Cosmic-ray Exposure Ages of Meteorites and Lunar Rocks and Their Significance

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THE YARKOVSKY AND YORP EFFECTS: Implications for Asteroid Dynamics (2006, background): “…result from this model is that the distribution of accumulated CRE ages in the population of fragments reaching Earth is in reasonable agreement with observations (e.g., Eugster 2003), with the CRE age histograms dependent on the age of the last event capable of dominating the local Earth swarm.”
Ureilitic breccias: clues to the petrologic structure and impact disruption of the ureilite parent asteroid (2004, background): “It is unlikely that this impact was responsible for delivery of ureilites to Earth, since ureilites show young (o35Ma) cosmic ray exposure ages (Eugster, 2003).”
Linking the collisional history of the main asteroid belt to its dynamical excitation and depletion (2005, background): “These values match the cosmic ray exposure ages of stony meteorites (e.g., Eugster, 2003).”
Irradiation Records, Cosmic-Ray Exposure Ages, and Transfer Times of Meteorites (2006, methodology): “…of science experienced remarkable development during the past 50 years and some comprehensive reviews were published (e.g., Anders, 1964; Lal, 1972; Reedy et al., 1983; Caffee et al., 1988; Vogt et al., 1990; Marti and Graf, 1992; Wieler and Graf, 2001; Wieler, 2002a; Herzog, 2003; Eugster, 2003).”