The DOI matches its Crossref record; 112 of the 113 references it cites were found in a registry or an index.
THE YARKOVSKY AND YORP EFFECTS: Implications for Asteroid Dynamics
Abstract
The Yarkovsky and YORP (Yarkovsky-O'Keefe-Radzievskii-Paddack) effects are thermal radiation forces and torques that cause small objects to undergo semimajor axis drift and spin vector modifications, respectively, as a function of their spin, orbit, and material properties. These mechanisms help to (a) deliver asteroids (and meteoroids) with diameter D < 40 km from their source locations in the main belt to chaotic resonance zones capable of transporting this material to Earth-crossing orbits; (b) disperse asteroid families, with drifting bodies jumping or becoming trapped in mean-motion and secular resonances within the main belt; (c) modify the rotation rates and obliquities of D < 40 km asteroids; and (d) allow asteroids to enter into spin-orbit resonances, which affect the evolution of their spin vectors and feedback into the Yarkovsky-driven semimajor axis evolution. Accordingly, we suggest that nongravitational forces should now be considered as important as collisions and gravitational perturbations to our overall understanding of asteroid evolution.
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“In this work, relativistic terms and the role of the Yarkovsky and Yarkovsky-O'Keefe-Radzievskii-Paddack (YORP) effects (see e.g. Bottke et al. 2006) have been ignored.”
From Asteroid 2014 OL339: yet another Earth quasi-satellite (2014) · cites this paper as Bottke et al. 2006
Citations
Cites
Radiation forces on small particles in the solar system
Burns, J. A., Lamy, P., & Soter, S. L. (1979) · Icarus · doi:10.1016/0019-1035(79)90050-2 · Cited by 1,471
Hazards due to comets and asteroids
(1995) · Choice Reviews Online · doi:10.5860/choice.33-0281 · Cited by 937
A comet model. I. The acceleration of Comet Encke
Whipple, F. L. (1950) · The Astrophysical Journal · doi:10.1086/145272 · Cited by 885
Catastrophic Disruptions Revisited
Benz, W. (1999) · Icarus · doi:10.1006/icar.1999.6204 · Cited by 851
Debiased Orbital and Absolute Magnitude Distribution of the Near-Earth Objects
Bottke, W. F. (2002) · Icarus · doi:10.1006/icar.2001.6788 · Cited by 740
Self-citationRadiative Spin-up and Spin-down of Small Asteroids
Rubincam, D. P. (2000) · Icarus · doi:10.1006/icar.2000.6485 · Cited by 610
Self-citationThe fossilized size distribution of the main asteroid belt
Bottke, W., Durda, D., Nesvorný, D., Jedicke, R., Morbidelli, A., Vokrouhlický, D., & Levison, H. (2003) · Icarus · doi:10.1016/j.icarus.2004.10.026 · Cited by 552
Self-citationLinking the collisional history of the main asteroid belt to its dynamical excitation and depletion
Bottke, W., Durda, D., Nesvorný, D., Jedicke, R., Morbidelli, A., Vokrouhlický, D., & Levison, H. (2005) · Icarus · doi:10.1016/j.icarus.2005.05.017 · Cited by 464
Self-citationDynamical Lifetimes of Objects Injected into Asteroid Belt Resonances
Gladman, B., Migliorini, F., Morbidelli, A., Zappalà, V., Patrick Michel, B., Cellino, A., Froeschlé, C., Levison, H. F., Bailey, M. E., & Duncan, M. J. (1997) · Science · doi:10.1126/science.277.5323.197 · Cited by 456
Chaotic behavior and the origin of the 31 Kirkwood gap
Wisdom, J. (1983) · Icarus · doi:10.1016/0019-1035(83)90127-6 · Cited by 427
Research works printed but not linked: 20
- Beekman G, 2005, J. Hist. Astron.
- Binzel RP, 1989, Asteroids II, 416
- Bottke WF, 2005, Dynamics of Populations of Planetary Systems, 357
- Dohnanyi JS, 1978, Cosmic Dust, 527
- Holsapple KA, 2005, Lunar Planet. Sci., 36, 2329
- Katasev LA, 1980, Astron. Vestn., 14, 225
- Muinonen K, 1998, Astron. Astrophys., 332, 1087
- Neiman VB, 1965, Earth Univ., 4, 63-64
- Nesvorný D, 2005, Icarus
- O'Keefe JA, 1976, Tektites and Their Origin. Developments in Petrology, No. 4
- Öpik EJ, 1951, Proc. R. Irish Acad., 54, 165
- Paddack SJ. 1973. Rotational bursting of small particles . PhD thesis. Catholic Univ. Washington, DC
- Radzievskii VV, 1952, Astron. Zh., 29, 162
- Radzievskii VV, 1954, Dokl. Akad. Nauk SSSR, 97, 49
- Slabinski VJ, 1977, BAAS, 9, 438
- Vokrouhlický D, 1998, Astron. Astrophys., 335, 1093
- Vokrouhlický D, 1998, Astron. Astrophys., 338, 353
- Vokrouhlický D, 1999, Astron. Astrophys., 344, 362
- Vokrouhlický D, 2005, Icarus
- Vokrouhlický D, 2005, Icarus
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LAURETTA, D. S., Balram-Knutson, S. S., Beshore, E. C., Boynton, W. V., d’Aubigny, C. D., DellaGiustina, D. N., Enos, H., Golish, D. R., Hergenrother, C. W., Howell, E. S., et al. (2017) · Space Science Reviews · doi:10.1007/s11214-017-0405-1 · Cited by 664
Self-citationSolar System evolution from compositional mapping of the asteroid belt
DeMeo, F. E., & Carry, B. (2014) · Nature · doi:10.1038/nature12908 · Cited by 564
MAIN BELT ASTEROIDS WITH WISE /NEOWISE. I. PRELIMINARY ALBEDOS AND DIAMETERS
Masiero, J. R., Mainzer, A. K., Grav, T., Bauer, J. M., Cutri, R. M., Dailey, J., Eisenhardt, P. R. M., McMillan, R. S., Spahr, T. B., Skrutskie, M. F., et al. (2011) · The Astrophysical Journal · doi:10.1088/0004-637x/741/2/68 · Cited by 444
An Archaean heavy bombardment from a destabilized extension of the asteroid belt
Bottke, W. F., Vokrouhlický, D., Minton, D. A., Nesvorný, D., Morbidelli, A., Brasser, R., Simonson, B. M., & Levison, H. F. (2012) · Nature · doi:10.1038/nature10967 · Cited by 392
Self-citationPravec, P., & Harris, A. W. (2007) · Icarus · doi:10.1016/j.icarus.2007.02.023 · Cited by 288
Metadata
- Authors
- Bottke, W. F., Vokrouhlický, D., Rubincam, D. P., & Nesvorný, D.
- Affiliations
- Southwest Research Institute (US)
- Charles University (CZ)
- Goddard Space Flight Center (US)
- Southwest Research Institute, Boulder, Colorado 80302;
- Venue
- Annual Review of Earth and Planetary Sciences
- Publisher
- Annual Reviews
- Published
- 2006-05-01
- Volume
- 34
- Issue
- 1
- Pages
- 157-191
- ISSN
- 0084-6597 (ISSN-L)
- 1545-4495
- OpenAlex
- W2144804653
- Cited by
- 720
- References
- 113
- Citations by year
- 2026: 36 · 2025: 40 · 2024: 47 · 2023: 40 · 2022: 53 · 2021: 37 · 2020: 36 · 2019: 32 · 2018: 39 · 2017: 42 · 2016: 34 · 2015: 52 · 2014: 44 · 2013: 39 · 2012: 23
- FWCI
- 2.11
- Type
- journal article
- Language
- en
- Open access
- closed
- Locations
- Annual Review of Earth and Planetary Sciences (publishedVersion)
- Topics
- Physical Sciences › Earth and Planetary Sciences › Space and Planetary Science › Astro and Planetary Science
- Physical Sciences › Engineering › Aerospace Engineering › Space Satellite Systems and Control
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Stellar, planetary, and galactic studies
- Keywords
- Yarkovsky effect, YORP effect, asteroid dynamics, asteroid families, mean motion resonance, spin-orbit resonance, asteroid rotation, non-gravitational forces, Earth-crossing orbits, main-belt asteroid, meteoroids
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