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Cited by 324

The DOI matches its Crossref record; 4 of the 4 references it cites were found in a registry or an index.

Dynamics of Lunar Formation

Canup, Robin M.·2004·Annual Review of Astronomy and Astrophysics

Abstract

▪ Abstract The giant impact theory is the leading hypothesis for the origin of the Moon. This review focuses on dynamical aspects of an impact-induced lunar formation, in particular those areas that have advanced considerably in the past decade, including (a) late-stage terrestrial accretion, (b) giant impact simulations, (c) protolunar disk evolution and lunar accretion, and (d) the origin of the initial lunar inclination. In all, recent developments now provide a reasonably consistent dynamical account of the origin of the Moon through a late giant impact with Earth, and suggest that the impact-generation of satellites is likely to be a common process in late-stage solid planet formation.

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Metadata

Authors
Canup, R. M.
Venue
Annual Review of Astronomy and Astrophysics
Published
2004-09-22
Volume
42
Issue
1
Pages
441-475
ISSN
  • 0066-4146 (ISSN-L)
  • 1545-4282
OpenAlex
W2140944900
Cited by
324
References
4
FWCI
1.15
Type
journal article
Language
en
Open access
closed

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CoChat. (2026). Citation check: Dynamics of Lunar Formation. https://app.cochat.ai/papers/10.1146/annurev.astro.41.082201.113457
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Canup, R. M. (2004). Dynamics of Lunar Formation. Annual Review of Astronomy and Astrophysics. https://doi.org/10.1146/annurev.astro.41.082201.113457

Data sources

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.