
Future Space Problems and Their Solutions
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Content
- Intro
- Contents
- Foreword
- Preface
- Acknowledgments
- Chapter 1
- Overview of Galactica Application
- 1.1. Introduction
- 1.2. Differential Equations and the Method for Their Solution
- 1.3. The Evolution of the Solar System for 100 Million Years
- 1.4. The Compound Model of the Earth's Rotation
- 1.5. The Compound Model of the Sun's Rotation
- 1.6. The Motion of the Asteroid Apophis
- 1.7. Optimization of Passive Orbit with the Use of Gravity Maneuver
- 1.8. Multilayer Ring Structures
- 1.9. The Free-Access Galactica System
- Conclusion
- Chapter 2
- Optimization of the Mission to the Sun
- 2.1. Introduction
- 2.2. Dependence of Approaching the Sun on the Launching Velocity
- 2.3. Optimal Start for Approaching the Sun
- 2.4. Optimal Gravitational Maneuver for Approaching the Sun
- Conclusion
- Chapter 3
- Multilayer Rotating Structures
- 3.1. Introduction
- 3.2. Statement of the Problem
- 3.3. The Forces Acting between the Bodies
- 3.4. Motion Equations of the Rotating Structure
- 3.5. Solution of the Equations
- 3.6. Examples of Rotating Structures
- 3.7. Stability Problems for Examined Structures and Their Applications
- Conclusion
- Chapter 4
- Dangerous Asteroids and their Possible Use
- 4.1. Introduction
- 4.2. Problem Statement
- 4.3. The Evolution of the Planets' Orbits
- 4.4. Preparation of Initial Data of Asteroids
- 4.5. Apophis's Encounters
- 4.6. Apophis Orbit Evolution
- 4.7. Influence of Initial Conditions
- 4.8. Apophis's Trajectory in the Vicinity of Earth
- 4.9. Possible Use of Asteroid Apophis
- 4.10. Asteroid 1950 DA Approaches the Earth
- 4.11. Evolution of the 1950 DA Orbit
- 4.12. The Trajectory of the 1950 DA in the Encounter Epoch
- 4.13. The Asteroid 1950 DA and Earthbound Satellite
- 4.14. Discussion
- Conclusion
- Chapter 5
- The Mercury's Perihelion Precession
- 5.1. Introduction
- 5.2. Observed Motion of the Vernal Equinox
- 5.3. The Relative Velocity of the Perihelion on the Observations
- 5.4. Absolute Velocity of the Perihelion on Observations
- 5.5. Computing Mercury's Perihelion Precession
- 5.5.1. Gravitational Tugs of the Other Planets
- 5.5.2. Influence of Finite Propagation Speed of Gravity
- 5.5.3. The Precession of the Perihelion under Action of the Sun
- 5.5.4. The Compound Models of the Sun's Oblateness
- 5.6. New Sources of the Mercury's Perihelion Precession
- Conclusion
- Chapter 6
- The Main Problems of Long-Term Climate Change
- 6.1. Introduction
- 6.2. The Theory of the Earth's Insolation
- 6.3. The Disadvantages of the Previous Theories
- 6.4. The Solution for the Orbital Problem
- 6.5. The Research into the Rotational Motion
- 6.6. The Compound Model of the Rotational Motion of the Earth
- Conclusion
- Chapter 7
- The Astronomical Theory of Climate Change
- 7.1. Introduction
- 7.2. Geometric Characteristics of Insolation
- 7.3. Insolation of the Earth
- 7.4. Evolution of Orbital Motion
- 7.5. Evolution of the Rotational Motion of the Earth
- 7.6. Evolution of Insolation
- 7.7. Checking Reliability of the Earth Rotation Problem Solution
- Conclusion
- Chapter 8
- New Insolation and Paleoclimate of West Siberia
- 8.1. Introduction
- 8.2. Evolution of Obliquity and Insolation at 65 N
- 8.3. Latitudinal Change in Insolation
- 8.4. Evolution of Insolation in Other Latitudes
- 8.5. Insolation and the Most Recent Glaciations in West Siberia
- 8.5.1. The Most Significant Recent Glaciation
- 8.5.2. The Last Glacial Maximum
- 8.5.3. Warm Interglacial
- 8.5.4. Optimum Insolation in the Holocene
- 8.6. Insolation Periods of Climate Change
- 8.7. Insolation Periods and Paleoclimate Classifications
- Chapter 9
- Space Mechanics and Future Mankind Progress
- 9.1. Introduction
- 9.2. Axisymmetric Interactions of N-Bodies
- 9.3. Multilayer Rotating Structures of N-Bodies
- 9.4. 3-D Structures of N Bodies
- 9.5. Simulation of Globular Star Clusters
- 9.6. Formation of the Future Habitat for Mankind
- 9.7. Discussion
- Reviewer's General Comments:
- Reviewer's Specific Comments:
- Author's Response to Reviewer's Report
- Answers to the Particular Comments
- Answers to the Major Comments
- Conclusion
- Chapter 10
- The Manual of the Galactica System
- 10.1. Introduction
- 10.2. Essentials of Galactica
- 10.3. Differential Equations of Motion
- 10.4. Solution Method
- 10.5. Input File galacf26.dat
- 10.5.1. General Description
- 10.5.2. Interaction Region Parameters
- 10.5.3. General Problem Solution Parameters
- 10.5.4. Parameters for the Output of Trajectories
- 10.5.5. On-Screen Display Parameters
- 10.6. Initial Condition and Integration Data Files
- 10.7. Trajectory Files 1t, 2t. . .Traekt.Prn
- 10.8. Close-Approach File Dice.Dat
- 10.9. On-Screen Display
- 10.10. Examples of Input Files Galacf26.Dat
- 10.11. Initial Condition Files for Several Solved Problems
- 10.12. Executable Files
- 10.13. Generation of Initial Condition File
- 10.14. Problem-Solving Procedure
- Conclusion
- Appendices
- Appendix 1. Example of MathCad Program for Generating an Initial Condition File
- Appendix 2. Modes of Display in the Standard Graphics of FORTRAN
- Appendix 3. Text of the Galactica Program
- References
- Author Contact Information
- Subject Index
- Index of Authors
- Blank Page
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