From Magnitudes to Diameters: The Albedo
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A. Morbidelli; R. Jedicke; W.F. Bottke; P. Michel; E.F. Tedesco
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Article
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2002
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Elsevier Science
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English
⚖ 287 KB
A recently published model of the Near Earth Object (NEO) orbital-magnitude distribution (Bottke et al., 2002, Icarus 156, 399-433.) relies on five intermediate sources for the NEO population: the ν 6 resonance, the 3 : 1 resonance, the outer portion of the main belt (i.e., 2.8-3.5 AU), the Mars-cro