D-type asteroid explained

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.

Examples

A list of some of the largest D-type asteroids.

Name of AsteroidClassificationDiameter
(km)
Diameter
method
Minor planet
category
SMASSTholen
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

See also

Notes and References

  1. Jones . Thomas D. . Lebofsky . Larry A. . Lewis . John S. . Marley . Mark S. . 1990-11-01 . The composition and origin of the C, P, and D asteroids: Water as a tracer of thermal evolution in the outer belt . Icarus . 88 . 1 . 172–192 . 10.1016/0019-1035(90)90184-B . 0019-1035.