D-type asteroids have a very low albedo and a featureless reddish spectrum. It has been suggested that they have a composition of organic-rich silicates, carbon and anhydrous silicates, possibly with water ice in their interiors.[1] 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.
The Nice model suggests that D-type asteroids may have originated in the Kuiper belt. 46 D-type asteroids are known, including: 3552 Don Quixote, 944 Hidalgo, 624 Hektor, and 10199 Chariklo.
A list of some of the largest D-type asteroids.
Name of Asteroid | Classification | Diameter (km) | Diameter method | Minor planet category | ||
---|---|---|---|---|---|---|
SMASS | Tholen | |||||
D | DU | Main-belt asteroid | ||||
D | IRAS | Outer main-belt asteroid | ||||
Xk | D | IRAS | Main-belt asteroid | |||
– | D | IRAS | Main-belt asteroid | |||
– | D | Direct imaging | Jupiter trojan | |||
– | D | IRAS | Outer main-belt asteroid | |||
T | D | IRAS | Main-belt asteroid | |||
– | D | Absmag | Jupiter trojan | |||
– | D | IRAS | Jupiter trojan | |||
– | D | Absmag | Centaur | |||
– | D | IRAS | Jupiter trojan | |||
– | D | IRAS | Outer main-belt asteroid | |||
– | D | IRAS | Jupiter trojan | |||
– | D | IRAS | Outer main-belt asteroid | |||
– | D | IRAS | Outer main-belt asteroid | |||
– | D | IRAS | Outer main-belt asteroid | |||
– | D | IRAS | Outer main-belt asteroid | |||
– | D | IRAS | Jupiter trojan | |||
– | D | IRAS | Outer main-belt asteroid | |||
– | D | IRAS | Jupiter trojan | |||
– | D | IRAS | Jupiter trojan | |||
– | D | IRAS | Jupiter trojan | |||
– | D | IRAS | Outer main-belt asteroid | |||
– | D | IRAS | Outer main-belt asteroid | |||
– | D | IRAS | Jupiter trojan | |||
– | D | IRAS | Jupiter trojan | |||
– | D | IRAS | Jupiter trojan | |||
– | D | IRAS | Jupiter trojan | |||
D | – | n.a. | Centaur |