The hydrology of carbonaceous chondrite parent bodies and the evolution of planet progenitors

Philosophical Transactions of the Royal Society A: Mathematical, Physical and Engineering Sciences

Volumn 359, Issue 1787, 2001, Pages 2095-2110

  Young, E D ^a   Bridges, J C ^a   Ash, R ^a   Allegre C ^a   Cassen, P ^a  

^a UNIVERSITY OF CALIFORNIA   (United States)

Author keywords

Carbonaceous chondrites; Early Solar System; Planetesimals; Thermal modelling

Indexed keywords

EID: 34447573619     PISSN: 1364503X     EISSN: None     Source Type: Journal    
DOI: 10.1098/rsta.2001.0900     Document Type: Conference Paper

References (19)

1. Carbonates in CM chondrites: Oxygen isotope geochemistry and implications for alteration of the CM parent body
2. Origin of graphitic carbon pentlandite in matrix olivines in the Allende meteorite
3. The oxygen isotope record in Murchison and other carbonaceous chondrites
4. Distribtuion of the pre-solar component in Allende and other carbonaceous chondrites
5. Modelling of liquid water on CM meteorite parent bodies and implications for amino acid racemization
6. Water and the thermal evolution of carbonaceous chondrite parent bodies
7. Time scale of aqueous activity in the early Solar System
8. Aqueous activity on asteroids: Evidence from carbonaceous chondrites
9. Mineralogical and chemical modification of components in CV3 chondrites: Nebular or asteroidal processing
10. Progressive alteration in CV3 chondrites: More evidence for asteroidal alteration
11. Oxidation during metamorphism of the ordinary chondrites
12. Water migration due to a temperature gradient in frozen soil
13. A model for diagenesis in proto-planetary bodies
14. Oxygen isotopes in separated components of CI and CM meteorites
15. The role of surface tension in microgravity slug flow
16. Early aqueous alteration, explosive disruption, and reprocessing of asteroids
17. Geochromatography on the parent body of the carbonaceous chondrite Ivuna
18. Oxygen reservoirs in the early solar nebula inferred from an Allende CAI
19. Fluid flow in chondrite parent bodies: Deciphering the compositions of planetesimals