Dynamical Evolution of Main Belt Meteoroids: Numerical Simulations Incorporating Planetary Perturbations and Yarkovsky Thermal Forces

By William Bottke, D. Rubincam, J. Burns. 2000

142 citations recorded by the source corpus.

View Paper: https://www.semanticscholar.org/paper/c6478df46b63a6a70ac33ef4841a99c7c32622bc

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In Astronomy and Astrophysics

Citations in the corpus

Yarkovsky Effect on Small Near-Earth Asteroids: Mathematical Formulation and Examples (2000, background): “In general, the seasonal drift is always smaller than the diurnal drift, which is again in good agreement with the previous results of Farinella et al. (1998) or Bottke et al. (2000) .”
Effects of thermal radiation on the dynamics of binary NEAs (2004, unknown): “space (Farinella et al., 1998; Bottke et al., 2000), and the dy-”
The orbital distribution of Near-Earth Objects inside Earth's orbit (2012, background): “…drift is believed to cause main-belt asteroids to migrate to either larger or smaller a, allowing them to drift into the supply resonances (Farinella and Vokrouhlický, 1999; Bottke et al., 2000b), but again its effect on the large-scale NEO orbital distribution with q < 1.3 AU should be minor.”
Mineralogies and source regions of near-Earth asteroids (2013, background): “One of the most probable mechanisms for delivering meteorites to Earth is the Yarkovsky effect (Bottke et al., 2002a, 2000; Rubincam 1995; Hartmann et al., 1999), which causes bodies to drift in orbital semi-major axis, thus increasing their potential to encounter resonances and be delivered to the…”
YORP-induced long-term evolution of the spin state of small asteroids and meteoroids (2002, background): “Implications of this fact in a combined model with their Yarkovsky delivery toward the Earth (e.g., Bottke et al. 2000, Vokrouhlický and Farinella 2000) needs to be studied in the future.”
The Flora Family: A Case of the Dynamically Dispersed Collisional Swarm? (2002, background): “The asteroidal obliquities are usually unknown but believed to be randomly distributed, so that the expected overall statistical trend of an ensemble of initially localized orbits is their dispersion in semimajor axis, with a minor average displacement toward the Sun due to the seasonal effect (Bott”
HED Meteorites and Their Relationship to the Geology of Vesta and the Dawn Mission (2011, background): “Alternatively, these ages could reflect derivation by recent impacts on Vesta itself, because the 10-40 Ma cosmic-ray ages are consistent with orbital evolution from Vesta by the Yarkovsky effect (Bottke et al. 2000).”
Debiased Orbital and Absolute Magnitude Distribution of the Near-Earth Objects (2002, methodology): “In contrast, our results also predict there may be ∼200 kilometer-size Encke-type objects with 2.5 < a < 3.0 AU, many more than the ∼100 predicted by Bottke et al. (2000a).”
Linking the collisional history of the main asteroid belt to its dynamical excitation and depletion (2005, methodology): “For example, Bottke et al. (2000a, 2002b) showed that the inner and central main belt populations (a < 2.8 AU) provide >80% of the observed NEOs, while the outer main belt has removal rates twice as high as the inner main belt (570 H < 18 objects lost per Myr in the outer main belt vs 220 H < 18…”
The fossilized size distribution of the main asteroid belt (2003, background): “If true, the near-Earth object (NEO) populat which is almost entirely replenished by the main belt(Bottke et al., 2000, 2002a, 2002b), should have decayed by factor of ∼3 or more over the last∼3 Gyr (Davis et al., 2002).”
In search of the source of asteroid (101955) Bennu: Applications of the stochastic YORP model (2015, methodology): “This is small enough to be reasonably mobile via the Yarkovsky effect, but not so mobile that it would easily be able to jump across major resonances (e.g., Bottke et al., 2000).”