Secular resonances in the primitive sola
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Anne Lemaitre; Pierre Dubru
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Article
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1991
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Springer Netherlands
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English
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We present here a very simple model that could explain the relatively high eccentricities and inclinations observed in the minor planet belt. This model is based upon the sweeping of the secular resonances u6 and u16 through the belt due to the gravitational effect of the dissipation of a primitive