The morphologic and morphometric characteristics of craters on Ceres and implications for the crust
Author:
Funder
National Aeronautics and Space Administration
Publisher
Elsevier BV
Subject
Space and Planetary Science,Astronomy and Astrophysics
Reference106 articles.
1. Central pit craters on Ganymede;Alzate;Icarus,2011
2. Distribution of phyllosilicates on the surface of Ceres;Ammannito;Science,2016
3. Impact cratering on slopes;Aschauer;Icarus,2017
4. Emplacement of Martian rampart crater deposits;Baloga;JGR,2005
5. Martian subsurface volatile concentrations as a function of time: clues from layered ejecta craters;Barlow;Geophys. Res. Lett.,2004
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1. The inevitability of large shallow craters on Callisto and Ganymede: Implications for crater depth-diameter trends;Icarus;2024-01
2. What Is a Polygonal Impact Crater? A Proposed Framework Toward Quantifying Crater Shapes;Earth and Space Science;2023-07
3. Quantifying the Ejecta Thickness From Large Complex Craters on (1) Ceres;Journal of Geophysical Research: Planets;2023-06
4. Spherical multi-lacunarity reveals possible equatorial-polar differences in crater densities on the dwarf planet Ceres;Icarus;2022-09
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