We have investigated the possible role of secular resonances in the dynamical evolution of Trojans during the early phases of the Solar System. According to our previous studies (Marzari and Scholl 1998a, 1998b) a significant population of planetesimals can be captured in Jupiter and Saturn Trojan o
โฆ LIBER โฆ
Trojan orbits in secular resonances
โ Scribed by R. Bien; J. Schubart
- Publisher
- Springer Netherlands
- Year
- 1984
- Tongue
- English
- Weight
- 315 KB
- Volume
- 34
- Category
- Article
- ISSN
- 1572-9478
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We present here a very simple model that could explain the relatively high eccentricities and inclinations observed in the minor planet belt. This model is based upon the sweeping of the secular resonances u6 and u16 through the belt due to the gravitational effect of the dissipation of a primitive