The DOI matches its Crossref record; 4 of the 4 references it cites were found in a registry or an index.
Making More Terrestrial Planets
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Citations
Cites
A hybrid symplectic integrator that permits close encounters between massive bodies
Chambers, J. E. (1999) · Monthly Notices of the Royal Astronomical Society · doi:10.1046/j.1365-8711.1999.02379.x · Cited by 1,820
Self-citationSource regions and timescales for the delivery of water to the Earth
Morbidelli, A., Chambers, J., Lunine, J. I., Petit, J. M., Robert, F., Valsecchi, G. B., & Cyr, K. E. (2000) · Meteoritics & Planetary Science · doi:10.1111/j.1945-5100.2000.tb01518.x · Cited by 881 · cited 2×
“There are several hypotheses to explain mass loss from the belt (see for example, Morbidelli et al. 2000 and Chambers and Wetherill 2001), but all rely on the presence of unstable resonances with the giant planets.”
BackgroundSelf-citationMaking the Terrestrial Planets: N-Body Integrations of Planetary Embryos in Three Dimensions
Chambers, J. E., & Wetherill, G. W. (1998) · Icarus · doi:10.1006/icar.1998.6007 · Cited by 583
Self-citationThe chaotic obliquity of the planets
Laskar, J., & Robutel, P. (1993) · Nature · doi:10.1038/361608a0 · Cited by 499 · cited 2×
“However, the current spin axes of the terrestrial planets are unlikely to be primordial (see Lissauer and Kary 1991, Laskar and Robutel 1993 ), so this does not imply that giant impacts, of the kind seen in the simulations, did not occur.”
Background
Cited by
Forming a Moon with an Earth-like composition via a giant impact
Canup, R. M. (2012) · Science · doi:10.1126/science.1226073 · Cited by 656
Zsom, A., Ormel, C. W., Güttler, C., Blum, J., & Dullemond, C. P. (2010) · Astronomy and Astrophysics · doi:10.1051/0004-6361/200912976 · Cited by 587
Terrestrial planet formation with strong dynamical friction
OBRIEN, D., MORBIDELLI, A., & LEVISON, H. (2006) · Icarus · doi:10.1016/j.icarus.2006.04.005 · Cited by 467
Making other earths: dynamical simulations of terrestrial planet formation and water delivery
Raymond, S. N., Quinn, T., & Lunine, J. I. (2004) · Icarus · doi:10.1016/j.icarus.2003.11.019 · Cited by 455
Building the terrestrial planets: Constrained accretion in the inner Solar System
Raymond, S. N., O’Brien, D. P., Morbidelli, A., & Kaib, N. A. (2009) · Icarus · doi:10.1016/j.icarus.2009.05.016 · Cited by 437
Metadata
- Authors
- Chambers, J.
- Venue
- Icarus
- Publisher
- Elsevier BV
- Published
- 2001-08
- Volume
- 152
- Issue
- 2
- Pages
- 205-224
- ISSN
- 0019-1035 (ISSN-L)
- OpenAlex
- W2139170529
- Cited by
- 664
- References
- 4
- FWCI
- 9.37
- Type
- journal article
- Language
- en
- Open access
- closed
About these checks
Registry, retraction, Cites and statistics results are computed, not judged, with one exception: a printed reference that no index lists is read once by a model before it counts as a citation error. Claims are extracted by a model and kept only when their quote appears verbatim in the text; each cited source is then checked, with a model’s help, for whether it says what the claim relies on. Those verdicts can be wrong — read the claim’s quote and the cited source before relying on one.
Statistics and arithmetic are recomputed, not judged.
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How to cite
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- CoChat. (2026). Citation check: Making More Terrestrial Planets. https://app.cochat.ai/papers/10.1006/icar.2001.6639
- The paper
- Chambers, J. (2001). Making More Terrestrial Planets. Icarus. https://doi.org/10.1006/icar.2001.6639
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.