The DOI matches its Crossref record; 15 of the 15 references it cites were found in a registry or an index.
Dynamical Lifetimes of Objects Injected into Asteroid Belt Resonances
Abstract
Numerical simulations of particles placed in orbital resonances in the main asteroid belt show that the typical dynamical lifetimes of objects that could become near-Earth asteroids or meteorites are only a few million years, with the majority destroyed by being transferred to Jupiter-crossing orbits or being driven into the sun. Particles that fortuitously migrate to the terrestrial planet region may be pushed to high-inclination orbits by resonances but are still dynamically eliminated on time scales of ∼10 million years. These shorter lifetimes may require a reassessment of our qualitative understanding about near-Earth asteroids and meteorite delivery.
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Citations
Cites
Radiation forces on small particles in the solar system
Burns, J. A., Lamy, P. L., & Soter, S. (1979) · Icarus · doi:10.1016/0019-1035(79)90050-2 · Cited by 1,469
The Long-Term Dynamical Behavior of Short-Period Comets
Levison, H. F., & Duncan, M. J. (1994) · Icarus · doi:10.1006/icar.1994.1039 · Cited by 908
Self-citationThe Exchange of Impact Ejecta Between Terrestrial Planets
Gladman, B. J., Burns, J. A., Duncan, M., Lee, P., & Levison, H. F. (1996) · Science · doi:10.1126/science.271.5254.1387 · Cited by 292
Self-citationThe Dynamical Structure of the Kuiper Belt
Duncan, M. J., Levison, H. F., & Budd, S. M. (1995) · The Astronomical Journal · doi:10.1086/117748 · Cited by 280
Self-citationAsteroids falling into the Sun
Farinella, P., Froeschlé, C., Froeschlé, C., Gonczi, R., Hahn, G. J., Morbidelli, A., & Valsecchi, G. B. (1994) · Nature · doi:10.1038/371314a0 · Cited by 223
Self-citationMeteorites may follow a chaotic route to Earth
Wisdom, J. (1985) · Nature · doi:10.1038/315731a0 · Cited by 177
ASTEROIDAL SOURCE OF ORDINARY CHONDRITES*
Wetherill, G. W. (1985) · Meteoritics · doi:10.1111/j.1945-5100.1985.tb00842.x · Cited by 161
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Chaotic Diffusion and the Origin of Comets from the 2/3 Resonance in the Kuiper Belt
Morbidelli, A. (1997) · Icarus · doi:10.1006/icar.1997.5681 · Cited by 152
Self-citationWhere do the Apollo objects come from?
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Cited by
THE YARKOVSKY AND YORP EFFECTS: Implications for Asteroid Dynamics
Bottke, W. F., Vokrouhlický, D., Rubincam, D. P., & Nesvorný, D. (2006) · Annual Review of Earth and Planetary Sciences · doi:10.1146/annurev.earth.34.031405.125154 · Cited by 720
Solar System evolution from compositional mapping of the asteroid belt
DeMeo, F. E., & Carry, B. (2014) · Nature · doi:10.1038/nature12908 · Cited by 527
Planetary accretion in the inner Solar System
Chambers, J. E. (2004) · Earth and Planetary Science Letters · doi:10.1016/j.epsl.2004.04.031 · Cited by 341
Metadata
- Authors
- Gladman, B. J., Migliorini, F., Morbidelli, A., Zappalà, V., Michel, P., Cellino, A., Froeschlé, C., Levison, H. F., Bailey, M., & Duncan, M.
- Venue
- Science
- Published
- 1997-07-11
- Volume
- 277
- Issue
- 5323
- Pages
- 197-201
- ISSN
- 0036-8075 (ISSN-L)
- 1095-9203
- OpenAlex
- W2055696734
- Cited by
- 455
- References
- 15
- FWCI
- 21.39
- Type
- journal article
- Language
- en
- Open access
- closed
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- Gladman, B. J., Migliorini, F., Morbidelli, A., Zappalà, V., Michel, P., Cellino, A., Froeschlé, C., Levison, H. F., Bailey, M., & Duncan, M. (1997). Dynamical Lifetimes of Objects Injected into Asteroid Belt Resonances. Science. https://doi.org/10.1126/science.277.5323.197
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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.
