Fig. 5From: Asteroid Ryugu before the Hayabusa2 encounterFigure taken from Rodgers et al. (2016) showing the size frequency distribution of the blocks measured on Eros, Itokawa, Phobos, and comet 67P/Churyumov-Gerasimenko (see Rodgers et al. 2016, Fig. 1)Back to article page