D-type asteroids have a very low albedo and a featureless reddish electromagnetic spectrum.[citation needed] It has been suggested that they have a composition of organic rich silicates, carbon and anhydrous silicates, possibly with water ice in their interiors.[citation needed] D-type asteroids are found in the outer asteroid belt and beyond; examples are 152 Atala, and 944 Hidalgo as well as the majority of Jupiter's Trojans.
The Nice model suggests that D-type asteroids may have originated in the Kuiper belts.[1]
