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Cited by 340

The DOI matches its Crossref record; 23 of the 23 references it cites were found in a registry or an index.

A Giant Impact Origin of Pluto-Charon

Canup, Robin M.·2005·Science

Abstract

Pluto and its moon, Charon, are the most prominent members of the Kuiper belt, and their existence holds clues to outer solar system formation processes. Here, hydrodynamic simulations are used to demonstrate that the formation of Pluto-Charon by means of a large collision is quite plausible. I show that such an impact probably produced an intact Charon, although it is possible that a disk of material orbited Pluto from which Charon later accumulated. These findings suggest that collisions between 1000-kilometer-class objects occurred in the early inner Kuiper belt.

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Metadata

Authors
Canup, R. M.
Venue
Science
Published
2005-01-28
Volume
307
Issue
5709
Pages
546-550
ISSN
  • 0036-8075 (ISSN-L)
  • 1095-9203
OpenAlex
W2012651603
Cited by
340
References
23
FWCI
10.54
Type
journal article
Language
en
Open access
closed

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CoChat. (2026). Citation check: A Giant Impact Origin of Pluto-Charon. https://app.cochat.ai/papers/10.1126/science.1106818
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Canup, R. M. (2005). A Giant Impact Origin of Pluto-Charon. Science. https://doi.org/10.1126/science.1106818

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Bibliographic data: Semantic Scholar, OpenAlex, Crossref.

Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).

Semantic Scholar’s data is described in: Kinney, R., et al. (2023). The Semantic Scholar Open Data Platform. arXiv:2301.10140.