Radiative Spin-up and Spin-down of Small Asteroids

By D. Rubincam. 2000

604 citations recorded by the source corpus.

View Paper: https://www.semanticscholar.org/paper/e14267632cedb28a59bc53f802cb49f19cd9aab6

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In Astronomy and Astrophysics

Citations in the corpus

Extreme sensitivity of the YORP effect to small-scale topography (2009, background): “This impliesthat a YORP cycle (Rubincam, 2000) can be interrupted in a major way by a comparatively minor event, and suggests that the spin evolution of small NEOs may be more stochastic than previously recognized.”
Linking the collisional history of the main asteroid belt to its dynamical excitation and depletion (2005, background): “They included factors such as collisional disruption, collisional spin axis reorientation events, and the effects of YORP (Rubincam, 2000; see also, Bottke et al., 2002a).”
The fossilized size distribution of the main asteroid belt (2003, background): “examined nearly 400 asteroids with D > 50 km, a size range where the thermal spin up/down mechanism (YORP) is not expected to significantly modify asteroid spin rates (Rubincam, 2000; Vokrouhlický and Čapek, 2002).”
Yarkovsky/YORP chronology of asteroid families (2006, background): “Vokrouhlický et al. estimated from these results that the Koronis family was likely ∼2.5 Gyr, in agreement with the cratering record observed on Ida (e.g., Chapman, 2002) and the large dynamical spread of the family (e.g., Bottke et al., 2001).”
The YORP effect with finite thermal conductivity (2004, methodology): “…both detections would fairly well constrain asteroi mass and surface thermal properties in an uncorrelated All previous studies of the YORP effect(Rubincam, 2000; Vokrouhlický anďCapek, 2002), including this paper assumed principal axis rotation and rigid shape of the b These assumptions are…”
The Strange Case of 133P/Elst-Pizarro: A Comet among the Asteroids (2004, background): “Rubincam (2000) estimates that the timescale for the YORP effect to significantly alter the spin state of a kilometer-scale body ranges from 106 to 108 yr, depending on the shape, size, and location of the body.”
Thermal inertia of near-Earth asteroids and implications for the magnitude of the Yarkovsky effect (2007, methodology): “This mechanism was named by Rubincam (2000) as the Yarkovsky-O’Keefe-Radzievskii-Paddack effect, or YORP for short.”
Fast and Slow Rotation of Asteroids (2000, background): “…include that (1) slow rotato extinct comet nuclei that were slowed by outgassing proces (2) they are binary objects which have been tidally modified, as Earth’s Moon has slowed Earth’s spin rate; or (3) their sp have been modified by a radiation pressure effect, called YO effect (Rubincam 2000).”
YORP-induced long-term evolution of the spin state of small asteroids and meteoroids (2002, methodology): “Following Rubincam (2000) we shall thus assume effectively immediate thermal reemission of the absorbed energy.”
Rubble Pile Asteroids (2018, neutral): “Bottke WF. Jr., Vokrouhlický D, Rubincam DP, Broz M. 2002a.”
Effects of thermal radiation on the dynamics of binary NEAs (2004, methodology): “More recently, a related effect, usually referred to as YORP (Rubincam, 2000; Vokrouhlický and Čapek, 2002), has been discovered to affect an asteroid’s rotation.”
THE YARKOVSKY AND YORP EFFECTS: Implications for Asteroid Dynamics (2006, background): “…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).”