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Celestial Mechanics
This book presents a treatment of celestial mechanics, integrating numerical methods, geometry, and Newtonian gravitation to model and predict celestial motion. It progresses from mathematical foundations to orbital theory, ephemeris computation, perturbations, and the analysis of planetary systems and binary stars, tightly linking theory with observational astronomy.
- Author
- Jeremy Tatum
- Publisher
- University of Victoria
- Source
- LibreTexts
- License
- CC BY-NC
- Language
- EN
- Category
- Basic Sciences
Contents· 181 sections
- 01: Numerical Methods
- 1.01: Introduction
- 1.02: Numerical Integration
- 1.03: Quadratic Equations
- 1.04: The Solution of f(x) 0
- 1.05: The Solution of Polynomial Equations
- 1.06: Failure of the Newton-Raphson Method
- 1.07: Simultaneous Linear Equations N n
- 1.08: Simultaneous Linear Equations N n
- 1.09: Nonlinear Simultaneous Equations
- 1.10: 1.10-Besselian Interpolation
- 1.11: Fitting a Polynomial to a Set of Points - Lagrange Polynomials and Lagrange Interpolation
- 1.12: Fitting a Least Squares Straight Line to a Set of Observational Points
- 1.13: Fitting a Least Squares Polynomial to a Set of Observational Points
- 1.14: Legendre Polynomials
- 1.15: Gaussian Quadrature - the Algorithm
- 1.16: Gaussian Quadrature - Derivation
- 1.17: Frequently-needed Numerical Procedures
- 02: Conic Sections
- 2.01: The Straight Line
- 2.02: The Ellipse
- 2.03: The Parabola
- 2.04: The Hyperbola
- 2.05: Conic Sections
- 2.06: The General Conic Section
- 2.07: Fitting a Conic Section Through Five Points
- 2.08: Fitting a Conic Section Through n Points
- 03: Plane and Spherical Trigonometry
- 3.01: Introduction
- 3.02: Plane Triangles
- 3.03: Cylindrical and Spherical Coordinates
- 3.04: Velocity and Acceleration Components
- 3.05: Spherical Triangles
- 3.06: Rotation of Axes Two Dimensions
- 3.07: Rotation of Axes Three Dimensions. Eulerian Angles
- 3.08: Trigonometrical Formulas
- 04: Coordinate Geometry in Three Dimensions
- 4.01: Introduction
- 4.02: Planes and Straight Lines
- 4.03: The Ellipsoid
- 4.04: The Paraboloid
- 4.05: The Hyperboloid
- 4.06: The Cylinder
- 4.07: The Cone
- 4.08: The General Second Degree Equation in Three Dimensions
- 4.09: Matrices
- 05: Gravitational Field and Potential
- 5.01: Introduction
- 5.02: Gravitational Field
- 5.03: Newton's Law of Gravitation
- 5.04: The Gravitational Fields of Various Bodies
- 5.4.01: Field of a Point Mass
- 5.4.02: Field on the Axis of a Ring
- 5.4.03: Plane discs
- 5.4.04: Infinite Plane Laminas
- 5.4.05: Hollow Hemisphere
- 5.4.06: Rods
- 5.4.07: Solid Cylinder
- 5.4.08: Hollow Spherical Shell
- 5.4.09: Solid Sphere
- 5.4.10: Bubble Inside a Uniform Solid Sphere
- 5.05: Gauss's Theorem
- 5.06: Calculating Surface Integrals
- 5.07: Potential
- 5.08: The Gravitational Potentials Near Various Bodies
- 5.8.01: Potential Near a Point Mass
- 5.8.02: Potential on the Axis of a Ring
- 5.8.03: Plane Discs
- 5.8.04: Infinite Plane Lamina
- 5.8.05: Hollow Hemisphere
- 5.8.06: Rods
- 5.8.07: Solid Cylinder
- 5.8.08: Hollow Spherical Shell
- 5.8.09: Solid Sphere
- 5.09: Work Required to Assemble a Uniform Sphere
- 5.10: Nabla Gradient and Divergence
- 5.11: Legendre Polynomials
- 5.12: Gravitational Potential of any Massive Body
- 5.13: Pressure at the Centre of a Uniform Sphere
- 06: The Celestial Sphere
- 6.01: Introduction to the Celestial Sphere
- 6.02: Altazimuth Coordinates
- 6.03: Equatorial Coordinates
- 6.04: Conversion Between Equatorial and Altazimuth Coordinates
- 6.05: Ecliptic Coordinates
- 6.06: The Mean Sun
- 6.07: Precession
- 6.08: Nutation
- 6.09: The Length of the Year
- 6.10: Problems
- 6.11: Solutions
- 07: Time
- 08: Planetary Motions
- 8.01: Introduction to Planetary Motions
- 8.02: Opposition Conjunction and Quadrature
- 8.03: Sidereal and Synodic Periods
- 8.04: Direct and Retrograde Motion and Stationary Points
- 09: The Two Body Problem in Two Dimensions
- 9.01: Kepler's Laws
- 9.02: Kepler's Second Law from Conservation of Angular Momentum
- 9.03: Some Functions of the Masses
- 9.04: Kepler's First and Third Laws from Newton's Law of Gravitation
- 9.05: Position in an Elliptic Orbit
- 9.06: Position in a Parabolic Orbit
- 9.07: Position in a Hyperbolic Orbit
- 9.08: Orbital Elements and Velocity Vector
- 9.09: Osculating Elements
- 9.10: Mean Distance in an Elliptic Orbit
- 10: Computation of an Ephemeris
- 10.01: Introduction to an Ephemeris
- 10.02: Elements of an Elliptic Orbit
- 10.03: Some Additional Angles
- 10.04: Elements of a Circular or Near-circular Orbit
- 10.05: Elements of a Parabolic Orbit
- 10.06: Elements of a Hyperbolic Orbit
- 10.07: Calculating the Position of a Comet or Asteroid
- 10.08: Quadrant Problems
- 10.09: Computing an Ephemeris
- 10.10: Orbital Elements and Velocity Vector
- 10.11: Hamiltonian Formulation of the Equations of Motion
- 11: Photographic Astrometry
- 11.01: Introduction to Photographic Astrometry
- 11.02: Standard Coordinates and Plate Constants
- 11.03: Refinements and Corrections
- 11.3.01: Parallaxes of the Comparison Stars
- 11.3.02: Proper Motions of the Comparison Stars
- 11.3.03: Refraction
- 11.3.04: Aberration of Light
- 11.3.05: Optical Distortion
- 11.3.06: Errors Mistakes and Blunders
- 12: CCD Astrometry
- 13: Calculation of Orbital Elements
- 13.01: Introduction to Calculating Orbital Elements
- 13.02: Triangles
- 13.03: Sectors
- 13.04: Kepler's Second Law
- 13.05: Coordinates
- 13.06: Example
- 13.07: Geocentric and Heliocentric Distances - First Attempt
- 13.08: Improved Triangle Ratios
- 13.09: Iterating
- 13.10: Higher-order Approximation
- 13.11: Light-time Correction
- 13.12: Sector-Triangle Ratio
- 13.13: Resuming the Numerical Example
- 13.14: Summary So Far
- 13.15: Calculating the Elementss
- 13.16: Topocentric-Geocentric Correction
- 13.17: Concluding Remarks
- 14: General Perturbation Theory
- 14.01: Introduction to General Perturbation Theory
- 14.02: Contact Transformations and General Perturbation Theory
- 14.03: The Poisson Brackets for the Orbital Elements
- 14.04: Lagrange's Planetary Equations
- 14.05: Motion Around an Oblate Symmetric Top
- 15: Special Perturbations
- 15.01: Introduction
- 15.02: Orbital elements and the position and velocity vector
- 15.03: The equations of motion
- 16: Equivalent Potential and the Restricted Three-Body Problem
- 16.01: Introduction
- 16.02: Motion Under a Central Force
- 16.03: Inverse Square Attractive Force
- 16.04: Hooke's Law
- 16.05: Inverse Fourth Power Force
- 16.06: The Collinear Lagrangian Points
- 16.07: The Equilateral Lagrangian Points
- 17: Visual Binary Stars
- 17.01: Introduction to Visual Binary Stars
- 17.02: Determination of the Apparent Orbit
- 17.03: The Elements of the True Orbit
- 17.04: Determination of the Elements of the True Orbit
- 17.05: Construction of an Ephemeris
- 18: Spectroscopic Binary Stars
- 18.01: Introduction to Spectroscopic Binary Stars
- 18.02: The Velocity Curve from the Elements
- 18.03: Preliminary Elements from the Velocity Curve
- 18.04: Masses
- 18.05: Refinement of the Orbital Elements
- 18.06: Finding the Period
- 18.07: Measuring the Radial Velocity