Abstract
ASTEROID families are groups of objects produced in disruptive collisions of a parent body. Although family members are widely dispersed in real space, they cluster in the parameter space defined by their so-called proper elements, and can thus be distinguished from the background asteroid population1–3. For most asteroids, these parameters are very close to being invariants of motion and families are still apparent billions of years after their formation4'5. But these parameters undergo chaotic diffusion, and in some cases the rate of diffusion might be large enough that a family member exits from the region of proper-element space occupied by the family after a characteristic time which is shorter than the lifetime of the Solar System. In this case, the characteristic time should provide an approximate upper bound to the age of the family. Here we use this 'chaotic chronology' method to estimate the lifetime of the unusually compact Veritas family. Calculations of the evolu-tion of the proper elements of the family show that two members (including the largest, 490 Veritas) wander outside the borders of the family on a timescale of about 50 Myr, indicating that the family has an age of less than this.
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References
Milani, A., Farinella, P. & Knežević, Z. in Interrelations between Physics and Dynamics for Minor Bodies in the Solar System (eds Benest, D. & Froeschlé, C.) 85–132 (Editions Frontières, Gif-sur-Yvette, 1992).
Knežević, Z. & Milani, A. in Asteroids Comets Meteors 1993 (eds Milani, A., Cellino, A. & Di Martino, M.) (Kluwer, Dordrecht, in the press).
Zappalà, V. & Cellino, A. in Asteroids Comets Meteors 1993 (eds Milani, A., Cellino, A. & Di Martino, M.) (Kluwer, Dordrecht, in the press).
Zappalà, V., Cellino, A., Farinella, P. & Milani, A. Astr. J. 107, 772–801 (1994).
Milani, A. & Knežević, Z. Icarus 107, 219–254 (1994).
Milani, A. & Knežević, Z. Celest. Mech. 49, 347–411 (1990).
Milani, A. & Knežević, Z. Icarus 98, 211–232 (1992).
Zappalà, V., Cellino, A., Farinella, P. & Knežević, Z. Astr. J. 100, 2030–2046 (1990).
Poincaré, H. Méthodes Nouvelles de la Méchanique Céleste Vol. 1 (Gauthier-Villars, Paris, 1892).
Poincaré, H. Méthodes Nouvelles de la Méchanique Céleste Vol. 3 (Gauthier-Villars, Paris, 1898).
Arnold, V. I. Russ. math. Sun. 18, 85–191 (1963).
Wisdom, J. Icarus 56, 51–74 (1983).
Milani, A., Carpino, M., Hahn, G. & Nobili, A. M. Icarus 78, 212–269 (1989).
Milani, A. & Nobili, A. M. Nature 357, 569–570 (1992).
Milani, A. Celest. Mech. 57, 59–94 (1993).
Farinella, P. et al. Astr. Astrophys. 217, 298–306 (1989).
Carpino, M., Milani, A. & Nobili, A. M. Astr. Astrophys. 181, 182–194 (1987).
Milani, A. in From Newton to Chaos: Modern Techniques for Understanding and Coping with Chaos in N-Body Dynamical Systems (eds Roy, A. E. & Steves, B. A.) (Plenum, New York, in the press).
Tedesco, E. F. in Asteroids Comets Meteors 1993 (eds Milani, A., Cellino, A. & Di Martino, M.) 463–466 (Kluwer, Dordrecht, 1994).
Tholen, D. J. in Asteroids II (eds Binzel, R. P., Gehrels, T. & Matthews, M. S.) 1139–1150 (Univ. Arizona Press, 1989).
Williams, J. G. in Asteroids II (eds Binzel, R. P., Gehrels, T. & Matthews, M. S.) 1034–1072 (Univ. Arizona Press, 1989).
Lindblad, B. A. in Asteroids, Comets, Meteors 1991 (eds Harris, A. W. & Bowell, E.) 363–366 (Lunar & Planetary, Houston, 1992).
Housen, K. R., Schmidt, R. M. & Holsapple, K. A. Icarus 94, 180–190 (1991).
Farinella, P., Davis, D. R., Paolicchi, P., Cellino, A. & Zappalà, V. Astr. Astrophys. 253, 604–614 (1992).
Farinella, P. & Davis, D. R. Icarus 97, 111–123 (1992).
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Milani, A., Farinella, P. The age of the Veritas asteroid family deduced by chaotic chronology. Nature 370, 40–42 (1994). https://doi.org/10.1038/370040a0
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DOI: https://doi.org/10.1038/370040a0
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