D-type asteroids have a very low albedo and a featureless reddish spectrum.[1] It has been suggested that they have a composition of organic-rich silicates, carbon and anhydrous silicates, possibly with water ice in their interiors.[2] D-type asteroids are found in the outer asteroid belt and beyond; examples are 152 Atala, 944 Hidalgo and most Jupiter trojans. It has been suggested that the Tagish Lake meteorite was a fragment from a D-type asteroid, and that the Martian moon Phobos is closely related.[3]
^Fitzsimmons, A.; et al. (February 1994). "A spectroscopic survey of D-type asteroids". Astronomy and Astrophysics. 282 (2): 634–642. Bibcode:1994A&A...282..634F.