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Cascade disruption in Rampo family
Published online by Cambridge University Press: 30 May 2022
Abstract
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.
- 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