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• W1493731061 abstract "Context. To investigate the distribution of rotation periods of asteroids from different regions of the Solar System and distribution of diameters of near-Earth asteroids (NEAs). Aims. Verify if nonextensive statistics satisfactorily describes the data. Methods. Light curve data was taken from Planetary Database System (PDS) with Rel $ge 2$. Taxonomic class and region of the Solar System was also considered. Data of NEA were taken from Minor Planet Center. Results. The rotation periods of asteroids follow a $q$-Gaussian with $q=2.6$ regardless of taxonomy, diameter or region of the Solar System of the object. The distribution of rotation periods is influenced by observational bias. The diameters of NEAs are described by a $q$-exponential with $q=1.3$. According to this distribution, there are expected to be $994 pm 30$ NEAs with diameters greater than 1 km." @default.
• W1493731061 created "2016-06-24" @default.
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• W1493731061 date "2012-03-01" @default.
• W1493731061 modified "2023-10-11" @default.
• W1493731061 title "Nonextensive distributions of asteroid rotation periods and diameters" @default.
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• W1493731061 doi "https://doi.org/10.1051/0004-6361/201117767" @default.
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