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Volcanism in the Solar System

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Abstract

Volcanic activity is the main process for heat-material exchange and circulation for differentiated planets. All terrestrial planets in the Solar System, the Moon, the satellites of giant planets, and the dwarf planets once experienced or are currently experiencing volcanic activities. This paper summarized the volcanism (main volcanic features and their formation) on the Moon, Mars, Venus, and Mercury in the inner Solar System, volcanism and cryovolcanism on satellites (Io, Europa, Enceladus) of giant planets, as well as volcanism on dwarf planets including Cere in the main asteroid belt and Pluto in the Kuiper belt. This work shows volcanism in the Solar System is driven by various factors, forming abundant volcanic landforms. It has significant meanings to compare volcanism happening on different planets using comparative planetology approaches for a better understanding of volcanism, the planetary habitability, and the information contained on the origin and evolution of planets in the Solar System.

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Acknowledgements

We thank the constructive suggestions from Prof. Hejiu HUI and the three anonymous reviewers. This study was supported by the National Natural Science Foundation of China (Grant Nos. 42241111, 41773061, 41773063).

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  1. School of Earth Sciences, China University of Geosciences, Wuhan, 430074, China

    Long Xiao, Jun Huang & Yuqi Qian

  2. School of Atmospheric Sciences, Sun Yat-sen University, Zhuhai, 519082, China

    Zhiyong Xiao

  3. Key Laboratory of Earth and Planetary Physics, Institute of Geology and Geophysics, Chinese Academy of Sciences, Beijing, 100029, China

    Chao Qi

  4. College of Earth and Planetary Sciences, University of Chinese Academy of Sciences, Beijing, 100049, China

    Chao Qi

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Xiao, L., Huang, J., Xiao, Z. et al. Volcanism in the Solar System. Sci. China Earth Sci. 66, 2419–2440 (2023). https://doi.org/10.1007/s11430-022-1085-y

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