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920923s1992 nyua b 001 0 eng |
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|a 523.2
|2 20
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| 100 |
1 |
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|a Taylor, Stuart Ross,
|d 1925-
|0 http://id.loc.gov/authorities/names/n82020430
|1 http://viaf.org/viaf/108589885
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| 245 |
1 |
0 |
|a Solar system evolution :
|b a new perspective : an inquiry into the chemical composition, origin, and evolution of the solar system /
|c Stuart Ross Taylor.
|
| 260 |
|
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|a New York :
|b Cambridge University Press,
|c 1992.
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| 263 |
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|a 9209
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| 300 |
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|a xvi, 307 p. :
|b ill. ;
|c 26 cm.
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| 336 |
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|a text
|b txt
|2 rdacontent
|0 http://id.loc.gov/vocabulary/contentTypes/txt
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|a unmediated
|b n
|2 rdamedia
|0 http://id.loc.gov/vocabulary/mediaTypes/n
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|a volume
|b nc
|2 rdacarrier
|0 http://id.loc.gov/vocabulary/carriers/nc
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| 504 |
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|a Includes bibliographical references and index.
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| 505 |
0 |
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|g Ch. 1.
|t Planetary Formation: A Historical Perspective.
|g 1.1.
|t The Nature of the Problem.
|g 1.2.
|t Pre-Copernican Views and the Copernican Revolution.
|g 1.3.
|t Tidal Theories.
|g 1.4.
|t Solar Accretion Theories.
|g 1.5.
|t Nebular Theories.
|g 1.6.
|t Titius-Bode Rule.
|g 1.7.
|t Giant Gaseous Protoplanets.
|g 1.8.
|t Differences Between Inner and Outer Planets.
|g 1.9.
|t Formation of the Giant Planets.
|g 1.10.
|t Accretion from Dust or from a Hierarchy of Objects.
|g 1.11.
|t Planetesimals.
|g 1.12.
|t Fractionation in Precursor Planetesimals.
|g 1.13.
|t Accretion of Planetesimals.
|g 1.14.
|t An Accretionary Sequence --
|g Ch. 2.
|t The Solar Nebula.
|g 2.1.
|t The Initial Concept.
|g 2.2.
|t The Origin of the Universe.
|g 2.3.
|t Big Bang Scenarios and Element Synthesis.
|g 2.4.
|t The Scale and Structure of the Universe.
|g 2.5.
|t Galaxies.
|g 2.6.
|t Molecular Clouds and Interstellar Dust.
|g 2.7.
|t Separation of Nebulae.
|g 2.8.
|t Dust Disks Around Stars.
|g 2.9.
|t Nebular Collapse, Nebular Lifetime, and Angular Momentum Transfer.
|g 2.10.
|t Star Formation and Evolution.
|g 2.11.
|t Early Violent Stellar Activity: T Tauri and FU Orionis Stars.
|g 2.12.
|t The Formation and Composition of the Sun.
|g 2.13.
|t Massive vs. Small Nebulae.
|g 2.14.
|t Nebular Structure and Temperature.
|g 2.15.
|t Nebular Composition: CI Chondrites and Comets as Samples.
|g 2.16.
|t The Noble Gases.
|g 2.17.
|t Volatile Elements (C, H, O, N) and Nebular Chemistry.
|g 2.18.
|t Homogeneity or Heterogeneity?
|g 2.19.
|t Heliocentric and Vertical Zoning.
|g 2.20.
|t Asteroid Belt Zonation.
|g 2.21.
|t Gas Loss from the Inner Nebula.
|g 2.22.
|t Volatile Element Depletion in the Early Nebula --
|g Ch. 3.
|t The Meteorite Evidence.
|g 3.1.
|t The Most Ancient Samples.
|g 3.2.
|t Presolar Material.
|g 3.3.
|t Refractory or Calcium-Aluminum Inclusions (CAIs).
|g 3.4.
|t Matrix.
|g 3.5.
|t Chondrules.
|g 3.6.
|t Chondrites and Other Primitive Meteorites.
|g 3.7.
|t Chronology.
|g 3.8.
|t Composition of the Nebula.
|g 3.9.
|t "Condensation Sequence"
|g 3.10.
|t Comets.
|g 3.11.
|t Asteroidal and Cometary Dust.
|g 3.12.
|t Fractionated Meteorites and Parent Bodies.
|g 3.13.
|t The Asteroid Belt as a Source.
|g 3.14.
|t Meteorites as Planetary Building Blocks --
|g Ch. 4.
|t The Role of Impacts.
|g 4.1.
|t A Reluctant Conversion.
|g 4.2.
|t Surface Histories of the Planets and Satellites.
|g 4.3.
|t Effects of Cratering.
|g 4.4.
|t Impacts and Planetary Obliquities.
|g 4.5.
|t Formation of Planetary Nebular Disks.
|g 4.6.
|t Addition and Removal of Planetary Atmospheres.
|g 4.7.
|t Lunar Cratering and Origin.
|g 4.8.
|t Mercury.
|g 4.9.
|t The Early Intense Bombardment.
|g 4.10.
|t Large Impact Basins.
|g 4.11.
|t Lunar Cataclysms?
|g 4.12.
|t Early Cratering Flux on the Terrestrial Planets.
|g 4.13.
|t Early Cratering Flux in the Outer Solar System.
|g 4.14.
|t The Impactor Population in the Early Solar System.
|g 4.15.
|t Cratering Flux since the Heavy Bombardment.
|g 4.16.
|t Effects on Biological Evolution.
|g 4.17.
|t Large Collisions and Planetary Accretion: A Summary --
|g Ch. 5.
|t The Planets.
|g 5.1.
|t A Difficult Task.
|g 5.2.
|t Giant and Terrestrial Planets.
|g 5.3.
|t Mercury.
|g 5.4.
|t Venus.
|g 5.5.
|t Earth.
|g 5.6.
|t Mars.
|g 5.7.
|t Compositional Differences Among the Terrestrial Planets and Meteorites.
|g 5.8.
|t Core-Mantle Relationships.
|g 5.9.
|t Crystal Development on the Terrestrial Planets.
|g 5.10.
|t Terrestrial Planetary Atmospheres and Hydrospheres.
|g 5.11.
|t The Asteroid Belt.
|g 5.12.
|t The Giant Planets.
|g 5.13.
|t Planet X.
|g 5.14.
|t The Long-term Stability of the Solar System --
|g Ch. 6.
|t Rings and Satellites.
|g 6.1.
|t Miniature Solar Systems?
|g 6.2.
|t Planetary Subnebulae.
|g 6.3.
|t Ring Systems.
|g 6.4.
|t Satellite Classification.
|g 6.5.
|t Regular Satellites.
|g 6.6.
|t Captured Satellites: Phobos and Deimos.
|g 6.7.
|t Galilean Satellites I: Io and Volcanism.
|g 6.8.
|t Galilean Satellites II: Ganymede and Planetary Expansion.
|g 6.9.
|t Galilean Satellites III: Europa and Callisto.
|g 6.10.
|t Saturnian Satellites.
|g 6.11.
|t Titan.
|g 6.12.
|t Uranian Satellites.
|g 6.13.
|t Triton, Nereid, and the Other Neptunian Satellites.
|g 6.14.
|t Pluto and Charon.
|g 6.15.
|t The Moon.
|g 6.16.
|t Evolution of the Moon.
|g 6.17.
|t Hypotheses of Lunar Origin.
|g 6.18.
|t Large Impact Model for the Origin of the Moon --
|g Ch. 7.
|t The New Solar System.
|g 7.1.
|t The End of Clockwork Solar Systems.
|g 7.2.
|t The Collapse of Grand Unified Theories.
|g 7.3.
|t Our Present Understanding.
|
| 650 |
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|a Cosmochemistry
|0 http://id.loc.gov/authorities/subjects/sh85033157
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| 651 |
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|a Solar system
|0 http://id.loc.gov/authorities/names/n83826333
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| 651 |
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|a Solar system
|x Origin
|0 http://id.loc.gov/authorities/subjects/sh85124548
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| 650 |
|
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|a Cosmochemistry.
|2 fast
|0 http://id.worldcat.org/fast/fst00880582
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| 650 |
|
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|a Origin of the Solar system.
|2 fast
|0 http://id.worldcat.org/fast/fst01353926
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| 651 |
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|a Solar system.
|2 fast
|0 http://id.worldcat.org/fast/fst01244288
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| 928 |
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