@macgregor16b; 61 Vir, @marino17). The parent body distributions are therefore giving insights to the possible overall structure of the planetary systems.

HD 95086 is a young (17$\pm$4 Myr, @meshkat13) A8 star that possesses a large infrared excess, indicative of a massive debris disk [@chen12], and a $\sim$5 $M_J$ planet at the projected distance of $\sim$56 AU [@rameau13; @rameau16]. Compared to the Hipparcos catalog, the Gaia DR1 catalog gives a slightly closer distance, 83.8$\pm$1.9 pc [@gaia16], which we adopt throughout the paper. Its disk was marginally resolved by [*Herschel *]{} and found to be inclined at $\sim$25$^{\circ}$ from face-on [@moor13]. Analysis of its detailed infrared SED and re-analysis of the resolved images suggest that the debris structure around HD 95086 is very similar to that of HR 8799: a warm ($\sim$170 K) belt, a cold ($\sim$60 K) disk, and an extended disk halo (up to $\sim$800 AU) [@su15]. Modeling the disk surface brightness distribution at 70 and 160 $\mu$m suggests that the extended emission seen in the far-infrared is largely from the small grains produced by frequent collisions due to dynamical stirring of planetesimals and launched from the system by stellar radiation in the form of a disk halo. Therefore, the 