The invasion of a free floating planet and the number asymmetry of Jupiter Trojans
arXiv:2304.13598 · doi:10.1051/0004-6361/202346223
Abstract
This paper extends our previous study (Li et al. 2023) of the early evolution of Jupiter and its two Trojan swarms by introducing the possible perturbations of a free floating planet (FFP) invading the Solar System. In the framework of the invasion of a FFP, we aim to provide some new scenarios to explain the number asymmetry of the L4 and L5 Jupiter Trojans, and some other observed features. We investigate two different cases: (i) The indirect case, where Jupiter experiences a scattering encounter with the FFP and jumps outwards at a speed that is much higher than that considered in(Li et al. 2023), resulting in a change in the numbers of the L4 (N4) and L5 (N5) Trojans swarms. (ii) The direct case, in which the FFP traverses the L5 region and affects the stability of the local Trojans. In the indirect case, the outward migration of Jupiter can be fast enough to make the L4 islands disappear temporarily, inducing a resonant amplitude increase of the local Trojans. After the migration is over, the L4 Trojans come back to the re-appeared and enlarged islands. As for the L5 islands, they always exist but expand even more considerably. Since the L4 swarm suffers less excitation in the resonant amplitude than the L5 swarm, more L4 Trojans are stable and could survive to the end. In the direct case, the FFP could deplete a considerable fraction of the L5 Trojans, while the L4 Trojans at large distances are not affected and all of them could survive. Both the indirect and direct cases could result in a number ratio of R45=N4/N5~1.6 that can potentially explain the current observations. The latter has the advantage of producing the observed resonant amplitude distribution. For achieving these results, we propose that the FFP should have a mass of at least of a few tens of Earth masses and its orbital inclination is allowed to be as high as 40 degrees.
Accepted for publication in A&A, 13 pages, 7 figures, 5 tables
References in corpus (7)
- The Properties of Jovian Trojan Asteroids Listed in SDSS Moving Object Catalog 3
- A rich population of free-floating planets in the Upper Scorpius young stellar association
- Was Planet 9 captured in the Sun's natal star-forming region?
- Asymmetry in the number of L4 and L5 Jupiter Trojans driven by jumping Jupiter
- The effect of planetary migration on the corotation resonance
- Stability of Jovian Trojans and their collisional families
- Calibration of the angular momenta of the minor planets in the solar system