Sameas Fig. 3, but for the best-fit final radar shape model of (85990) 1999 JV6. The X, Y, and Z axes are in kilometres. This model best reproduces the combined light curve and radar data set, with the rotation pole located at λ = 132°, β = −86 °, corresponding to a solution with a χ² within 1% of the best solution from the search depicted in Fig. 6. Combining radar with optical light-curve data provides excellent viewing geometry coverage, meaning more than 99% of the asteroid surface was observed. The red areas represent the surface elements that were not observed by either radar imaging or light curves. The yellow colour marks regions that were not observed by radar but were observed using light curves. The ‘Y-’ view shows an indentation in the largerlobe.