Planetary Science

In the published article, there was an error in the Acknowledgments. The authors wish to add their Acknowledgments of the whole Tianwen-1 team and their data provider. The correct statement appears below:

“The authors thank all the scientists and engineers who were involved in the Tianwen-1 mission, including the China National Space Administration (CNSA), the National Astronomical Observatories of the Chinese Academy of Sciences (NAOC), China Academy of Space Technology (CAST), Beijing Aerospace Control Center (BACC), and other critical institutes. The data set used in this article is processed and produced by “Ground Research and Application System (GRAS) of China’s Lunar and Planetary Exploration Program, provided by CNSA (http://moon.bao.ac.cn).” The TensorFlow implementation of the Cascade R-CNN model is based on Wang et al. (2022), and the authors thank Zhuowei Xiao for his assistance in training the model.”

The authors apologize for this error and state that this does not change the scientific conclusions of the article in any way. The original article has been updated.

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