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...
Saved in:
| 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 |
| Tags: |
Add Tag
No Tags, Be the first to tag this record!
|
Similar Items
-
Magnetic field experiment at Phobos and in space around Mars by the Martian Moons eXploration (MMX) mission
by: Ayako Matsuoka, et al.
Published: (2025-08-01) -
Evolutionary History of the Large-Scale Scarp in Jules Verne Crater, Moon
by: Congzhe Wu, et al.
Published: (2025-04-01) -
Crater formation and erosional truncation of Arkhangelskaya kimberlite pipe (Russia)
by: A. V. Bolonin, et al.
Published: (2019-09-01) -
Evolution of Supernova Remnants in a Cloudy Multiphase Interstellar Medium
by: Minghao Guo, et al.
Published: (2025-01-01) -
Toxicology of Nuclear Polyhedrosis Virus, Botanical and Synthetic Pesticides on Mortality Rate of Crocidolomia binotalis (Zeller)
by: Bakhroini Habriantono, et al.
Published: (2023-02-01)