The Effect of Yarkovsky Thermal Forces on the Dynamical Evolution of Asteroids and Meteoroids

By William Bottke, David Vokrouhlický, D. Rubincam, M. Brož. 2002

214 citations recorded by the source corpus.

View Paper: https://www.semanticscholar.org/paper/c47e116e477da1e582cb0f972d9f0fb0b72d2a47

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

Citations in the corpus

Near Earth Asteroids with measurable Yarkovsky effect (2012, methodology): “Observations of Small Solar System Bodies with GAIA.”
Mineralogies and source regions of near-Earth asteroids (2013, methodology): “The Bottke et al. (2002a) model determines the probability that an asteroid is derived from one of five primary source regions: the m6 secular resonance with Saturn, the intermediate source Mars-crossing region (IMC), the 3:1 mean motion resonance at 2.5 AU, the outer belt region (OB), and the…”
The Compositional Structure of the Asteroid Belt (2015, methodology): “An important dynamical process affecting the entire Main Asteroid Belt is the Yarkovsky effect (see Bottke et al., 2002a and Bottke et al., 2006).”
Thermal inertia of near-Earth asteroids and implications for the magnitude of the Yarkovsky effect (2007, methodology): “6, rather than the generally assumed D-1 dependence for size-independent thermal inertia.”
The hazard of near-Earth asteroid impacts on earth (2004, background): “, the Yarkovsky Effect, which is a force on a small body due to asymmetric re-radiation of absorbed sunlight on the warmer ‘‘afternoon’’ side of a spinning asteroid [3]).”
Identification and Dynamical Properties of Asteroid Families (2015, methodology): “could be detected in the catalogs of osculatingorbital elements (Marsden, 1980; Bowell et al., 1994), where they should show up as clusters in 5D space of a, e, i, ̟ andΩ. The search in 5D space of the osculating orbital elements can be performed with the HCM method and metricd(2)5 = d 2 + (na)(2)(k”
Density of asteroids (2012, background): “They represent the most direct witnesses of the conditions that reigned in the proto-planetary nebula (Bottke et al., 2002a).”
Rubble Pile Asteroids (2018, background): “…explain this population and Bottke et al. (2002) proposed that a thermal affect similar to the Yarkovsky effect that changes orbits, known as the Yarkovsky-O’Keefe-Radzievskii-Paddack effect, or YORP-effect, might be capable of spinning asteroids to disruption (Rubincam 2000, Bottke et al. 2002).”
Dynamical erosion of the asteroid belt and implications for large impacts in the inner Solar System (2009, background): “10 km) into the terrestrial planet region and are responsible for delivering the majority of terrestrial planet impactors over the last ∼ 3.5 Gy (Bottke et al., 2000, 2002a,b; Strom et al., 2005).”
Hydrated Minerals on Asteroids: The Astronomical Record (2003, background): “Furthermore, given the evolving understanding of meteorite delivery (Bottke et al., 2002), and the realization that the meteorite collection may be dominated by a relatively small number of parent bodies, the finding that some asteroid mineralogies are not represented as meteorites is not as…”