Longitudinal heterogeneity of Phobos’ crater size-frequency distribution: coevolution of resurfacing and orbital dynamics

Abstract Phobos always keeps the same side facing its host planet like Earth’s Moon, making it a key comparative target for studying the coevolution of planet–satellite systems. The heterogeneity of satellite surface evolution under a host planet’s gravity is crucial for understanding the evolution...

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Bibliographic Details
Main Authors: Yuki Uchida, Kosei Toyokawa, Tomohiro Usui, Yudai Suzuki, Haruhisa Tabata
Format: Article
Language:English
Published: SpringerOpen 2025-08-01
Series:Progress in Earth and Planetary Science
Subjects:
Online Access:https://doi.org/10.1186/s40645-025-00741-3
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