Orbital Mechanics, Second Edition
by
John E. Prussing
and
Bruce A. Conway
Oxford University Press
2013
Contents
Chapter 1 The n - Body Problem
1.1 Introduction, 1
1.2 Equations of Motion for the n - Body Problem, 4
1.3 Justification of the Two-Body Model, 8
1.4 The Two-Body Problem, 11
1.5 The Elliptic Orbit, 13
1.6 Parabolic, Hyperbolic, and Rectilinear Orbits, 16
1.7 Energy of the Orbit, 17
References, 20
Problems, 20
Chapter 2 Position in Orbit as a Function of Time
2.1 Introduction, 25
2.2 Position and Time in an Elliptic Orbit, 25
2.3 Solution for the Eccentric Anomaly, 29
2.4 The f and g Functions and Series, 31
2.5 Position versus Time in Hyperbolic and Parabolic Orbits: Universal Variables,
36
References, 41
Problems, 42
Chapter 3 The Orbit in Space
3.1 Introduction, 46
3.2 The Orbital Elements, 46
3.3 Determining the Orbital Elements from r and v , 49
3.4 Velocity Hodographs, 54
Reference, 59
Problems, 59
Chapter 4 The Three-Body Problem
4.1 Introduction, 60
4.2 Stationary Solutions of the Three-Body Problem, 60
4.3 The Circular Restricted Problem, 65
4.4 Surfaces of Zero Velocity, 66
4.5 Stability of the Equilibrium Points, 66
4.6 Periodic Orbits in the Restricted Case, 70
4.7 Invariant Manifolds, 72
4.8 Special Solutions, 75
References, 76
Problems, 77
Chapter 5 Lambert's Problem
5.1 Introduction, 79
5.2 Transfer Orbits Between Specified Points, 79
5.3 Lambert's Theorem, 84
5.4 Properties of the Solutions to Lambert's Equation, 86
5.5 The Terminal Velocity Vectors, 91
5.6 Applications of Lambert's Equation, 94
5.7 Multiple-Revolution Lambert Solutions, 95
References, 99
Problems, 99
Chapter 6 Rocket Dynamics
6.1 Introduction, 101
6.2 The Rocket Equation, 101
6.3 Solution of the Rocket Equation in Field-Free Space, 103
6.4 Solution of the Rocket Equation with External Forces, 107
6.5 Rocket Payloads and Staging, 108
6.6 Optimal Staging, 113
References, 117
Problems, 117
Chapter 7 Impulsive Orbit Transfer
7.1 Introduction, 119
7.2 The Impulsive Thrust Approximation, 119
7.3 Two-Impulse Transfer between Circular Orbits, 121
7.4 The Hohmann Transfer, 123
7.5 Coplanar Extensions of the Hohmann Transfer, 127
7.6 Noncoplanar Extensions of the Hohmann Transfer, 130
7.7 Conditions for Intercept and Rendezvous, 133
References, 135
Problems, 135
Chapter 8 Continuous-Thrust Orbit Transfer
8.1 Introduction, 138
8.2 Equation of Motion, 139
8.3 Propellant Consumption, 139
8.4 Quasi-Circular Orbit Transfer, 142
8.5 The Effects of Nonconstant Mass, 144
8.6 Optimal Quasi-Circular Orbit Transfer, 145
8.7 Constant Radial Thrust Acceleration, 146
8.8 Shifted Circular Orbits, 151
References, 152
Problems, 153
Chapter 9 Interplanetary Mission Analysis
9.1 Introduction, 154
9.2 Sphere of Influence, 154
9.3 Patched Conic Method, 155
9.4 Velocity Change from Circular to Hyperbolic Orbit, 162
9.5 Planetary Flyby (Gravity- Assist) Trajectories, 163
9.6 Flyby Following a Hohmann Transfer, 166
9.7 Gravity-Assist Applications, 171
References, 175
Problems, 175
Chapter 10 Linear Orbit Theory
10.1 Introduction, 179
10.2 Linearization of the Equations of Motion, 179
10.3 The Hill-Clohessy-Wiltshire (CW) Equations, 182
10.4 The Solution of the CW Equations, 184
10.5 Linear Impulsive Rendezvous, 189
10.6 State Transition Matrix for a General Conic Orbit, 192
References, 196
Problems, 196
Chapter 11 Perturbation
11.1 Introduction, 155
11.2 The Perturbation Equations, 155
11.3 Effect of Atmospheric Drag, 164
11.4 Effect of Earth Oblateness, 164
11.5 Effects of Solar-Lunar Attraction, 209
11.6 Effect on the Orbit of the Moon, 214
References, 215
Problems, 215
Chapter 12 Canonical Systems and Lagrange Variational Equations
12.1 Introduction, 219
12.2 Hamilton's Equations, 220
12.3 Canonical Transformations, 220
12.4 Necessary and Sufficient Conditions for a Canonical Transformation, 222
12.5 Generating Functions, 224
12.6 Jacobi's Theorem, 226
12.7 Canonical Equations for the Two-Body Problem, 228
12.8 The Delaunay Variables, 231
12.9 Average Effects of Earth Oblateness Using Delaunay Variables, 232
12.10 Lagrange Equations, 234
References, 235
Problems, 235
Chapter 13 Perturbations Due to Nonspherical Terms in the Earth's Potential
13.1 Introduction, 238
13.2 Effect of the Zonal HArmonic Terms, 239
13.3 Short-Period Variations, 241
13.4 Long-Period Variations, 242
13.5 Variations at O(J22) , 243
13.6 The Potential in Terms of Conventional Elements, 245
13.7 Variations Due to the Tesseral Harmonics, 247
13.8 Resonance of a Near-Geostationary Orbit, 249
References, 251
Problems, 251
Chapter 14 Orbit Determination
14.1 Introduction, 253
14.2 Angles-Only Orbit Determination, 253
14.3 Laplacian Initial Orbit Determination, 255
14.4 Gaussian Initial Orbit Determination, 259
14.5 Orbit Determination from Two Position Vectors, 263
14.6 Differential Correction, 263
References, 267
Problems, 267
Appendix 1 Astronomical Constants, 270
Appendix 2 Physical Characteristics of the Planets, 271
Appendix 3 Elements of the Planetary Orbits, 272
Index, 273
PREFACE
This text takes its title from an elective course at the University
of Illinois at Urbana-Champaign that has been taught to senior undergraduates
and first-year graduate students for the past 42 years. Many of these students
chose aerospace engineering because of their keen interest in space exploration.
For them, the senior-year elective courses, such as orbital mechanics, rocket
propulsion, and spacecraft design, are the reason they came to the university.
We attempt to develop the subject of orbital mechanics starting from the
first principles of Newton's Laws of Motion and the Law of Gravitation.
While it is not unusual in an introductory book to derive Kepler's Laws
of Planetary Motion from Newton's laws, we also derive the other important
results: Lambert's equation, the rocket equation, the hyperbolic gravity-
assist relations, the Hill-Clohessy-Wiltshire equations of relative motion,
the Lagrange perturbation equations,
the three-body equations of motion,
and the Gauss and Laplace methods of
orbit determination, from first principles.
NEW TO THIS EDITION
A considerable amount of new material has been added to this second edition:
A new chapter onthe three-body problem (Chapter 4). Since the
original book was published in 1993, this subject has received much more
attention; the Lagrange points are now being considered
as destinations, and thhe low-energy and periodic orbits in the
system have been used for several space missions.
A new chapter on continuous-thrust transfer (Chapter 8)
recognizes that since teh original publication, low-thrust
electtricx propulsion has now been used for several space
missions, such as Deep Space 1 and Dawn, so familiarity
with the techniques for generating their trajectories
is important.
A new chapter describing canonical systems and the derivation
of the Lagrange variational equations (Chapter 12).
These are advanced topics that appear infew texts but are useful
when the disturbances on a spacecraft are derivable from
a potential function, such as the coomplete earth
gravitational potential, which is now described
in the new Chapter 13.
New sections on multiple-revolution Lambert solutions,
gravity-assist applications, and the state transition matrix
for a general conic orbit.
Many new examples and problems have been added.
This was a suggestion of the book's reviewers to make it
more useful as a text.
These are primarily of the practial type, i.e., where numerical
results are obtained, for there were already
many problems that required derivinig an analytical result.
Note that problems preceded by an asterik are considered
by the authors as being more difficult to solve than
other problems.
J.E.P.
B.A.C.
Urbana, Illinois
February 2012