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Cascade disruption in Rampo family

Published online by Cambridge University Press:  30 May 2022

Mariia Vasileva Open the ORCID record for Mariia Vasileva [Opens in a new window] ,
Eduard Kuznetsov Open the ORCID record for Eduard Kuznetsov [Opens in a new window] ,
Alexey Rosaev Open the ORCID record for Alexey Rosaev [Opens in a new window]  and
Eva Plávalová
Mariia Vasileva
Affiliation:
Department of Astronomy, Geodesy, Ecology and Environmental Monitoring, Ural Federal University, Lenina Avenue, 51, Yekaterinburg, 620000, Russia emails: [email protected], [email protected]
Eduard Kuznetsov
Affiliation:
Department of Astronomy, Geodesy, Ecology and Environmental Monitoring, Ural Federal University, Lenina Avenue, 51, Yekaterinburg, 620000, Russia emails: [email protected], [email protected]
Alexey Rosaev
Affiliation:
Research and Educational Center “Nonlinear Dynamics”, Yaroslavl State University, Yaroslavl, Russia email: [email protected]
Eva Plávalová
Affiliation:
Mathematical Institute of the Slovak Academy of Sciences, Bratislava, Slovakia email: [email protected]
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Abstract

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We have found three new members of the Rampo asteroids family: 2009HD95, 2010VO19, 2013JF69. We estimated the Yarkovsky semimajor axis drift rate. Based on the simulation results, estimates of the asteroid pairs’ age included in the family are obtained. In the scenario of the cascade disruption of the parent body of the asteroid (10321) Rampo, one can note the concentration of estimates of the pairs’ age to values of 900, 750, 500, and 250 kyr.

Keywords

Celestial mechanicsmethods: numericalminor planetsasteroids
Type
Poster Paper
Information
Proceedings of the International Astronomical Union , Volume 15 , Symposium S364: Multi-scale (Time and Mass) Dynamics of Space Objects (Oct 2021) , October 2019 , pp. 262 - 263
Copyright
© The Author(s), 2022. Published by Cambridge University Press on behalf of International Astronomical Union

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