If a planetary-mass body were present in the asteroid belt, the orbits of the terrestrial planets and those of the giant planets would be more closely coupled. A greater exchange of angular momentum could affect the stability of the terrestrial planets. Moreover, the planet in the asteroid belt coul
A Numerical Survey of Transient Co-orbitals of the Terrestrial Planets
โ Scribed by Apostolos A. Christou
- Publisher
- Elsevier Science
- Year
- 2000
- Tongue
- English
- Weight
- 500 KB
- Volume
- 144
- Category
- Article
- ISSN
- 0019-1035
No coin nor oath required. For personal study only.
โฆ Synopsis
We have investigated numerically the evolution of near-Earth asteroids (3753) Cruithne, (3362) Khufu, 1989 VA, (10563) 1993 WD, and 1994 TF2 that enter the coorbital regions of the Earth or Venus. We show that the coorbital libration modes identified in F. Namouni (1999, Icarus 137, 293-314) and F. Namouni et al. (1999, Phys. Rev. Lett. 83, 2506-2509) are strong enough to survive tens of thousands of years under planetary perturbations in the Solar System. We give a detailed analysis of the nature of libration modes as functions of the argument of perihelion. The effects of close approaches with the coorbiting planet as well as neighboring planets are characterized. Based on these results, we argue for a steady-state flux of objects temporarily captured in coorbital configurations with the planets.
๐ SIMILAR VOLUMES
We have performed N-body simulation on final accretion stage of terrestrial planets, including the effect of damping of eccentricity and inclination caused by tidal interaction with a remnant gas disk. As a result of runway and oligarchic accretion, about 20 Marssized protoplanets would be formed in