Skip to main content
Fig. 18 | Progress in Earth and Planetary Science

Fig. 18

From: Asteroid Ryugu before the Hayabusa2 encounter

Fig. 18

Close-up on the clast in Fig. 17, showing the bottom of one bed (upper left) with a sharp contact with the top of the succeeding bed (lower right). The mineralogy of the clast is mainly olivine, with Fe-rich olivine being lighter in shade. The highest concentration of light gray, Fe-rich olivine is at the bottom of the bed. Insert image at lower left is a lower mag view of the same area, with the high mag area at the lower left of the insert. Note that the grain size extends down to the micron scale

Back to article page