Studying the jovian Trojan dust

DE ELÍA, G. C.; BRUNINI, A.

ASTRONOMY AND ASTROPHYSICS

EDP SCIENCES S A

Lugar: Paris; Año: 2010 vol. 512 p. 65 - 77

0004-6361

Aims. 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 anddynamical evolution of the L4 jovian Trojans. This algorithm considers catastrophic collisions and cratering events, includes a dynamicaltreatment that takes the stability and instability zones of the L4 jovian swarm into account, and incorporates the effects of thePoynting-Robertson radiation.Results. From this analysis, we infer that the time evolution of the L4 jovian Trojan dust luminosity has the characteristics of a diffusionprocess, since its current value is fairly insensitive to variations in the initial size distribution. Moreover, our results indicate thatthe current luminosity of the dust in the L4 jovian swarm ranges from ∼3.2 × 10−8 to 3.4 × 10−8 L.Conclusions. From these estimates, we conclude that the current luminosity of the dust in the L4 jovian swarm is comparable to theluminosity of the inner Solar System dust, and, at least, one order of magnitude lower than the luminosity of the outer Solar Systemdust.