A Search for Resonant Structures in the Zodiacal Cloud with COBE DIRBE: The Mars Wake and Jupiter's Trojan Clouds
We searched the COBE DIRBE Sky and Zodi Atlas for a wake of dust trailing Mars and for Trojan dust near Jupiter's L5 Lagrange point. We compare the DIRBE images to a model Mars wake based on the empirical model of Earth's wake as seen by the DIRBE and place a 3-σ upper limit on the fractional overdensity of particles in the Mars wake of 18% of the fractional overdensity trailing Earth. We place a 3-σ upper limit on the effective emitting area of large (10- to 100-μm-diameter) particles trapped at Jupiter's L5 Lagrange point of 6×10^(17) cm^2, assuming that these large dust grains are distributed in space like the Trojan asteroids. We would have detected the Mars wake if the surface area of dust in the wake scaled simply as the mass of the planet times the Poynting–Robertson time scale.
Additional Information© 2000 Academic Press. Received 6 May 1999, Revised 18 October 1999, Available online 25 May 2002. We thank Antonin Bouchez, Eric Gaidos, Peter Goldreich, Renu Malhotra, and Ingrid Mann for helpful discussions, and our referees for their thoughtful comments.
Accepted Version - 0002038.pdf