The composition and origin of the C, P, and D asteroids: Water as a tracer of thermal evolution in the outer belt
- 1 November 1990
- Vol. 88 (1) , 172-192
- https://doi.org/10.1016/0019-1035(90)90184-b
Abstract
No abstract availableKeywords
This publication has 34 references indexed in Scilit:
- An idealized short-period comet model: Surface insolation, H2O flux, dust flux, and mantle evolutionPublished by Elsevier ,2002
- Carbonates and Sulfates in CI Chondrites: Formation by Aqueous Activity on the Parent BodyMeteoritics, 1988
- Organic Matter on Asteroid 130 ElektraScience, 1987
- The nature of c-class asteroids from 3-μm spectrophotometryIcarus, 1985
- The oxygen isotope record in Murchison and other carbonaceous chondritesEarth and Planetary Science Letters, 1984
- Compositional Structure of the Asteroid BeltScience, 1982
- The composition of the Trojan asteroidsNature, 1980
- Dust release and mantle development in cometsThe Astrophysical Journal, 1979
- The low-temperature electrical properties of carbonaceous meteoritesEarth and Planetary Science Letters, 1975
- Surface properties of asteroids: A synthesis of polarimetry, radiometry, and spectrophotometryIcarus, 1975