YORP-induced long-term evolution of the spin state of small asteroids and meteoroids

By David Vokrouhlický, D. Čapek. 2002

163 citations recorded by the source corpus.

View Paper: https://www.semanticscholar.org/paper/b40cf16799e809d6f358eaf500cf7510f1fcb4da

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In Astronomy and Astrophysics

Citations in the corpus

In search of the source of asteroid (101955) Bennu: Applications of the stochastic YORP model (2015, background): “As an aside, we point out that other endstate obliquities of YORP evolution are possible (e.g., including 90 ; see Vokrouhlický and Čapek, 2002; Scheeres and Mirrahimi, 2008).”
Yarkovsky/YORP chronology of asteroid families (2006, background): “Vokrouhlický and Čapek (2002) and Čapek and Vokrouhlický (2004) estimated that the typical timescale for a so-called “YORP cycle” among ∼5 km objects is ∼300–600 Myr.”
The Effect of Yarkovsky Thermal Forces on the Dynamical Evolution of Asteroids and Meteoroids (2002, background): “For example, Vokrouhlický and ©apek (2002) recently pointed out that the YORP-evolving rotation state may become temporarily locked in one of the resonances between the precession rate and the proper or forced frequencies of the long-term orbital-plane evolution.”
The Strange Case of 133P/Elst-Pizarro: A Comet among the Asteroids (2004, background): “Vokrouhlický & Čapek (2002) report that a Themis-family asteroid with an initial rotational period of Prot 6 hr can spin up to as fast as Prot 4 hr after about 25–35 Myr of YORP evolution before spinning down to Prot > 100 hr after 100 Myr.”
The YORP effect with finite thermal conductivity (2004, methodology): “Capek, 2002 ). On a long-term, YORP can significantly change rotation rate and obliquity of small bodies in the Solar System, driving them toward some asymptotic values.”
THE YARKOVSKY AND YORP EFFECTS: Implications for Asteroid Dynamics (2006, methodology): “…are combined with the related Yarkovsky effect, YORP may help to explain several puzzling issues about the rotational, orbital, and physical parameters of small asteroids ( Bottke et al. 2002b, Rubincam 2000, Rubincam et al. 2002, Vokrouhlický & Čapek 2002, Morbidelli & Vokrouhlický 2003).”
Thermal inertia of near-Earth asteroids and implications for the magnitude of the Yarkovsky effect (2007, background): “The value of the thermal inertia also plays an important role in the YORP effect (Rubincam, 2000; Vokrouhlický and Capek, 2002), which is a torque produced by the thermal radiation emitted by asteroids with irregular shapes causing a slow spin-up/spindown and a change of the spin axis obliquities of”
Rubble Pile Asteroids (2018, background): “The YORP-effect can also alter obliquities, effectively pushing asteroids towards 0 or 180deg obliquities (Vokrouhlicky & Čapek 2002,Čapek and Vokrouhlický 2004).”