Issue |
A&A
Volume 449, Number 2, April II 2006
|
|
---|---|---|
Page(s) | 817 - 820 | |
Section | Planets and planetary systems | |
DOI | https://doi.org/10.1051/0004-6361:20054319 | |
Published online | 21 March 2006 |
Dynamical origin of the asteroid (25143) Itokawa: the target of the sample-return Hayabusa space mission
1
Observatoire de la Côte d'Azur, UMR 6202 Cassiopée/CNRS, BP 4229, 06304 Nice Cedex 4, France e-mail: Patrick.Michel@obs-azur.fr
2
Japan Aerospace Exploration Agency, Institute of Space and Astronautical Science, 3-1-1 Yoshinodai, Sagamihara, Kanagawa 229-8510, Japan
Received:
7
October
2005
Accepted:
22
December
2005
Aims.We have studied numerically the origin and dynamical
evolution of the asteroid (25143) Itokawa on which a Japanese space probe landed
and may have collected a sample. The return to Earth is planed in 2010.Methods.To estimate the most probable source of Itokawa, we have used
the most recent model of the Near-Earth Object population, which allows us to relate
the orbital parameters of a NEO to the different identified source regions
of the NEO population.Results.The two source regions that are the
most likely to transport an object to Itokawa's orbit are the
secular resonance in the main belt and at a lower level of probability
the Mars-crosser population. This result is consistent with the
spectral characteristics of Itokowa, identified as S-type, which is
the dominant spectral type of objects in these sources. In a previous study, we
had found that its most likely fate may be an impact with the
Earth on a million year timescale. Here, we show that its
evolution is consistent with the typical evolution of asteroids coming
from the identified source and which are extracted in the Earth-crossing zone
by planetary encounters.Conclusions.We conclude
that Itokawa is a typical NEO, which probably arrived at its orbit from
the main belt through the
channel. It belongs to the most
common spectral-type in the inner Solar System. Therefore, unless this
asteroid had a peculiar collisional history, the data obtained
by the satellite Hayabusa will clarify some properties representative
of the S-type NEO population.
© ESO, 2006
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