Recalibration of Mariner 10 color image data allows the identification
of distinct color units on the mercurian surface. We analyze these da
ta in terms of opaque mineral abundance, iron content, and soil maturi
ty and find color units consistent with the presence of volcanic depos
its on Mercury's surface. Additionally, materials associated with some
impact craters have been excavated from a layer interpreted to be def
icient in opaque minerals within the crust, possibly analogous to the
lunar anorthosite crust. These observations suggest that Mercury has u
ndergone complex differentiation like the other terrestrial planets an
d the Earth's moon.