Celestial Mechanics and Astrodynamics: Theory and Practice
- Introduction
- Definitions
- History
- Properties of Conics
- The Ellipse, 0 < e < 1
- The Parabola, e = 1
- The Hyperbola, e > 1
- Astronomical Background
- Stability and Chaos
- Three-Body Problem
- Solar System
- Resonances, Singularities and Regularization
- Stability Determination
- Poincaré Surface of Section
- Hill Stability
- Lyapunov
- Kolmogorov-Arnold-Moser Theorem
- Spacecraft Orbit Stability
- Chaos Determination
- Observational Data
- Transit Circle
- Photographic
- Vectors
- Introduction
- Scalar Product
- Vector Product
- Triple Scalar and Vector Products
- Velocity of Vector
- Rotation of Axes
- Angular Velocity
- Gradient of a Scalar
- Momentum and Energy
- Simple Harmonic Motion
- Linear Motion in an Inverse Square Field
- Foucoult’s Pendulum
- Reference Systems and Relativity
- Reference Systems
- Relativistic Coordinate Systems
- Newtonian Coordinates
- Relativistic Coordinates
- ICRS, BCRS, GCRS
- Geodesic Precession and Nutation
- Reference Frames
- Celestial Reference Frames
- CIP and CIO
- Equation of Equinoxes
- Equation of Origins
- Terrestrial Reference Frames
- Terrestrial Intermediate Origin
- ECEF, ECI, ECR
- Satellite Geodesy
- GNSS Reference Systems
- Time Scales
- Coordinate Systems
- Origins and Planes
- Horizon Reference Frame
- Geocentric Coordinates
- Geodetic Coordinates
- Geographic Coordinates
- Astronomical Coordinates
- Kinematics of the Earth
- Earth Orientation
- Precession
- Nutation
- Polar Motion
- Observation Effects
- Aberration
- Proper Motion
- Radial Velocities
- Parallax
- Refraction
- Relativistic Light Deflection
- Space Motion
- Tidal Effects
- Earth Satellite Equations of Motion in GCRS
- Central Force Motion
- Introduction
- Law of Areas
- Linear and Angular Velocities
- Integrals of Angular Momentum and Energy
- Equation of the Orbit
- Inverse Square Law
- Eccentricity Vector
- From Orbit to Force Law
- Einstein’s Modification of the Orbit Equation
- University of Newton’s Law
- The Two-Body Problem
- Introduction
- Classical Orbital Elements
- Osculating Orbital Elements
- Nonsingular Orbital Elements
- Motion of the Center of Mass
- Relative Motion
- The Integral of Areas
- Elements of the Orbit from Position and Velocity
- Properties of Motion
- The Constant of Gravitation
- Kepler’s Equation
- Series Expansion
- Differential Method
- Position in the Elliptic Orbit
- Position in the Parabolic Orbit
- Position in a Hyperbolic Orbit
- Position on the Celestial Sphere
- Heliocentric Coordinates
- Geocentric Coordinates
- Orbit Determination
- Introduction
- Known Radius Vectors
- Laplace’s Method
- Gauss’s Method
- Lambert’s Theorem
- Parabolic Orbits, Olber’s Method
- Circular Orbits
- The n-Body Problem
- Introduction
- Equations of Motion
- Angular Momentum, or Areal Velocity, Integral
- Integral of Energy
- Stationary Solutions of the Three-Body Problem
- Generalization to n Bodies
- Equations of Relative Motion
- The Restricted Three-Body Problem
- Introduction
- Equations of Motion
- The Jacobi Constant
- Zero Velocity Curves
- The Lagrangian Points
- Stability of Motion Near the Lagrangian Points
- Hill’s Restricted Three-Body Problem
- Equations of Motion
- Hill’s Equations of Motion
- Families of Periodic Orbits
- Numerical Procedures
- Differences and Sums
- Interpolation
- Lagrangian Methods
- Differentiation
- Integration
- Differential Equations
- Errors
- Numerical Integration
- Numerical Integration by Runge-Kutta Methods
- Accumulation of Errors in Numerical Integration
- Numerical Integration of Orbits
- Equations for Cowell’s Method
- Equations for Encke’s Method
- Comparison of Cowell’s and Encke’s Methods
- Equations with Origin at the Center of Mass
- Canonical Equations
- Introduction
- Canonical Form of the Equations
- Eliminating the Time Dependency
- Integral of a System of Canonical Equations
- Canonical Transformation of Variables
- Necessary Condition
- Sufficient Condition
- Examples of Canonical Transformations
- Change of Variables by Means of a Generating Function
- Conjugate Variables to Qj
- Jacobi’s Theorem
- Canonical Equations for the Two-Body Problem
- Application of Jacobi’s Theorem to the Two-body Problem
- Meaning of the Constants a
- Variables Conjugate to Qi
- Application to the General Problem
- The Delaunay Variables
- The Lagrange Equations
- Small Eccentricity and Small Inclination
- Small Eccentricity
- Small Inclination
- Universal Variables
- General Perturbations Theory
- Introduction
- Variation of Parameters**
- Properties of the Lagrange Brackets
- Evaluation of the Lagrange Brackets
- Solution of the Perturbation Equations
- Case I: Radial, Transverse, and Orthogonal Components
- Case II: Tangential, Normal, and Orthogonal Components
- Expansion of the Third-Body Potential
- The Factor (r|r’)2
- The Factor P2.cos phi
- The Earth-Moon System**
- Expansion of the Gravitational Potential
- Atmospheric Drag
- Regularization of Perturbed Motion
- Motion Around Oblate Planets
- Introduction
- Axially-Symmetric Gravitational Field
- Equatorial Motion
- The Orbital Angle and Radial Period**
- New Orbital Elements
- Open Orbits and the Escape Velocity
- Circular Orbits
- The Cid-Lahulla Approach
- Polar-Nodal Coordinates
- The Cid-Lahulla Radial Intermediary**
- Comparison with Brouwer’s Approximation
- Solution for Motion in a Cid-Lahulla Potential**
- Main Steps Towards a Solution**
- New Independent Variable
- Semi analytical Orbit Theory
- Introduction
- Preliminaries
- Semianalytical Models
- The Zonal Part of the Geopotential**
- Second-Order Effects
- The Tesseral-Sectorial Part of the Geopotential
- Atmospheric Drag
- Frozen Orbits
- Sun-synchronous and Repeat Ground-track Orbits
- Geostationary Orbits
- In-Plane Motion
- Out-of-Plane Motion
- Averaged Solution
- The Perturbed Problem**
- Satellite Orbit Control
- Introduction
- Stability and Control of Dynamical Systems
- Impulsive and Continuous Maneuvers
- Gravity Assist Maneuvers
- Multiple Gravity Assists
- Concatenation Rules**
- Optimization of Orbits
- Dynamic Optimization
- Linear Orbit Control**
- Low Earth Orbit Control
- Altitude Correction
- Frozen Orbit Control
- Sun-synchronous Orbit Control
- Repeat Ground-track Orbit Control
- Geostationary Orbit Control
- North-South Stationkeeping
- East-West Stationkeeping
- Eccentricity Correction
- Nonlinear Feedback Control of Orbits**
- Fixed-Magnitude Continuous-Thrust Orbit Control**
- Comparison of Continuous-Thrust Controllers
- Optimal Impulsive Orbit Transfers
- Introduction
- Modified Hohmann Transfer***
- Modified Bi-Elliptic and Bi-Parabolic Transfers
- Definitions
- Modified Bi-Elliptic Transfer
- Calculating Ycrit**
- Evaluating the effect of X on maneuvers where Y =Ycrit
- Extending the evaluation to include all Ycrit < Y
- Modified Bi-Parabolic Transfer
- Comparison Between the Modified Bi-Parabolic and the Modified Hohmann Transfers
- Bi-Elliptic Transfer
- Bi-Parabolic Transfer
- Orbit Data Processing
- Introduction
- Principle of Least Squares
- Least Squares Approximation
- Orthogonal Polynomials
- Chebyshev Series
- Chebyshev Approximation**
- Other Polynomial Approximations
- Fourier Approximation: Continuous Range
- Fourier Approximation: Discrete Range**
- Optimum Polynomial Interpolation
- Chebyshev Interpolation
- Economization of Power Series
- Recursive Filtering
- Mean Elements Estimator
- Initial Conditions and Parameter Values
- Uncontrolled Orbits, Single Run
- Orbits with No Control Inputs, Monte-Carlo Runs
- Impulsive Maneuvers
- Continuous Thrust
- Space Debris
- Introduction
- SGP4 Propagator and TLE
- Sizing the Debris
- Time of Closest Approach
- Probability of Collision
- Calculating the Required v