The twin sister planets Venus and Earth : why are they so different? /: why are they so different?. (2015)
- Record Type:
- Book
- Title:
- The twin sister planets Venus and Earth : why are they so different? /: why are they so different?. (2015)
- Main Title:
- The twin sister planets Venus and Earth : why are they so different?
- Further Information:
- Note: Robert J. Malcuit.
- Authors:
- Malcuit, Robert J
- Contents:
- Preface; Acknowledgements; Contents; Chapter 1; Introduction; 1.1 The Scientific Method; 1.2 Some Special Features of Earth as a Planet; 1.3 Some Special Features of Venus as a Planet; References; Chapter 2; The Origin of the Sun and the Early Evolution of the Solar System; 2.1 List of Some Important Facts to be Explained by a Successful Model; 2.2 A Composite Working Model for Origin and Evolution of the Solar System; Summary; References; Chapter 3; Models for the Origin and Evolution of the Earth-Moon System; 3.1 List of Facts to be Explained by a Successful Model. 3.2 Fission from the Earth Early in Earth History3.3 Co-formation of the Earth and Moon from the Same Cloud of Dust and Gas; 3.4 Intact Capture of the Moon by the Earth (1952-1986); 3.5 Other Recent Attempts at Intact Capture; 3.6 Orbital Traceback Models Suggesting Intact Capture; 3.7 More on the Singer (1968) Model of Prograde Capture; 3.8 Disintegrative Capture Models; 3.9 A Miltiple-Small-Moon Model; 3.10 A New (Post-Kona) View of the Intact Capture Process; 3.11 Formation of the Moon Resulting from a Giant Impact Early in Earth History. 3.11.1 The Angular Momentum Problem of the Earth-Moon System3.11.2 The Oxygen Isotope Similarities Between Earth and Moon; 3.11.3 The Mass and Density of the Moon; 3.12 A Report Card for Models of Lunar Origin; References; Chapter4; A Prograde Gravitational Capture Model for℗ the Origin and Evolution of℗ the℗ Earth-Moon℗ System; 4.1 Place of Origin for Luna and SiblingPreface; Acknowledgements; Contents; Chapter 1; Introduction; 1.1 The Scientific Method; 1.2 Some Special Features of Earth as a Planet; 1.3 Some Special Features of Venus as a Planet; References; Chapter 2; The Origin of the Sun and the Early Evolution of the Solar System; 2.1 List of Some Important Facts to be Explained by a Successful Model; 2.2 A Composite Working Model for Origin and Evolution of the Solar System; Summary; References; Chapter 3; Models for the Origin and Evolution of the Earth-Moon System; 3.1 List of Facts to be Explained by a Successful Model. 3.2 Fission from the Earth Early in Earth History3.3 Co-formation of the Earth and Moon from the Same Cloud of Dust and Gas; 3.4 Intact Capture of the Moon by the Earth (1952-1986); 3.5 Other Recent Attempts at Intact Capture; 3.6 Orbital Traceback Models Suggesting Intact Capture; 3.7 More on the Singer (1968) Model of Prograde Capture; 3.8 Disintegrative Capture Models; 3.9 A Miltiple-Small-Moon Model; 3.10 A New (Post-Kona) View of the Intact Capture Process; 3.11 Formation of the Moon Resulting from a Giant Impact Early in Earth History. 3.11.1 The Angular Momentum Problem of the Earth-Moon System3.11.2 The Oxygen Isotope Similarities Between Earth and Moon; 3.11.3 The Mass and Density of the Moon; 3.12 A Report Card for Models of Lunar Origin; References; Chapter4; A Prograde Gravitational Capture Model for℗ the Origin and Evolution of℗ the℗ Earth-Moon℗ System; 4.1 Place of Origin for Luna and Sibling Planetoids and a Model for Magnetization of the Crust of Luna and Sibling Vulcanoid Planetoids; 4.2 Migration History of Luna and Sibling Vulcanoid Planetoids; 4.2.1 Stability of Vulcanoid Planetoid Orbits. 4.2.2 Transfer of Vulcanoid Planetoids from Orbits of Origin to Venus-Earth Space4.2.3 Summary for the Transfer Scheme; 4.3 Prograde Gravitational Capture of Luna and the Subsequent Orbit Circularization: Two-Body Analysis and a Discussion of theParadoxes Associated with the Capture Process; 4.4 Numerical Simulations of Gravitational Capture of a Lunar-Like Body by an Earth-Like Planet; 4.4.1 Computer Code Information; 4.4.2 Development of the Computer Code; 4.4.3 A Sequence of Typical Orbital Encounter Scenarios Leading to a Stable Capture Scenario. 4.4.4 Geometry of Stable Capture Zones for Planetoids Being Captured by Planets4.4.5 The Post-Capture Orbit Circularization Calculation; 4.4.6 A Qualitative Model for Generation of a Mare-Age Lunar Magnetic Field; 4.4.7 Subsequent Orbit Expansion due to Angular Momentum Exchange between the Rotating Earth and the Lunar Orbit; 4.5 Summary and Statement of the Fourth Paradox; 4.6 Summary and Conclusions for the Chapter; Appendix; References; Chapter5; Some Critical Interpretations and℗ Misinterpretations of Lunar Features; 5.1 Discussion of Some Speculations of Harold Urey and℗ Zdenek Kopal. … (more)
- Publisher Details:
- Cham : Springer
- Publication Date:
- 2015
- Extent:
- 1 online resource (xix, 401 pages), illustrations (some color)
- Subjects:
- 523.4
Earth sciences
Geography
Geochemistry
Planetary science
Geology
Exobiology
SCIENCE -- Astronomy
Exobiology
Geochemistry
Geography
Geology
Planetary science
Earth Sciences
Planetology
Geochemistry
Astrobiology
Geomorphology
Geophysics and Environmental Physics
Science -- Earth Sciences -- General
Science -- Earth Sciences -- Geography
Science -- Geophysics
Geochemistry
UFOs & extraterrestrial beings
Geological surface processes (geomorphology)
Geophysics
Planetology
Astrobiology
Science -- Earth Sciences -- Geology
Solar system: the Sun & planets
Venus (Planet)
Earth (Planet)
Earth (Planet)
Venus (Planet)
Electronic books
Electronic books - Languages:
- English
- ISBNs:
- 9783319113883
3319113887 - Related ISBNs:
- 9783319113876
3319113879 - Notes:
- Note: Includes bibliographical references and indexes.
- Access Rights:
- Legal Deposit; Only available on premises controlled by the deposit library and to one user at any one time; The Legal Deposit Libraries (Non-Print Works) Regulations (UK).
- Access Usage:
- Restricted: Printing from this resource is governed by The Legal Deposit Libraries (Non-Print Works) Regulations (UK) and UK copyright law currently in force.
- View Content:
- Available online (eLD content is only available in our Reading Rooms) ↗
- Physical Locations:
- British Library HMNTS - ELD.DS.371587
- Ingest File:
- 02_351.xml