Astronomy and Astrophysics – Astrophysics – Earth and Planetary Astrophysics
Scientific paper
2009-09-02
ApJL 702 (2009), L19-L22
Astronomy and Astrophysics
Astrophysics
Earth and Planetary Astrophysics
5 pages, 4 figures, published in ApJL
Scientific paper
10.1088/0004-637X/702/1/L19
In this Letter, we give new constraints on planet migration. They were obtained under the assumption that Saturn's current obliquity is due to a capture in resonance with Neptune's ascending node. If planet migration is too fast, then Saturn crosses the resonance without being captured and it keeps a small obliquity. This scenario thus gives a lower limit on the migration time scale tau. We found that this boundary depends strongly on Neptune's initial inclination. For two different migration types, we found that tau should be at least greater than 7 Myr. This limit increases rapidly as Neptune's initial inclination decreases from 10 to 1 degree. We also give an algorithm to know if Saturn can be tilted for any migration law.
Boué Gwenaël
Kuchynka Petr
Laskar Jacques
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