Fundamentals of Classical Astrodynamics and Applications
This 2-3 Day course focuses on the fundamental problems and applications of classical astrodynamics.
Overview
This course presents the fundamental principles of classical astrodynamics and applications. It is intended for GNC engineers, spacecraft systems engineers, space mission designers, technical managers, and graduate students, who are interested in a comprehensive introduction to the classical astrodynamics problems, such as the two-body problem, Kepler’s problem, Lambert’s problem, angles-only initial orbit determination problem, circular restricted three-body problem, and orbit perturbations. This course is based on the instructor’s two AIAA textbooks: “Space Vehicle Dynamics and Control (2nd edition, 2008)” and “Space Vehicle Guidance, Control, and Astrodynamics (2015),”with additional new materials on emerging astrodynamical topics. This course will complement AIAA’s other on-demand course: “Fundamentals of Space Vehicle Guidance, Control, and Astrodynamics.”
What You Will Learn
· The fundamentals of classical orbital dynamics and modern computational astrodynamics
· The basic principles of orbital transfer, intercept, and rendezvous guidance problems
· Various astrodynamical methods required for the successful development of advanced space systems and complex space missions
Key Course Topics
· Classical Two-Body Problem
· Kepler’s Problem and Its Solution via Universal Variables
· Lambert’s Problem and its Various Computational Solutions; Lambert Guidance
· Angles-Only Initial Orbit Determination (IOD) Problem and Numerical Examples
· Circular Restricted Three-Body Problem (CR3BP); Lagrange Points; Halo Orbits
· Circular and Elliptical Clohessy-Wiltshir-Hill (CWH) Relative Equations of Motion
· Orbital Transfer, Intercept, and Rendezvous Guidance Problems
· Vinti’s Analytical/Computational Method for J2, J3, and J4 Effects
· Perturbed Orbit Simulation of LEO and GEO Satellites
· Close-Proximity Orbit Simulation around an Irregular-Shaped Asteroid
· See detailed outline below
Who Should Attend
This course is intended for GNC/AOCS engineers and researchers, space mission designers, space systems engineers, and graduate students, who want to enhance their basic understanding of classical astrodynamics. This introductory course focuses on the basic physical concepts and mathematical tools required for the analysis and design of advanced space missions and GNC systems of space vehicles.
Course Information:
Type of Course: Instructor-Led Short Course
Course Level: Intermediate/Advanced
Course Length: 2 or 3 days
AIAA CEU's available: Yes
This course is also available as an on-demand course. Register here.
Lecture 1: Two-Body Problem
1.1 Constants of Two-Body Problem
1.2 Orbit Equation
1.3 Kepler’s Equation
1.4 Classical Orbital Elements
Lecture 2: Kepler’s Problem and Solutions
2.1 Kepler’s Orbit Prediction Problem
2.2 Lagrange’s f and g Functions
2.3 A Universal Variable Formulation of Time-of-Flight (TOF)
2.4 Solution of Kepler’s Problem via Universal Variables
Lecture 3: Lambert’s Problem and Solutions I
3.1 Lambert’s Problem; Lambert Guidance
3.2 Lambert Theorem
3.3 A Classical Solution of Lambert’s Problem
3.4 Gauss/Battin Methods for Lambert’s Problem
Lecture 4: Lambert’s Problem and Solutions II
4.1 Universal Variables Solution of Lambert’s Problem
4.2 Unified Form of TOF by Lancaster and Blanchard
4.3 Improved Solutions by Gooding and Sun
4.4 Asteroid Intercept Mission Design Examples
Lecture 5: Angles-Only Initial Orbit Determination (IOD) Problem
5.1 Lagrange’s Formulation
5.2 Laplace’s Formulation
5.3 Gauss’ Formulation
5.4 Numerical Examples
Lecture 6: Circular Restricted Three-Body (CR3B) Problem
6.1 CR3BP Formulation
6.2 Stability of Lagrange Points
6.3 Halo Orbits
6.4 Sub-L1 Lagrange Halo Orbit for a Solar Sail Mission
Lecture 7: Orbit Perturbations
7.1 Gravitational Potential of an Irregular-Shaped Body
7.2 Perturbed Orbit Simulations of LEO and GEO Satellites
7.3 Close-Proximity Orbits around an Irregular-Shaped Asteroid
7.4 Vinti’s Spheroidal Method for J2, J3, and J4 Effects
Lecture 8: Orbital Transfer, Intercept, and Rendezvous Guidance
8.1 Clohessy-Wiltshir-Hill (CWH) Equations of Motion
8.2 Elliptical CWH Equations
8.3 Orbital Transfer Guidance
8.4 Orbital Intercept and Rendezvous Guidance
AIAA Training Links
For information, group discounts,
and private course pricing, contact:
Lisa Le, Education Specialist (lisal@aiaa.org)