Nebular thermal evolution and the properties of primitive planetary materials

Meteoritics and Planetary Science

Volumn 36, Issue 5, 2001, Pages 671-700

  Cassen, P ^a  

^a NASA AMES RESEARCH CENTER   (United States)

Author keywords

[No Author keywords available]

Indexed keywords

PLANETARY EVOLUTION; THERMAL EVOLUTION;

EID: 0034969697     PISSN: 10869379     EISSN: None     Source Type: Journal    
DOI: 10.1111/j.1945-5100.2001.tb01908.x     Document Type: Article

References (81)

1. Simulation of chemical reactions and dust destruction in protoplanetary accretion disks
2. Reprocessing in luminous disks
3. The structure and appearance of protostellar accretion disks: Limits on disk flaring
4. 3D solar nebula models: Implications for earth origin
5. Physics of the primitive solar nebula and of giant gaseous protoplanets
6. Why convective heat transport in the solar nebula was inefficient
7. Utilitarian models of the primitive solar nebula
8. Nebula models for the fractionation of moderately volatile elements
9. N-body simulations of planet formation: Varying the initial number of planetary embryos
10. Making the terrestrial planets: N-body integrations of planetary embryos in three dimensions
11. Oxygen isotopes in meteorites
12. The oxygen isotope record in Murchison and other carbonaceous chondrites
13. A component of primitive nuclear composition in carbonaceous meteorites
14. Oxygen isotopic studies of ordinary chondrites
15. Turbulence, chondrules, and planetesimals
16. Distribution and evolution of water ice in the solar nebula: Implications for solar system body formation
17. Accretion disks around young objects. 1. The detailed vertical structure
18. Structure and transport in the solar nebula from constraints and deuterium enrichment and giant planets formation
19. Differential rotation as a source of angular momentum transfer in the solar nebula
20. The dust subdisk in the protoplanetary nebula
21. Destruction processes for dust in protoplanetary accretion disks
22. Condensation in dust-enriched systems
23. Evidence for oxidizing conditions in the solar nebula from Mo and W depletions in refractory inclusions in carbonaceous chondrites
24. Chemical reactions in protoplanetary accretion disks III. The role of ionisation process
25. Chemical reactions in protoplanetary accretion disks II. Carbon dust oxidation
26. Chemical reactions in protoplanetary accretion disks IV. Multicomponent dust mixture
27. Chemical fractionations of chondrites: Signatures of events before chondrule formation
28. Accretion and the evolution of T Tauri disks
29. Dust opacities for protoplanetary accretion disks - Influence of dust aggregates
30. 16O excesses in olivine inclusions Yamamoto-89009 and Murchison chondrites and their relation to CAIs
31. Processes determining the volatile abundances of the meteorites and terrestrial planets
32. Potassium isotope cosmochemistry: Genetic implications of volatile element depletion
33. Pre-main sequence evolution in the Taurus-Auriga molecular cloud
34. Meteoritical and astrophysical constraints on the oxidation state of the solar nebula
35. The cosmoclassification of the elements
36. Chemical fractionations in meteorites-II. Abundance patterns and their interpretations
37. Protostellar cosmic rays and extinct radioactives in meteorites
38. The oxygen isotopic composition of olivine and pyroxene from CI chondrites
39. Oxygen isotope geochemistry of olivine from carbonaceous chondrites
40. The temperature gradient in the solar nebula
41. On the dynamical origin of the solar system
42. Timescales for planetary accretion and the structure of the protoplanetary disk
43. The outer solar system: Chemical constraints at low temperatures on planet formation
44. The evolution of viscous discs and the origin of the nebular variables
45. Oxygen isotopic abundances in calcium-aluminum-rich inclusions from ordinary chondrites: Implications for nebular heterogeniety
46. Physics and chemistry in the primitive solar nebula
47. Protoplanetary accretion discs with coagulation and evaporation
48. Protoplanetary accretion disc models: The effects of several meteoritic, astronomical, and physical constraints
49. Dynamical and chemical evolution of the protoplanetary nebula
50. Settling and growth of dust particles in a laminar phase of a low-mass solar nebula
51. Presolar oxide grains in meteorites
52. A low-temperature origin for the planetesimals that formed Jupiter
53. Moderately volatile elements
54. The condensation origin of zoned metal grains in QUE94411: Implications for the formation of bencubbin/ch-like chondrites (abstract)
55. Theoretical, observational and isotopic estimates of the lifetime of the solar nebula
56. Optical properties of grains in molecular clouds and accretion disks
57. The dynamical evolution of the protosolar nebula
58. 26Al in the solar nebula and constraints on nebula timescales
59. Oxygen-isotopic compositions of calcium-aluminum-rich inclusions and chondrules: Evidence for dust-gas fractionation prior to nebular condensation
60. Black holes in binary systems. Observational appearance
61. Toward an astrophysical theory of chondrites
62. X-rays and fluctuating x-winds from protostars
63. Global evolution of solid matter in turbulent protoplanetary disks. I. Aerodynamics of solid particles
64. Global evolution of solid matter in turbulent protoplanetary disks. II. Development of icy planetesimals
65. Rapid formation of Jupiter by diffusive redistribution of water vapor in the solar nebula
66. Evolutionary timescales for circumstellar disks associated with intermediate and solar-type stars
67. Tidal interaction between a planet and a three-dimensional gaseous disk
68. The formation of Uranus and Neptune in the Jupiter-Saturn region
69. X-ray sources in regions of star formation. III. Naked T Tauri stars associated with the Taurus-Auriga complex
70. Density waves in the solar nebula: Differential Lindblad torque
71. Protoplanet migration by nebula tides
72. Fractionation of moderately volatile elements in ordinary chondrites
73. Aerodynamics of solid bodies in the solar nebula
74. Formation of planetesimals in the solar nebula
75. An alternative model for the formation of the asteroids
76. The formation and habitability of extra-solar planets
77. The solar-oxygen isotopic composition: Predictions and implications for solar nebula processes
78. Olivine and pyroxene compositions in Type II carbonaceous chondrites
79. Mineral equilibrium in fractionated nebular systems
80. Astronomical constraints on nebular temperatures: Implications for planetesimal formation
81. Oxygen reservoirs in the early solar nebula inferred from an Allende CAI