Spatial Distribution of Ray Craters on Callisto: Implications for Ray Retention and Impactor Sources on Jovian Satellites-Reference-Cited by-同舟云学术

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Spatial Distribution of Ray Craters on Callisto: Implications for Ray Retention and Impactor Sources on Jovian Satellites

Published:2019-07 Issue:7 Volume:124 Page:1717-1727
ISSN:2169-9097
Container-title:Journal of Geophysical Research: Planets
language:en
Short-container-title:J. Geophys. Res. Planets

Author:

Xu Luyuan¹²^ORCID,Hirata Naoyuki³^ORCID,Miyamoto Hideaki⁴⁵

Affiliation:

1. State Key Laboratory of Lunar and Planetary Sciences Macau University of Science and Technology Macau China

2. Graduate School of Frontier Sciences The University of Tokyo Kashiwa Japan

3. Graduate School of Science Kobe University Kobe Japan

4. Department of Systems Innovation, School of Engineering The University of Tokyo Tokyo Japan

5. Planetary Science Institute Tucson AZ USA

Publisher

American Geophysical Union (AGU)

Subject

Space and Planetary Science,Earth and Planetary Sciences (miscellaneous),Geochemistry and Petrology,Geophysics

Link

https://onlinelibrary.wiley.com/doi/pdf/10.1029/2019JE005968

Reference29 articles.

1. Origin of the Ganymede–Callisto dichotomy by impacts during the late heavy bombardment

2. Standard techniques for presentation and analysis of crater size-frequency data

3. Origin and Evolution of the Cometary Reservoirs

4. Galileo views of the geology of Callisto

5. Differential impact cratering of Saturn's satellites by heliocentric impactors

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