Hostname: page-component-cd9895bd7-jn8rn Total loading time: 0 Render date: 2024-12-23T14:03:19.788Z Has data issue: false hasContentIssue false
  • English
  • Français

Mapping of the asteroid families

Published online by Cambridge University Press:  03 March 2020

Nataša Todorović
Nataša Todorović*
Affiliation:
Belgrade Astronomical Observatory Volgina 7, P.O.Box 74 11060Belgrade, Serbia email: [email protected]
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

In this work we map one of the most populated regions in the main belt - the asteroid family Themis. Computed with a good choice of parameters, the map enables us to get a refined picture of the dynamics in the family, to reexamine the role of resonances therein, to understand better the distribution of asteroids inside the region and to identify dynamical pathways along which particles can drift away.

Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 14 , Symposium A30: Astronomy in Focus XXX , August 2018 , pp. 17 - 18
Copyright
© International Astronomical Union 2020

References

Froeschlé, Cl ., Lega, E., & Gonczi, R. 1997, CeMDA, 67, 41 CrossRefGoogle Scholar
Hirayama, K. 1918, ApJ, 31, 743 CrossRefGoogle Scholar