The DOI matches its Crossref record.
Asteroid Density, Porosity, and Structure
Abstract
New data from observations of asteroid mutural perturbation events, observations of asteroid satellites, and spacecraft encounters have revolutionized our understanding of asteroid bulk density.
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Citations
Cited by
Chaotic capture of Jupiter's Trojan asteroids in the early Solar System
Morbidelli, A., Levison, H. F., Tsiganis, K., & Gomes, R. (2005) · Nature · doi:10.1038/nature03540 · Cited by 939
THE IMPORTANCE OF SECONDARY CRATERING TO AGE CONSTRAINTS ON PLANETARY SURFACES
McEwen, A. S., & Bierhaus, E. B. (2006) · Annual Review of Earth and Planetary Sciences · doi:10.1146/annurev.earth.34.031405.125018 · Cited by 284
Ceres: Evolution and current state
McCord, T. B., & Sotin, C. (2005) · Journal of Geophysical Research: Planets · doi:10.1029/2004je002244 · Cited by 272
Geophysical evolution of the Themis family parent body
Castillo‐Rogez, J. C., & Schmidt, B. E. (2010) · Geophysical Research Letters · doi:10.1029/2009gl042353 · Cited by 47
Metadata
- Authors
- Britt, D. T., Yeomans, D., Housen, K., & Consolmagno, G.
- Venue
- Asteroids III
- Publisher
- University of Arizona Press
- Published
- 2002-12-01
- Pages
- 485-500
- OpenAlex
- W1614250381
- Cited by
- 471
- References
- 0
- FWCI
- 54.23
- Type
- book chapter
- 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.
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How to cite
Cite CoChat for the checks on this page, and the paper for its own findings.
- This page
- CoChat. (2026). Citation check: Asteroid Density, Porosity, and Structure. https://app.cochat.ai/papers/10.2307/j.ctv1v7zdn4.37
- The paper
- Britt, D. T., Yeomans, D., Housen, K., & Consolmagno, G. (2002). Asteroid Density, Porosity, and Structure. Asteroids III. https://doi.org/10.2307/j.ctv1v7zdn4.37
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.
