Studying the jovian Trojan dust

DE ELÍA, G. C.; BRUNINI, A.

ASTRONOMY AND ASTROPHYSICS

EDP Sciences

Lugar: Les Ulis, Francia; Año: 2009

0004-6361

Aims: In this paper, we analyze the jovian Trojan dust in the L4 swarm.Methods: To do this, we use a modification of the numerical code developed by us and previously applied to the collisional and dynamical evolution of the L4 jovian Trojans. This algorithm considers catastrophic collisions and cratering events, includes a dynamical treatment that takes into account the stability and instability zones of the L4 jovian swarm, and incorporates the effects of the Poynting-Robertson radiation.Results: From this analysis, we infer that the time evolution of the L4 jovian Trojan dust luminosity has characteristics of a diffusion process, since its current value is fairly insensitive to variations in the initial size distribution. Moreover, our results indicate that the current luminosity of the dust in the L4 jovian swarm ranges from ~ 3.2 × 10^{-8} to 3.4 × 10^{-8} Lsol.Conclusions: From such estimates, we conclude that the current luminosity of the dust in the L4 jovian swarm is comparable to the luminosity of the inner Solar System dust, and, at least, one order of magnitude smaller than the luminosity of the outer Solar System dust.