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Secular evolution of asteroid families: the role of Ceres

Published online by Cambridge University Press:  01 March 2016

Bojan Novaković
Affiliation:
Department of Astronomy, Faculty of Mathematics, University of Belgrade, Studentski trg 16, 11000 Belgrade, Serbia email: bojan@matf.bg.ac.rs
Georgios Tsirvoulis
Affiliation:
Astronomical Observatory, Volgina 7, 11060 Belgrade 38, Serbia
Stefano Marò
Affiliation:
Dipartimento di Matematica, Università di Pisa, Largo B. Pontecorvo 5, 56127 Pisa, Italy
Vladimir Đošović
Affiliation:
Department of Astronomy, Faculty of Mathematics, University of Belgrade, Studentski trg 16, 11000 Belgrade, Serbia email: bojan@matf.bg.ac.rs
Clara Maurel
Affiliation:
Institut Supérieur de l'aéronautique et de l'Espace (ISAE-Supaéro), University of Toulouse, 31055 Toulouse Cedex 4, France
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Abstract

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We consider the role of the dwarf planet Ceres on the secular dynamics of the asteroid main belt. Specifically, we examine the post impact evolution of asteroid families due to the interaction of their members with the linear nodal secular resonance with Ceres. First, we find the location of this resonance and identify which asteroid families are crossed by its path. Next, we summarize our results for three asteroid families, namely (1726) Hoffmeister, (1128) Astrid and (1521) Seinajoki which have irregular distributions of their members in the proper elements space, indicative of the effect of the resonance. We confirm this by performing a set of numerical simulations, showcasing that the perturbing action of Ceres through its linear nodal secular resonance is essential to reproduce the actual shape of the families.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2016 

References

Bottke, W. F., Vokrouhlický, D., Broz, M., Nesvorný, D., & Morbidelli, A. 2001, Science, 294, 1693CrossRefGoogle Scholar
Carruba, V., Burns, J. A., Bottke, W., & Nesvorný, D. 2003, Icarus, 162, 308CrossRefGoogle Scholar
Carruba, V. 2009, MNRAS, 395, 358CrossRefGoogle Scholar
Carry, B. 2012, Planetary and Space Science, 73, 98Google Scholar
Cellino, A., Bus, S. J., Doressoundiram, A., Lazzaro, D. 2002, in: Bottke, W. F. Jr., Cellino, A., Paolicchi, P., & Binzel, R. P. (eds.), Asteroids III (University of Arizona Press) p. 633CrossRefGoogle Scholar
Cellino, A., Dell'Oro, A., & Tedesco, E. F. 2009, Planetary and Space Science, 57, 173CrossRefGoogle Scholar
Cibulková, H., Brož, M., & Benavidez, P. G. 2014, Icarus, 241, 358Google Scholar
Delbó, M. & Tanga, P. 2009, Planetary and Space Science, 57, 259CrossRefGoogle Scholar
Dell'Oro, A. & Cellino, A. 2007, MNRAS, 380, 399CrossRefGoogle Scholar
Durda, D. D., Bottke, W. F., Enke, B. L., Merline, W. J., Asphaug, E., Richardson, D. C., & Leinhardt, Z. M. 2004, Icarus, 170, 243CrossRefGoogle Scholar
Farinella, P., & Vokrouhlicky, D. 1999, Science 283, 1507CrossRefGoogle Scholar
Knežević, Z., Milani, A., Farinella, P., Froeschle, C., & Froeschle, C. 1991, Icarus, 93, 316CrossRefGoogle Scholar
Knežević, Z., & Milani, A. 2000, Celestial Mechanics and Dynamical Astronomy, 78, 17CrossRefGoogle Scholar
Knežević, Z., & Milani, A. 2003, A&A, 403, 1165Google Scholar
Marzari, F., Farinella, P., & Davis, D. R. 1999, Icarus, 142, 63Google Scholar
Masiero, J. R., Mainzer, A. K., Grav, T., et al. 2011, ApJ, 741, 68CrossRefGoogle Scholar
Michel, P., Benz, W., Tanga, P., & Richardson, D. C. 2001, Science, 294, 1696Google Scholar
Milani, A. & Knežević, Z. 1994, Icarus, 107, 219CrossRefGoogle Scholar
Milani, A., Cellino, A., Knežević, Z., Novaković, B., Spoto, F., & Paolicchi, P. 2014, Icarus, 239, 46Google Scholar
MilićŽitnik, I. Žitnik, I. & Novaković, B. 2015, MNRAS, 451, 2109CrossRefGoogle Scholar
Nesvorný, D., Morbidelli, A., Vokrouhlický, D., Bottke, W. F., & Brož, M. 2002. Icarus, 157, 155CrossRefGoogle Scholar
Novaković, B. 2010, MNRAS, 407, 1477Google Scholar
Novaković, B., Tsiganis, K., & Knežević, Z. 2010a, MNRAS, 402, 1263CrossRefGoogle Scholar
Novaković, B., Tsiganis, K., & Knežević, Z. 2010b, Celestial Mechanics and Dynamical Astronomy, 107, 35CrossRefGoogle Scholar
Novaković, B., Maurel, C., Tsirvoulis, G., & Knežević, Z. 2015, ApJ, 807, L5.CrossRefGoogle Scholar
Spoto, F., Milani, A., & Knežević, Z. 2015, Icarus, 257, 275Google Scholar
Vernazza, P., Binzel, R. P., Rossi, A., Fulchignoni, M., & Birlan, M. 2009, Nature 458, 993CrossRefGoogle Scholar
Vokrouhlický, D. 1998, A&A, 335, 1093Google Scholar
Vokrouhlický, D. 1999, A&A, 344, 362Google Scholar