Origin and Evolution of Near-Earth Objects
By A. Morbidelli, William Bottke, C. Froeschlé, Patrick Michel. 2002
144 citations recorded by the source corpus.
View Paper: https://www.semanticscholar.org/paper/5b390642b3e41fb797f4392376e221296fb6d358
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Citations in the corpus
- The rayed crater Zunil and interpretations of small impact craters on Mars (2005, background): “These fects largely control the orbital evolution and SFD of Ear crossing asteroids(Morbidelli et al., 2002), such that near Earth asteroids (NEAs) larger than 1 km (producing cra larger than 10 km) should have a SFD only slightly stee than that in the main belt(Morbidelli and Vokrouhlicky, 2003).”
- THE IMPORTANCE OF SECONDARY CRATERING TO AGE CONSTRAINTS ON PLANETARY SURFACES (2006, background): “These processes affect the orbital evolution and SFD of Earthcrossing asteroids (Morbidelli et al. 2002), such that near-Earth asteroids (NEAs) larger than 1 km (producing craters larger than 10 km) should have a SFD only slightly steeper than that in the main belt (Morbidelli & Vokrouhlicky 2003).”
- Modal mineralogy of CI and CI-like chondrites by X-ray diffraction (2015, background): “In this scenario the CI-like chondrites could be derived from one of the many known C-type near-Earth objects (NEOs) with low perihe-lia orbits such as 3200 Phaethon (Binzel et al., 2002; Morbidelli et al., 2002; Chaumard et al., 2012).”
- Meteoritic parent bodies: Their number and identification (2002, background): “One possibility is that most source bodies are near-Earth asteroids [NEAs; see Morbidelli et al. (2002)] distributed throughout terrestrial space.”
- Observed spectral properties of near-Earth objects: results for population distribution, source regions, and space weathering processes (2004, background): “NEOs are “immigrants” to the inner So lar System with lifetimes of order 106–107 years(Morbidelli et al., 2002a).”
- The significance of meteorite density and porosity (2008, background): “(2006); 14: Neish et al. (2003); 15: Abe et al.”