The possible presence of noise affecting the proper elements of asteroid families (due to several dynamical and also physical effects) influences the reconstruction of the original velocity fields. A noise on eccentricities alone is not sufficient to explain the observed features, and a noise on semimajor axes must also be taken into account. A preliminary quantitative evaluation of these noises on both elements is attempted.

Estimation of ageing of proper elements from the observed structures of asteroid families

PAOLICCHI, PAOLO;
2002-01-01

Abstract

The possible presence of noise affecting the proper elements of asteroid families (due to several dynamical and also physical effects) influences the reconstruction of the original velocity fields. A noise on eccentricities alone is not sufficient to explain the observed features, and a noise on semimajor axes must also be taken into account. A preliminary quantitative evaluation of these noises on both elements is attempted.
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11568/227546
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